diff --git a/cs/doublestar/BU_800-AB.md b/cs/doublestar/BU_800-AB.md index 7c78a4d41..3d131845b 100644 --- a/cs/doublestar/BU_800-AB.md +++ b/cs/doublestar/BU_800-AB.md @@ -1,6 +1,6 @@ --- name: BU 800-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-02 11:54:34.273201 diff --git a/cs/doublestar/GRB_34-AB.md b/cs/doublestar/GRB_34-AB.md index 90e0285f2..ec57007d5 100644 --- a/cs/doublestar/GRB_34-AB.md +++ b/cs/doublestar/GRB_34-AB.md @@ -1,6 +1,6 @@ --- name: GRB 34-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-16 12:56:34.322987 diff --git a/cs/doublestar/SKF_1311.md b/cs/doublestar/SKF_1311.md index 50ce76505..98609cc0a 100644 --- a/cs/doublestar/SKF_1311.md +++ b/cs/doublestar/SKF_1311.md @@ -1,6 +1,6 @@ --- name: SKF 1311 -rating: None +rating: references: created_by: David1 created_date: 2023-10-11 11:28:20.614673 diff --git a/cs/doublestar/STF_1424-AB.md b/cs/doublestar/STF_1424-AB.md index b40daa4cb..82f199b16 100644 --- a/cs/doublestar/STF_1424-AB.md +++ b/cs/doublestar/STF_1424-AB.md @@ -1,6 +1,6 @@ --- name: STF 1424-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-03 09:12:28.311440 diff --git a/cs/doublestar/STF_1536-AB.md b/cs/doublestar/STF_1536-AB.md index c18aea482..091a51dde 100644 --- a/cs/doublestar/STF_1536-AB.md +++ b/cs/doublestar/STF_1536-AB.md @@ -1,6 +1,6 @@ --- name: STF 1536-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-03 09:54:19.283384 diff --git a/cs/doublestar/STF_1722.md b/cs/doublestar/STF_1722.md index 5d4f77938..08a113a02 100644 --- a/cs/doublestar/STF_1722.md +++ b/cs/doublestar/STF_1722.md @@ -1,6 +1,6 @@ --- name: STF 1722 -rating: None +rating: references: created_by: David1 created_date: 2023-10-02 11:13:59.166575 diff --git a/cs/doublestar/STF_1877-AB.md b/cs/doublestar/STF_1877-AB.md index 8ba7607ee..55774de09 100644 --- a/cs/doublestar/STF_1877-AB.md +++ b/cs/doublestar/STF_1877-AB.md @@ -1,6 +1,6 @@ --- name: STF 1877-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-05 09:08:50.575999 diff --git a/cs/doublestar/STF_1888-AB.md b/cs/doublestar/STF_1888-AB.md index 9475d2985..e285afd5f 100644 --- a/cs/doublestar/STF_1888-AB.md +++ b/cs/doublestar/STF_1888-AB.md @@ -1,6 +1,6 @@ --- name: STF 1888-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-05 09:23:53.173052 diff --git a/cs/doublestar/STF_1930-AB.md b/cs/doublestar/STF_1930-AB.md index 10bf29137..7e3a3b868 100644 --- a/cs/doublestar/STF_1930-AB.md +++ b/cs/doublestar/STF_1930-AB.md @@ -1,6 +1,6 @@ --- name: STF 1930-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-11 11:06:45.620526 diff --git a/cs/doublestar/STF_1965.md b/cs/doublestar/STF_1965.md index 371d9a86d..c34a051a0 100644 --- a/cs/doublestar/STF_1965.md +++ b/cs/doublestar/STF_1965.md @@ -1,6 +1,6 @@ --- name: STF 1965 -rating: None +rating: references: created_by: David1 created_date: 2023-10-06 09:43:43.501401 diff --git a/cs/doublestar/STF_2032-AB.md b/cs/doublestar/STF_2032-AB.md index d3680879f..8d4862e33 100644 --- a/cs/doublestar/STF_2032-AB.md +++ b/cs/doublestar/STF_2032-AB.md @@ -1,6 +1,6 @@ --- name: STF 2032-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-06 11:00:09.064889 diff --git a/cs/doublestar/STF_2262-AB.md b/cs/doublestar/STF_2262-AB.md index 5af979b75..e50d15e0d 100644 --- a/cs/doublestar/STF_2262-AB.md +++ b/cs/doublestar/STF_2262-AB.md @@ -1,6 +1,6 @@ --- name: STF 2262-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-12 12:20:21.025160 diff --git a/cs/doublestar/STF_2272-AB.md b/cs/doublestar/STF_2272-AB.md index 6c360438a..a12bdcf99 100644 --- a/cs/doublestar/STF_2272-AB.md +++ b/cs/doublestar/STF_2272-AB.md @@ -1,6 +1,6 @@ --- name: STF 2272-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-12 11:23:47.587179 diff --git a/cs/doublestar/STF_2323-AB.md b/cs/doublestar/STF_2323-AB.md index ce963fdea..e1b878531 100644 --- a/cs/doublestar/STF_2323-AB.md +++ b/cs/doublestar/STF_2323-AB.md @@ -1,6 +1,6 @@ --- name: STF 2323-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-09 11:35:47.423010 diff --git a/cs/doublestar/STF_2398-AB.md b/cs/doublestar/STF_2398-AB.md index 528089e9d..f437aa254 100644 --- a/cs/doublestar/STF_2398-AB.md +++ b/cs/doublestar/STF_2398-AB.md @@ -1,6 +1,6 @@ --- name: STF 2398-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-09 12:06:12.240757 diff --git a/cs/doublestar/STF_2576-FG.md b/cs/doublestar/STF_2576-FG.md index 51ef49133..f76dd905a 100644 --- a/cs/doublestar/STF_2576-FG.md +++ b/cs/doublestar/STF_2576-FG.md @@ -1,6 +1,6 @@ --- name: STF 2576-FG -rating: None +rating: references: created_by: David1 created_date: 2023-10-01 17:58:24.381890 diff --git a/cs/doublestar/STF_2579-AB.md b/cs/doublestar/STF_2579-AB.md index 753872668..d9401218a 100644 --- a/cs/doublestar/STF_2579-AB.md +++ b/cs/doublestar/STF_2579-AB.md @@ -1,6 +1,6 @@ --- name: STF 2579-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-01 19:42:00.137806 diff --git a/cs/doublestar/STF_2580-AB.md b/cs/doublestar/STF_2580-AB.md index 6c151cf98..36ae50110 100644 --- a/cs/doublestar/STF_2580-AB.md +++ b/cs/doublestar/STF_2580-AB.md @@ -1,6 +1,6 @@ --- name: STF 2580-AB -rating: None +rating: references: created_by: skybber created_date: 2023-10-01 09:58:01.625572 diff --git a/cs/doublestar/STF_262-AB.md b/cs/doublestar/STF_262-AB.md index a5b720fc2..acfaa88b9 100644 --- a/cs/doublestar/STF_262-AB.md +++ b/cs/doublestar/STF_262-AB.md @@ -1,6 +1,6 @@ --- name: STF 262-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-25 10:31:05.732665 diff --git a/cs/doublestar/STF_3062.md b/cs/doublestar/STF_3062.md index 2886684d9..158bea20d 100644 --- a/cs/doublestar/STF_3062.md +++ b/cs/doublestar/STF_3062.md @@ -1,6 +1,6 @@ --- name: STF 3062 -rating: None +rating: references: created_by: David1 created_date: 2023-10-24 10:56:13.560680 diff --git a/cs/doublestar/STF_60-AB.md b/cs/doublestar/STF_60-AB.md index 66b1f2e8f..cf1312346 100644 --- a/cs/doublestar/STF_60-AB.md +++ b/cs/doublestar/STF_60-AB.md @@ -1,6 +1,6 @@ --- name: STF 60-AB -rating: None +rating: references: created_by: David1 created_date: 2023-10-24 10:52:24.243261 diff --git a/cs/doublestar/STF_79.md b/cs/doublestar/STF_79.md index c8dae3373..eb9c5f137 100644 --- a/cs/doublestar/STF_79.md +++ b/cs/doublestar/STF_79.md @@ -1,6 +1,6 @@ --- name: STF 79 -rating: None +rating: references: created_by: David1 created_date: 2023-10-16 13:14:17.807223 diff --git a/cs/dso/Abell/Abell10.md b/cs/dso/Abell/Abell10.md new file mode 100644 index 000000000..3951c12bc --- /dev/null +++ b/cs/dso/Abell/Abell10.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.518180 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.518183 +--- diff --git a/cs/dso/Abell/Abell12.md b/cs/dso/Abell/Abell12.md new file mode 100644 index 000000000..f7b1308e8 --- /dev/null +++ b/cs/dso/Abell/Abell12.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.521401 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.521403 +--- diff --git a/cs/dso/Abell/Abell13.md b/cs/dso/Abell/Abell13.md new file mode 100644 index 000000000..2b42a15c1 --- /dev/null +++ b/cs/dso/Abell/Abell13.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.560804 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.560806 +--- diff --git a/cs/dso/Abell/Abell14.md b/cs/dso/Abell/Abell14.md new file mode 100644 index 000000000..453d88fc3 --- /dev/null +++ b/cs/dso/Abell/Abell14.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.524535 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.524537 +--- diff --git a/cs/dso/Abell/Abell15.md b/cs/dso/Abell/Abell15.md new file mode 100644 index 000000000..62e0bb270 --- /dev/null +++ b/cs/dso/Abell/Abell15.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.765585 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.765588 +--- diff --git a/cs/dso/Abell/Abell16.md b/cs/dso/Abell/Abell16.md new file mode 100644 index 000000000..a8b7b331e --- /dev/null +++ b/cs/dso/Abell/Abell16.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.629088 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.629090 +--- diff --git a/cs/dso/Abell/Abell18.md b/cs/dso/Abell/Abell18.md new file mode 100644 index 000000000..2bb860840 --- /dev/null +++ b/cs/dso/Abell/Abell18.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.439537 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.439540 +--- diff --git a/cs/dso/Abell/Abell19.md b/cs/dso/Abell/Abell19.md new file mode 100644 index 000000000..c11ac4ab9 --- /dev/null +++ b/cs/dso/Abell/Abell19.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.493747 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.493749 +--- diff --git a/cs/dso/Abell/Abell20.md b/cs/dso/Abell/Abell20.md new file mode 100644 index 000000000..b47a4d380 --- /dev/null +++ b/cs/dso/Abell/Abell20.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.598051 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.598054 +--- diff --git a/cs/dso/Abell/Abell22.md b/cs/dso/Abell/Abell22.md new file mode 100644 index 000000000..8fe96ccbe --- /dev/null +++ b/cs/dso/Abell/Abell22.md @@ -0,0 +1,9 @@ +--- +name: 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b/cs/dso/Abell/Abell29.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.608403 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.608405 +--- diff --git a/cs/dso/Abell/Abell3.md b/cs/dso/Abell/Abell3.md new file mode 100644 index 000000000..bef851583 --- /dev/null +++ b/cs/dso/Abell/Abell3.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.914389 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.914391 +--- diff --git a/cs/dso/Abell/Abell30.md b/cs/dso/Abell/Abell30.md new file mode 100644 index 000000000..485126b35 --- /dev/null +++ b/cs/dso/Abell/Abell30.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.136835 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.136838 +--- diff --git a/cs/dso/Abell/Abell35.md b/cs/dso/Abell/Abell35.md new file mode 100644 index 000000000..f9e546bb2 --- /dev/null +++ b/cs/dso/Abell/Abell35.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.290965 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.290967 +--- diff --git a/cs/dso/Abell/Abell36.md b/cs/dso/Abell/Abell36.md new file mode 100644 index 000000000..512177497 --- /dev/null +++ b/cs/dso/Abell/Abell36.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.280584 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.280587 +--- diff --git a/cs/dso/Abell/Abell4.md b/cs/dso/Abell/Abell4.md new file mode 100644 index 000000000..863c5ef70 --- /dev/null +++ b/cs/dso/Abell/Abell4.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.327611 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.327614 +--- diff --git a/cs/dso/Abell/Abell40.md b/cs/dso/Abell/Abell40.md new file mode 100644 index 000000000..8ade4d001 --- /dev/null +++ b/cs/dso/Abell/Abell40.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.714654 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.714656 +--- diff --git a/cs/dso/Abell/Abell41.md b/cs/dso/Abell/Abell41.md new file mode 100644 index 000000000..58f0fff93 --- /dev/null +++ b/cs/dso/Abell/Abell41.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.426380 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.426382 +--- diff --git a/cs/dso/Abell/Abell42.md b/cs/dso/Abell/Abell42.md new file mode 100644 index 000000000..33696e1f2 --- /dev/null +++ b/cs/dso/Abell/Abell42.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.690150 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.690153 +--- diff --git a/cs/dso/Abell/Abell43.md b/cs/dso/Abell/Abell43.md new 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/dev/null +++ b/cs/dso/BV/BV3.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.332134 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.332137 +--- diff --git a/cs/dso/Bol/Bol110.md b/cs/dso/Bol/Bol110.md deleted file mode 100644 index 74ed554c7..000000000 --- a/cs/dso/Bol/Bol110.md +++ /dev/null @@ -1,9 +0,0 @@ ---- -name: -rating: 1 -references: -created_by: skybber -created_date: 2023-10-23 19:27:09.421834 -updated_by: -updated_date: 2023-10-23 13:21:49.332224 ---- diff --git a/cs/dso/Bol/Bol12.md b/cs/dso/Bol/Bol12.md deleted file mode 100644 index 3aae64bfb..000000000 --- a/cs/dso/Bol/Bol12.md +++ /dev/null @@ -1,9 +0,0 @@ ---- -name: -rating: 1 -references: -created_by: skybber -created_date: 2023-10-23 19:07:15.456823 -updated_by: -updated_date: 2023-10-23 13:21:49.330958 ---- diff --git a/cs/dso/Bol/Bol158.md b/cs/dso/Bol/Bol158.md deleted file mode 100644 index 37b87dc7c..000000000 --- a/cs/dso/Bol/Bol158.md 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19:11:49.738041 -updated_by: -updated_date: 2023-10-23 13:21:49.337158 ---- diff --git a/cs/dso/Bol/Bol232.md b/cs/dso/Bol/Bol232.md deleted file mode 100644 index c04e77dda..000000000 --- a/cs/dso/Bol/Bol232.md +++ /dev/null @@ -1,9 +0,0 @@ ---- -name: -rating: 1 -references: -created_by: skybber -created_date: 2023-10-24 08:55:23.939896 -updated_by: -updated_date: 2023-10-24 08:25:05.704573 ---- diff --git a/cs/dso/Bol/Bol233.md b/cs/dso/Bol/Bol233.md deleted file mode 100644 index d2f7ffbfb..000000000 --- a/cs/dso/Bol/Bol233.md +++ /dev/null @@ -1,9 +0,0 @@ ---- -name: -rating: 1 -references: -created_by: skybber -created_date: 2023-10-24 08:57:06.122266 -updated_by: -updated_date: 2023-10-23 13:21:49.337158 ---- diff --git a/cs/dso/Bol/Bol240.md b/cs/dso/Bol/Bol240.md deleted file mode 100644 index 9797c8a19..000000000 --- a/cs/dso/Bol/Bol240.md +++ /dev/null @@ -1,9 +0,0 @@ ---- -name: -rating: 1 -references: -created_by: skybber -created_date: 2023-10-24 08:58:18.305691 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--- /dev/null +++ b/cs/dso/Pal/Pal3.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.663843 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.663845 +--- diff --git a/cs/dso/Pal/Pal4.md b/cs/dso/Pal/Pal4.md new file mode 100644 index 000000000..7f9dd55db --- /dev/null +++ b/cs/dso/Pal/Pal4.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.377990 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.377993 +--- diff --git a/cs/dso/Pal/Pal5.md b/cs/dso/Pal/Pal5.md new file mode 100644 index 000000000..a72d75831 --- /dev/null +++ b/cs/dso/Pal/Pal5.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.465822 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.465824 +--- diff --git a/cs/dso/Pal/Pal6.md b/cs/dso/Pal/Pal6.md new file mode 100644 index 000000000..27459a38d --- /dev/null +++ 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file mode 100644 index 000000000..85a4efcc3 --- /dev/null +++ b/cs/dso/UGC/UGC12856.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.020074 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.020078 +--- diff --git a/cs/dso/UGC/UGC12914.md b/cs/dso/UGC/UGC12914.md new file mode 100644 index 000000000..472a7fac1 --- /dev/null +++ b/cs/dso/UGC/UGC12914.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.023868 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.023872 +--- diff --git a/cs/dso/UGC/UGC1449.md b/cs/dso/UGC/UGC1449.md new file mode 100644 index 000000000..ed23c39d7 --- /dev/null +++ b/cs/dso/UGC/UGC1449.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.895248 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.895251 +--- diff --git a/cs/dso/UGC/UGC1775.md b/cs/dso/UGC/UGC1775.md new file mode 100644 index 000000000..09ff4b0a0 --- /dev/null +++ b/cs/dso/UGC/UGC1775.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.116381 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.116384 +--- diff --git a/cs/dso/UGC/UGC1810.md b/cs/dso/UGC/UGC1810.md new file mode 100644 index 000000000..a4efca47f --- /dev/null +++ b/cs/dso/UGC/UGC1810.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.060477 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.060491 +--- diff --git a/cs/dso/UGC/UGC1840.md b/cs/dso/UGC/UGC1840.md new file mode 100644 index 000000000..337c1bbaf --- /dev/null +++ b/cs/dso/UGC/UGC1840.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.063821 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.063823 +--- diff --git a/cs/dso/UGC/UGC2489.md b/cs/dso/UGC/UGC2489.md new file mode 100644 index 000000000..8ddd388e4 --- /dev/null +++ b/cs/dso/UGC/UGC2489.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.370497 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.370501 +--- diff --git a/cs/dso/UGC/UGC3258.md b/cs/dso/UGC/UGC3258.md new file mode 100644 index 000000000..04df5e268 --- /dev/null +++ b/cs/dso/UGC/UGC3258.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.557625 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.557627 +--- diff --git a/cs/dso/UGC/UGC3445.md b/cs/dso/UGC/UGC3445.md new file mode 100644 index 000000000..45b24b378 --- /dev/null +++ b/cs/dso/UGC/UGC3445.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.661900 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.661901 +--- diff --git a/cs/dso/UGC/UGC3573.md b/cs/dso/UGC/UGC3573.md new file mode 100644 index 000000000..c30283b05 --- /dev/null +++ b/cs/dso/UGC/UGC3573.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.507706 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.507709 +--- diff --git a/cs/dso/UGC/UGC3730.md b/cs/dso/UGC/UGC3730.md new file mode 100644 index 000000000..ebddd0fbf --- /dev/null +++ b/cs/dso/UGC/UGC3730.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.996967 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.996971 +--- diff --git a/cs/dso/UGC/UGC3828.md b/cs/dso/UGC/UGC3828.md new file mode 100644 index 000000000..56538433a --- /dev/null +++ b/cs/dso/UGC/UGC3828.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.664735 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.664737 +--- diff --git a/cs/dso/UGC/UGC4051.md b/cs/dso/UGC/UGC4051.md new file mode 100644 index 000000000..d02a4b07a --- /dev/null +++ b/cs/dso/UGC/UGC4051.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.667491 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.667493 +--- diff --git a/cs/dso/UGC/UGC4349.md b/cs/dso/UGC/UGC4349.md new file mode 100644 index 000000000..29ff0a688 --- /dev/null +++ b/cs/dso/UGC/UGC4349.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.285611 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.285615 +--- diff --git a/cs/dso/UGC/UGC4414.md b/cs/dso/UGC/UGC4414.md new file mode 100644 index 000000000..01fbe979a --- /dev/null +++ b/cs/dso/UGC/UGC4414.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.153843 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.153847 +--- diff --git a/cs/dso/UGC/UGC4653.md b/cs/dso/UGC/UGC4653.md new file mode 100644 index 000000000..07900ca81 --- /dev/null +++ b/cs/dso/UGC/UGC4653.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.670267 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.670269 +--- diff --git a/cs/dso/UGC/UGC4719.md b/cs/dso/UGC/UGC4719.md new file mode 100644 index 000000000..b1116e2d6 --- /dev/null +++ b/cs/dso/UGC/UGC4719.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.326762 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.326766 +--- diff --git a/cs/dso/UGC/UGC4881.md b/cs/dso/UGC/UGC4881.md new file mode 100644 index 000000000..3a9e0b28b --- /dev/null +++ b/cs/dso/UGC/UGC4881.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.673118 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.673120 +--- diff --git a/cs/dso/UGC/UGC5028.md b/cs/dso/UGC/UGC5028.md new file mode 100644 index 000000000..67a52e36b --- /dev/null +++ b/cs/dso/UGC/UGC5028.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.330121 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.330124 +--- diff --git a/cs/dso/UGC/UGC5459.md b/cs/dso/UGC/UGC5459.md new file mode 100644 index 000000000..bf2d2e045 --- /dev/null +++ b/cs/dso/UGC/UGC5459.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.334622 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.334624 +--- diff --git a/cs/dso/UGC/UGC5498.md b/cs/dso/UGC/UGC5498.md new file mode 100644 index 000000000..6647ea529 --- /dev/null +++ b/cs/dso/UGC/UGC5498.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.777881 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.777884 +--- diff --git a/cs/dso/UGC/UGC5832.md b/cs/dso/UGC/UGC5832.md new file mode 100644 index 000000000..dccb53ac3 --- /dev/null +++ b/cs/dso/UGC/UGC5832.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.782333 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.782336 +--- diff --git a/cs/dso/UGC/UGC5938.md b/cs/dso/UGC/UGC5938.md new file mode 100644 index 000000000..113ded189 --- /dev/null +++ b/cs/dso/UGC/UGC5938.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.431244 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.431245 +--- diff --git a/cs/dso/UGC/UGC6.md b/cs/dso/UGC/UGC6.md new file mode 100644 index 000000000..fe90961b3 --- /dev/null +++ b/cs/dso/UGC/UGC6.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.010014 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.010016 +--- diff --git a/cs/dso/UGC/UGC6073.md b/cs/dso/UGC/UGC6073.md new file mode 100644 index 000000000..fcfd02a9f --- /dev/null +++ b/cs/dso/UGC/UGC6073.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.786988 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.786991 +--- diff --git a/cs/dso/UGC/UGC6361.md b/cs/dso/UGC/UGC6361.md new file mode 100644 index 000000000..3c6ee23d5 --- /dev/null +++ b/cs/dso/UGC/UGC6361.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.792980 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.792984 +--- diff --git a/cs/dso/UGC/UGC6865.md b/cs/dso/UGC/UGC6865.md new file mode 100644 index 000000000..c1a5874c6 --- /dev/null +++ b/cs/dso/UGC/UGC6865.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.340813 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.340817 +--- diff --git a/cs/dso/UGC/UGC717.md b/cs/dso/UGC/UGC717.md new file mode 100644 index 000000000..0c0ae8049 --- /dev/null +++ b/cs/dso/UGC/UGC717.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.881589 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.881592 +--- diff --git a/cs/dso/UGC/UGC7522.md b/cs/dso/UGC/UGC7522.md new file mode 100644 index 000000000..5ce247cdb --- /dev/null +++ b/cs/dso/UGC/UGC7522.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.276036 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.276038 +--- diff --git a/cs/dso/UGC/UGC8335.md b/cs/dso/UGC/UGC8335.md new file mode 100644 index 000000000..6b536795a --- /dev/null +++ b/cs/dso/UGC/UGC8335.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.346438 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.346442 +--- diff --git a/cs/dso/UGC/UGC849.md b/cs/dso/UGC/UGC849.md new file mode 100644 index 000000000..6800fc1f0 --- /dev/null +++ b/cs/dso/UGC/UGC849.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.884636 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.884639 +--- diff --git a/cs/dso/UGC/UGC8696.md b/cs/dso/UGC/UGC8696.md new file mode 100644 index 000000000..596798c20 --- /dev/null +++ b/cs/dso/UGC/UGC8696.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.350229 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.350233 +--- diff --git a/cs/dso/UGC/UGC8713.md b/cs/dso/UGC/UGC8713.md new file mode 100644 index 000000000..e03b690dc --- /dev/null +++ b/cs/dso/UGC/UGC8713.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.578058 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.578059 +--- diff --git a/cs/dso/UGC/UGC8917.md b/cs/dso/UGC/UGC8917.md new file mode 100644 index 000000000..3e1d84268 --- /dev/null +++ b/cs/dso/UGC/UGC8917.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:31.582194 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:31.582195 +--- diff --git a/cs/dso/UGC/UGC9103.md b/cs/dso/UGC/UGC9103.md new file mode 100644 index 000000000..f5b7eaeab --- /dev/null +++ b/cs/dso/UGC/UGC9103.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.094088 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.094090 +--- diff --git a/cs/dso/UGC/UGC934.md b/cs/dso/UGC/UGC934.md new file mode 100644 index 000000000..ecf070e52 --- /dev/null +++ b/cs/dso/UGC/UGC934.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:29.887857 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:29.887859 +--- diff --git a/cs/dso/UGC/UGC9425.md b/cs/dso/UGC/UGC9425.md new file mode 100644 index 000000000..6594681ae --- /dev/null +++ b/cs/dso/UGC/UGC9425.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.097231 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.097233 +--- diff --git a/cs/dso/UGC/UGC9560.md b/cs/dso/UGC/UGC9560.md new file mode 100644 index 000000000..f4993356a --- /dev/null +++ b/cs/dso/UGC/UGC9560.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.100182 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.100184 +--- diff --git a/cs/dso/UGC/UGC9708.md b/cs/dso/UGC/UGC9708.md new file mode 100644 index 000000000..b1c70fd88 --- /dev/null +++ b/cs/dso/UGC/UGC9708.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:32.103127 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:32.103129 +--- diff --git a/cs/dso/UGC/UGC9829.md b/cs/dso/UGC/UGC9829.md new file mode 100644 index 000000000..f8cb7f8f3 --- /dev/null +++ b/cs/dso/UGC/UGC9829.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.460430 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.460433 +--- diff --git a/cs/dso/We/We1-9.md b/cs/dso/We/We1-9.md new file mode 100644 index 000000000..5b27df373 --- /dev/null +++ b/cs/dso/We/We1-9.md @@ -0,0 +1,9 @@ +--- +name: +rating: +references: +created_by: editor.cs +created_date: 2023-10-31 20:08:30.484907 +updated_by: editor.cs +updated_date: 2023-10-31 20:08:30.484909 +--- diff --git a/en/star/38_Psc.md b/en/star/38_Psc.md new file mode 100644 index 000000000..c7385eb00 --- /dev/null +++ b/en/star/38_Psc.md @@ -0,0 +1,9 @@ +--- +name: 38 Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 16:12:19.021017 +updated_by: editor.cs +updated_date: 2023-11-05 16:12:19.021021 +--- +Multiple star, attractive pair of yellow stars in a cluster of faint stars. The AB pair is indistinguishable and is perceived as a 7.9 magnitude object, but at a separation of 4.3", we can see a 7.8 magnitude companion. Another, this time of 12th magnitude, lies 63" southeast. \ No newline at end of file diff --git a/en/star/Barnardova_hviezda.md b/en/star/Barnardova_hviezda.md new file mode 100644 index 000000000..8da139b5f --- /dev/null +++ b/en/star/Barnardova_hviezda.md @@ -0,0 +1,9 @@ +--- +name: Barnardova hviezda +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 16:42:33.886581 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:33.886587 +--- +These interesting red stars, visible only through a telescope, move the fastest of all against the background of more distant stars - they shift by 10.31" per year, which means they change their position by the diameter of the Moon in 180 years. Sometimes they are also referred to as Barnard's arrow. Among all known stars, they have the largest proper motion, which was discovered by E. Barnard in 1916. After the Alpha Centauri system, they are the second closest star to our Sun, only 5.9 light-years away, which is also the main reason for their fast motion across the sky. Barnard's arrow is still approaching us, and in the year 9700, when it will be located in the head of Draco, it will be only 3.8 light-years away from us! Tracking its motion can be a very interesting activity. By drawing its position in the star field at least once a year with a higher magnification, we can see it for ourselves. \ No newline at end of file diff --git a/en/star/Brisbane_14.md b/en/star/Brisbane_14.md new file mode 100644 index 000000000..d5eeeeb85 --- /dev/null +++ b/en/star/Brisbane_14.md @@ -0,0 +1,9 @@ +--- +name: Brisbane 14 +constellation: CrA +created_by: editor.cs +created_date: 2023-11-05 16:29:33.396538 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:33.396544 +--- +The double star observed only 12' WSW of the reflection nebula NGC 6726-27, as a nearly equally bright pair of blue-white components with magnitudes 6.6 and 6.8, which can be resolved even with a small telescope. The mutual separation of the components is 12.7". \ No newline at end of file diff --git a/en/star/Burnham_441.md b/en/star/Burnham_441.md new file mode 100644 index 000000000..3457630a8 --- /dev/null +++ b/en/star/Burnham_441.md @@ -0,0 +1,9 @@ +--- +name: Burnham 441 +constellation: Vul +created_by: editor.cs +created_date: 2023-11-05 16:32:17.709612 +updated_by: editor.cs +updated_date: 2023-11-05 16:32:17.709614 +--- +This double star could be observed with a 100 mm telescope. It presents as a color contrast between a golden and blue component. The difference in magnitude is significant, with the golden component reaching 6.2 mag and the blue component only 10.7 mag. It is located at a separation of 5.9". \ No newline at end of file diff --git a/en/star/CAS_A.md b/en/star/CAS_A.md new file mode 100644 index 000000000..5e440ea91 --- /dev/null +++ b/en/star/CAS_A.md @@ -0,0 +1,9 @@ +--- +name: CAS A +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 17:42:57.941907 +updated_by: editor.cs +updated_date: 2023-11-05 17:42:57.941911 +--- +The remains of a supernova, which likely appeared in the sky several tens of thousands of years ago, so there are no proven records of it. Today, we observe the strongest stellar radio source in the entire sky from this region, south of M52. At the location of the radio object, we can find filamentary nebulae expanding at a velocity of 900 km/s, with their distance estimated at 10,000 light-years. \ No newline at end of file diff --git a/en/star/Cygnus_X-1.md b/en/star/Cygnus_X-1.md new file mode 100644 index 000000000..25952cbe6 --- /dev/null +++ b/en/star/Cygnus_X-1.md @@ -0,0 +1,9 @@ +--- +name: Cygnus X-1 +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 17:13:05.198576 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:05.198579 +--- +A binary star near η Cygni. It is a variable source of X-ray radiation. One component is visible, the other is not visible, but X-rays are emitted from its surroundings. The visible star is a luminous giant, the invisible component is likely a collapsed old star with a large mass - a black hole with a radius of only 10 km, which draws a huge amount of gas from the luminous giant (with a radius of 10 million km) and emits extremely intense X-ray radiation before it reaches its boundary, emitting X-rays. \ No newline at end of file diff --git a/en/star/Falešný_kríž.md b/en/star/Falešný_kríž.md new file mode 100644 index 000000000..070fcc385 --- /dev/null +++ b/en/star/Falešný_kríž.md @@ -0,0 +1,9 @@ +--- +name: Falešný kríž +constellation: Car +created_by: editor.cs +created_date: 2023-11-05 15:41:08.548981 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:08.548986 +--- +The quartet of stars ι, ε Car, and δ and κ Velorum form the letter X in the sky, which is often confused with the stars of the Southern Cross. However, the False Cross is slightly larger, more symmetrical, and less bright. ε Car is a beautiful double star distinguishable in a smaller telescope. It consists of two components with brightness of 3mag and 6mag, separated by 5". \ No newline at end of file diff --git a/en/star/Groombridge_1830.md b/en/star/Groombridge_1830.md new file mode 100644 index 000000000..3149db979 --- /dev/null +++ b/en/star/Groombridge_1830.md @@ -0,0 +1,9 @@ +--- +name: Groombridge 1830 +constellation: UMa +created_by: editor.cs +created_date: 2023-11-05 15:16:25.642252 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:25.642255 +--- +A nearby star, which has the third fastest known motion after Barnard's Star and Kapteyn's Star - 7.04" per year. In about 100,000 years, the star will move from Ursa Major to the constellation of Canis Major! Because it is 28 light-years away, its rapid apparent motion is more a result of its actual space velocity than its proximity. Such stars are part of the Galactic Halo and therefore as old as globular clusters. Arcturus in Boötes is their brightest example. \ No newline at end of file diff --git a/en/star/Groombridge_34_(Grb_34).md b/en/star/Groombridge_34_(Grb_34).md new file mode 100644 index 000000000..2e6622cf8 --- /dev/null +++ b/en/star/Groombridge_34_(Grb_34).md @@ -0,0 +1,9 @@ +--- +name: Groombridge 34 (Grb 34) +constellation: And +created_by: editor.cs +created_date: 2023-11-05 16:33:30.356282 +updated_by: editor.cs +updated_date: 2023-11-05 16:33:30.356285 +--- +The red star, a dwarf from the nearby vicinity, is only 11.56 light-years away and visible even with a small telescope at its 8.2 magnitude, about a quarter of a degree away from the star 26 And. A companion of brightness 10.6 magnitude orbits it at a distance of 35.5" in 2,600 years. The pair has a fast proper motion of 2.89" per year. Detailed drawings made at high magnifications once a year reveal this motion relative to the surrounding star field. \ No newline at end of file diff --git a/en/star/Herschel_3750.md b/en/star/Herschel_3750.md new file mode 100644 index 000000000..6cc9f8b9a --- /dev/null +++ b/en/star/Herschel_3750.md @@ -0,0 +1,9 @@ +--- +name: Herschel 3750 +constellation: Lep +created_by: editor.cs +created_date: 2023-11-05 17:13:23.571019 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:23.571024 +--- +This tight yellow-white-blue binary star was named by William Herschel as the "most beautiful binary star". It can be easily verified even with a smaller telescope. The components have magnitudes of 4.7 and 8.4, with a separation of 4.2". \ No newline at end of file diff --git a/en/star/Herschel_3780.md b/en/star/Herschel_3780.md new file mode 100644 index 000000000..bcf61ed7e --- /dev/null +++ b/en/star/Herschel_3780.md @@ -0,0 +1,9 @@ +--- +name: Herschel 3780 +constellation: Lep +created_by: editor.cs +created_date: 2023-11-05 16:13:09.894742 +updated_by: editor.cs +updated_date: 2023-11-05 16:13:09.894746 +--- +A small star cluster (NGC 2017), whose main members are listed in the Herschel catalog. A small telescope reveals a star of magnitude 6 with four companions of magnitude 8 to 10. In a larger telescope, it can be verified that two of the components are close binary stars. At the same time, a fainter star of magnitude 12, which complements the group, is also visible. \ No newline at end of file diff --git a/en/star/Herschel_3857.md b/en/star/Herschel_3857.md new file mode 100644 index 000000000..9123ab7d5 --- /dev/null +++ b/en/star/Herschel_3857.md @@ -0,0 +1,9 @@ +--- +name: Herschel 3857 +constellation: Col +created_by: editor.cs +created_date: 2023-11-05 16:36:09.190175 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:09.190179 +--- +We will see the triple star in the telescope with a 100 mm objective diameter as a nice wide yellow-orange pair of stars, with a brightness of 5.7 mag and 6.9 mag, respectively. The brighter component has a separation of 12.9 arcseconds from a fainter grayish-white companion with a magnitude of 10.8 mag. \ No newline at end of file diff --git a/en/star/Herschel_4423.md b/en/star/Herschel_4423.md new file mode 100644 index 000000000..021131378 --- /dev/null +++ b/en/star/Herschel_4423.md @@ -0,0 +1,9 @@ +--- +name: Herschel 4423 +constellation: Cen +created_by: editor.cs +created_date: 2023-11-05 17:32:07.330684 +updated_by: editor.cs +updated_date: 2023-11-05 17:32:07.330688 +--- +An attractive pair of yellow stars dominates a relatively sparse field of stars. The components have apparent magnitudes of 6.9 and 7.2, and they are separated by 2.4 arcseconds. \ No newline at end of file diff --git a/en/star/Herschel_4788.md b/en/star/Herschel_4788.md new file mode 100644 index 000000000..983a5524e --- /dev/null +++ b/en/star/Herschel_4788.md @@ -0,0 +1,9 @@ +--- +name: Herschel 4788 +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 16:12:09.350068 +updated_by: editor.cs +updated_date: 2023-11-05 16:12:09.350072 +--- +A binary star, which is a good test for a 100-150 mm telescope. During a calm night, this unequally bright pair of white and yellow stars appears as two disks in contact. However, if there is any turbulence in the atmosphere, the stars merge into one elongated droplet. They are separated by 2.2" and their magnitudes are 4.7mag and 6.7mag, respectively. \ No newline at end of file diff --git a/en/star/Herschel_5003.md b/en/star/Herschel_5003.md new file mode 100644 index 000000000..b8cc5efd4 --- /dev/null +++ b/en/star/Herschel_5003.md @@ -0,0 +1,9 @@ +--- +name: Herschel 5003 +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 16:26:06.292969 +updated_by: editor.cs +updated_date: 2023-11-05 16:26:06.292972 +--- +A triple star consisting of two red-orange stars, with the brighter one at 5.2 magnitude being redder. The fainter one at 6.9 magnitude is located at a distance of 5.5". Another, very faint companion at 13 magnitude can be found at a distance of 26.2" and can be resolved during a good night. These triple stars are located in a beautiful field of the Milky Way. \ No newline at end of file diff --git a/en/star/Herschel_84.md b/en/star/Herschel_84.md new file mode 100644 index 000000000..29e93954b --- /dev/null +++ b/en/star/Herschel_84.md @@ -0,0 +1,9 @@ +--- +name: Herschel 84 +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 16:31:22.590389 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:22.590394 +--- +A binary star consisting of a primary orange component (6.5 mag) and a secondary blue component (8.9 mag) with a separation of 28.2". In at least a 100 mm telescope and higher magnification, it is one of the most beautiful binary stars in the constellation. \ No newline at end of file diff --git a/en/star/Kapteynova_hviezda.md b/en/star/Kapteynova_hviezda.md new file mode 100644 index 000000000..db8ecfefa --- /dev/null +++ b/en/star/Kapteynova_hviezda.md @@ -0,0 +1,9 @@ +--- +name: Kapteynova hviezda +constellation: Pic +created_by: editor.cs +created_date: 2023-11-05 16:13:18.228796 +updated_by: editor.cs +updated_date: 2023-11-05 16:13:18.228799 +--- +The red star with a magnitude of 8.8 is still visible through a telescope, in the close vicinity of our Sun. It is only 13 light-years away from it and exhibits the largest proper motion - 8.7 arc seconds per year - after Barnard's Star. Its position will change by the diameter of the Moon in two centuries. This rapid motion, in space at a speed of 280 km/s, was discovered in 1897 by the Dutch astronomer Jacobus C. Kapteyn, after whom the star is named. Its luminosity is 50 times smaller than that of the Sun. \ No newline at end of file diff --git a/en/star/Keplerova_supernova.md b/en/star/Keplerova_supernova.md new file mode 100644 index 000000000..d1afe3dce --- /dev/null +++ b/en/star/Keplerova_supernova.md @@ -0,0 +1,9 @@ +--- +name: Keplerova supernova +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 16:32:23.931635 +updated_by: editor.cs +updated_date: 2023-11-05 16:32:23.931639 +--- +The last galactic supernova, which erupted on September 9, 1604. It is named after a famous German astronomer who observed it at that time. It was visible to the naked eye for 12 months and several weeks, and its brightness of -2.5mag surpassed even the planet Jupiter. Johannes Kepler and David Fabricius determined its position with such precision that the German-American astronomer Walter Baade could identify a faint nebula, the remnant of the supernova, in the same location in 1943. The star itself is now fainter than 19mag and can only be observed with the largest telescopes. Its remnant was also revealed by the Hubble Space Telescope. \ No newline at end of file diff --git a/en/star/Kruger_60.md b/en/star/Kruger_60.md new file mode 100644 index 000000000..d3a591d61 --- /dev/null +++ b/en/star/Kruger_60.md @@ -0,0 +1,9 @@ +--- +name: Kruger 60 +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 15:46:23.999696 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:23.999700 +--- +Although invisible to the naked eye, it is otherwise a well-known and interesting binary star. It lies 43' south of δ Cephei. To resolve the primary component with a brightness of 9.8 mag and its companion with a brightness of 11.3 mag, a minimum of a 120 mm telescope and high magnification will be needed, as they are separated by 2.4 arcseconds. It is located at a distance of only 13.1 light-years, making it one of our closest binary stars. The orbital period of these red dwarfs is only 44.5 years. Their average distance is 1.4 billion km, which is equivalent to the distance between the Sun and Saturn. The mass of the primary star represents about 0.25 times the mass of the Sun, and the mass of its companion is even only 0.15 times the mass of the Sun, with their luminosity being even smaller. \ No newline at end of file diff --git a/en/star/Lacaille_9352.md b/en/star/Lacaille_9352.md new file mode 100644 index 000000000..5ca47afd4 --- /dev/null +++ b/en/star/Lacaille_9352.md @@ -0,0 +1,9 @@ +--- +name: Lacaille 9352 +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 17:54:13.011005 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:13.011009 +--- +The red dwarf has a visual magnitude of 7.4. After Barnard's Star and Kapteyn's Star, and after Groombridge 1830 from Ursa Major, Lacaille 9352 exhibits the fourth fastest known proper motion. This star will move by 6.9" per year, and by the year 2100, it will already be located in the neighboring constellation of Sculptor. It is situated at a distance of only 10.7 light-years. \ No newline at end of file diff --git a/en/star/Lalande_21185.md b/en/star/Lalande_21185.md new file mode 100644 index 000000000..092df3ff1 --- /dev/null +++ b/en/star/Lalande_21185.md @@ -0,0 +1,9 @@ +--- +name: Lalande 21185 +constellation: UMa +created_by: editor.cs +created_date: 2023-11-05 16:27:00.569001 +updated_by: editor.cs +updated_date: 2023-11-05 16:27:00.569005 +--- +The nearby red dwarf, which has a brightness of 7.49 mag, is located at a distance of 8.1 light-years and is our fourth closest star after the Alpha Centauri system, Barnard's Star from Ophiuchus, and Wolf 359 from Leo. It has the 8th largest known proper motion - it moves across the sky by 4.78" per year. This red dwarf has an absolute magnitude of +10.5, which corresponds to a luminosity of 0.0048 times that of the Sun. Lalande 21185 has a companion, but it has never been visually observed. \ No newline at end of file diff --git a/en/star/N_1918_Aql.md b/en/star/N_1918_Aql.md new file mode 100644 index 000000000..28ebb9db5 --- /dev/null +++ b/en/star/N_1918_Aql.md @@ -0,0 +1,9 @@ +--- +name: N 1918 Aql +constellation: Aql +created_by: editor.cs +created_date: 2023-11-05 17:53:59.520215 +updated_by: skybber +updated_date: 2023-11-05 18:17:35.528758 +--- +After the nova, which appeared in the Aquila constellation in 389 and became brighter like Venus, astronomers witnessed another one in 1918. It became the brightest star in the constellation and the second brightest star in the sky, reaching -1.1 magnitude. Today, it cannot be observed with the naked eye or even with a telescope, as it only reaches 10.8 magnitude. \ No newline at end of file diff --git a/en/star/N_1991.md b/en/star/N_1991.md new file mode 100644 index 000000000..c57226b64 --- /dev/null +++ b/en/star/N_1991.md @@ -0,0 +1,9 @@ +--- +name: N 1991 +constellation: Mus +created_by: editor.cs +created_date: 2023-11-05 16:11:57.594820 +updated_by: editor.cs +updated_date: 2023-11-05 16:11:57.594825 +--- +In 1991, a nova erupted on the western edge of the constellation, designated as N 1991, which briefly became one of the brightest sources of X-ray radiation in the sky. It is believed to be a close binary star, with one component orbiting around a black hole, which can trigger processes leading to intense X-ray emission. \ No newline at end of file diff --git a/en/star/Nova_Delphini_1967.md b/en/star/Nova_Delphini_1967.md new file mode 100644 index 000000000..e9416bf09 --- /dev/null +++ b/en/star/Nova_Delphini_1967.md @@ -0,0 +1,9 @@ +--- +name: Nova Delphini 1967 +constellation: Del +created_by: editor.cs +created_date: 2023-11-05 16:49:26.449991 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:26.449994 +--- +The constellation was made famous by a nova discovered on July 8, 1967 by English teacher and amateur astronomers G. Alcock, who also discovered the Nova Vulpeculae in 1968. This peculiar nova gradually brightened and became visible to the naked eye, then its brightness irregularly fluctuated and weakened again in December 1967. According to records, it is the "slowest nova". Its current magnitude is approximately 12.7mag, making it visible with a slightly larger amateur telescope. \ No newline at end of file diff --git a/en/star/P_Hya.md b/en/star/P_Hya.md new file mode 100644 index 000000000..9d13776a2 --- /dev/null +++ b/en/star/P_Hya.md @@ -0,0 +1,9 @@ +--- +name: P Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 16:47:40.554172 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:40.554175 +--- +The easily distinguishable components of 5th magnitude and 6.9th magnitude are located at a separation of 4 arcminutes. Using a telescope with a 60mm objective diameter, we can determine that the fainter component has a 9.6 arcsecond companion of 9th magnitude. \ No newline at end of file diff --git a/en/star/Plaskettova_hviezda.md b/en/star/Plaskettova_hviezda.md new file mode 100644 index 000000000..501f364b8 --- /dev/null +++ b/en/star/Plaskettova_hviezda.md @@ -0,0 +1,18 @@ +--- +name: Plaskettova hviezda +constellation: Mon +created_by: editor.cs +created_date: 2023-11-05 16:38:58.290934 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:58.290938 +--- +Astronomický text: + +A spectral binary star of sixth magnitude, discovered in 1922 by Canadian astronomer and director of the Victoria Observatory, John Stanley Plaskett. It is the most massive known binary star. + +Překlad českých zkratek světových stran: + +N - North +W - West +S - South +E - East \ No newline at end of file diff --git a/en/star/RR_Lyrae.md b/en/star/RR_Lyrae.md new file mode 100644 index 000000000..c1581a7f4 --- /dev/null +++ b/en/star/RR_Lyrae.md @@ -0,0 +1,9 @@ +--- +name: RR Lyrae +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 16:42:55.505078 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:55.505082 +--- +This star, located on the border with Cygnus, is not visible to the naked eye and represents a significant class of variable stars whose brightness changes in a short period. These are old stars mainly found near the galactic center and in globular clusters, the oldest formations of the galaxy. RR Lyrae pulsates regularly, similar to delta Cephei, but its period is shorter than one day - 0.567 days. During this time - 13 hours and 36 minutes, the apparent brightness fluctuates from 7mag to 8.1mag. The cycle can therefore be observed (from some areas) practically in one night. It is white at maximum and takes on a yellowish hue at minimum. \ No newline at end of file diff --git a/en/star/RR_Tel.md b/en/star/RR_Tel.md new file mode 100644 index 000000000..6d00f435a --- /dev/null +++ b/en/star/RR_Tel.md @@ -0,0 +1,9 @@ +--- +name: RR Tel +constellation: Tel +created_by: editor.cs +created_date: 2023-11-05 15:42:26.291091 +updated_by: editor.cs +updated_date: 2023-11-05 15:42:26.291094 +--- +Although this star is too faint for a small telescope, it is one of the most interesting novae recorded in our history. Before 1945, its brightness fluctuated between 12.5 mag and 15 mag. However, it then flared up and maintained a brightness of 6.5 mag for 5 years. Although it later faded back to its original brightness, it still retained its original period of brightness changes. It is definitely a binary star, with the larger component being a red giant that varies in brightness, while the smaller component is a hot dense star that flared up as a nova. \ No newline at end of file diff --git a/en/star/RS_Oph.md b/en/star/RS_Oph.md new file mode 100644 index 000000000..b5af71ad2 --- /dev/null +++ b/en/star/RS_Oph.md @@ -0,0 +1,9 @@ +--- +name: RS Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 16:28:12.020715 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:12.020719 +--- +Recurrent nova, which gradually flared up in the years 1898, 1933, 1958, 1967, and 1985. It has a minimum brightness of 11.8mag and can flare up to 4.3mag. \ No newline at end of file diff --git a/en/star/RW_Tauri.md b/en/star/RW_Tauri.md new file mode 100644 index 000000000..83fbe4a18 --- /dev/null +++ b/en/star/RW_Tauri.md @@ -0,0 +1,9 @@ +--- +name: RW Tauri +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:28:59.918248 +updated_by: editor.cs +updated_date: 2023-11-05 17:28:59.918252 +--- +An eclipsing variable star, one degree northwest of 41 Tauri. The primary component is completely eclipsed every 2.76 days, which reduces its brightness from 7.9 mag to 11.4 mag. The total eclipse lasts for 9 hours, and the entire obscuration persists for an additional 84 minutes. Among eclipsing variable stars, RW Tauri exhibits one of the deepest magnitude decreases, up to 3.5. It is estimated that this system is located 1,370 light-years away. \ No newline at end of file diff --git a/en/star/RX_J185635-3754.md b/en/star/RX_J185635-3754.md new file mode 100644 index 000000000..1cc2c6449 --- /dev/null +++ b/en/star/RX_J185635-3754.md @@ -0,0 +1,9 @@ +--- +name: RX J185635-3754 +constellation: CrA +created_by: editor.cs +created_date: 2023-11-05 16:48:21.553843 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:21.553847 +--- +Under this obscure designation hides our closest neutron star, which is located at a distance of 200 light-years. With its apparent magnitude of 26mag, it cannot be observed in any case, it was discovered only in 1996 by the Hubble Space Telescope. It is a remnant of a supernova explosion that occurred a million years ago. \ No newline at end of file diff --git a/en/star/R_Ara.md b/en/star/R_Ara.md new file mode 100644 index 000000000..31808aae1 --- /dev/null +++ b/en/star/R_Ara.md @@ -0,0 +1,9 @@ +--- +name: R Ara +constellation: Ara +created_by: editor.cs +created_date: 2023-11-05 16:26:51.939864 +updated_by: editor.cs +updated_date: 2023-11-05 16:26:51.939868 +--- +An eclipsing variable star of Algol type, with a period of 4.4 days and a magnitude change from 6.0 to 6.9. In the field of view of the telescope, it is located along with the stars ζ and η Ara. \ No newline at end of file diff --git a/en/star/R_Cae.md b/en/star/R_Cae.md new file mode 100644 index 000000000..f13ee9808 --- /dev/null +++ b/en/star/R_Cae.md @@ -0,0 +1,9 @@ +--- +name: R Cae +constellation: Cae +created_by: editor.cs +created_date: 2023-11-05 17:17:28.309974 +updated_by: editor.cs +updated_date: 2023-11-05 17:17:28.309979 +--- +A relatively bright variable star of the Mira Ceti type, which changes its brightness between 6.7mag and 13.7mag in a period longer than 13 months. \ No newline at end of file diff --git a/en/star/R_Casiopeiae.md b/en/star/R_Casiopeiae.md new file mode 100644 index 000000000..f5f2b8c27 --- /dev/null +++ b/en/star/R_Casiopeiae.md @@ -0,0 +1,9 @@ +--- +name: R Casiopeiae +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 17:54:39.047379 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:39.047382 +--- +Long-period variable star with a magnitude range from 4.7 to 13.5 over 431 days. It is located closer to the border with the constellation of Andromeda. \ No newline at end of file diff --git a/en/star/R_Com.md b/en/star/R_Com.md new file mode 100644 index 000000000..dd1adb833 --- /dev/null +++ b/en/star/R_Com.md @@ -0,0 +1,9 @@ +--- +name: R Com +constellation: Com +created_by: editor.cs +created_date: 2023-11-05 16:29:55.199124 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:55.199128 +--- +The variable star of Mira Ceti type with a magnitude fluctuation ranging from 7.1 to 14.6 in a period of 363 days. \ No newline at end of file diff --git a/en/star/R_Corvi.md b/en/star/R_Corvi.md new file mode 100644 index 000000000..d616e9a74 --- /dev/null +++ b/en/star/R_Corvi.md @@ -0,0 +1,9 @@ +--- +name: R Corvi +constellation: Crv +created_by: editor.cs +created_date: 2023-11-05 17:11:34.057144 +updated_by: editor.cs +updated_date: 2023-11-05 17:11:34.057147 +--- +The orange-red variable star of Mira type changes its brightness in the range of magnitude 6.7 to 14.4 in a period of 10 months - 317 days. It forms the western vertex of a triangle together with two stars of magnitude 7.5. During their maximum, it brightly illuminates them, while during its minimum, it can hardly be seen even in a larger telescope. \ No newline at end of file diff --git a/en/star/R_Hydrae.md b/en/star/R_Hydrae.md new file mode 100644 index 000000000..1889dc1d2 --- /dev/null +++ b/en/star/R_Hydrae.md @@ -0,0 +1,9 @@ +--- +name: R Hydrae +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 15:59:17.607294 +updated_by: editor.cs +updated_date: 2023-11-05 15:59:17.607298 +--- +The red giant, one of the most famous Mira Ceti variable stars. It changes its apparent brightness from 3.5 mag to 10.9 mag in a period of 389.6 days, which astronomers first noticed in the 17th century. However, the period has likely shortened by about 100 days since then. It is approximately 700 light-years away and at its greatest maximum surpasses the luminosity of 7000 Suns. \ No newline at end of file diff --git a/en/star/R_LMi.md b/en/star/R_LMi.md new file mode 100644 index 000000000..aadfadc1b --- /dev/null +++ b/en/star/R_LMi.md @@ -0,0 +1,9 @@ +--- +name: R LMi +constellation: LMi +created_by: editor.cs +created_date: 2023-11-05 17:44:21.677062 +updated_by: editor.cs +updated_date: 2023-11-05 17:44:21.677065 +--- +The variable star of Mira type, similar in many ways to the permanently red R Leonis. Its period is about 372 days and its brightness varies from 6.3mag to 13.2mag, making it beyond the reach of small telescopes. It is located 45' southeast of the star 13 LMI, which has a brightness of 6.2mag. \ No newline at end of file diff --git a/en/star/R_Oct.md b/en/star/R_Oct.md new file mode 100644 index 000000000..cda268aa4 --- /dev/null +++ b/en/star/R_Oct.md @@ -0,0 +1,9 @@ +--- +name: R Oct +constellation: Oct +created_by: editor.cs +created_date: 2023-11-05 16:35:25.540417 +updated_by: editor.cs +updated_date: 2023-11-05 16:35:25.540421 +--- +The variable star of Mira Ceti type reaches a brightness of 6.4 mag at its maximum, which can be easily seen with a telescope. However, it drops to as low as 13.2 mag at its minimum and disappears from view. Its period is 406 days. \ No newline at end of file diff --git a/en/star/R_Ret.md b/en/star/R_Ret.md new file mode 100644 index 000000000..cc74f8d47 --- /dev/null +++ b/en/star/R_Ret.md @@ -0,0 +1,9 @@ +--- +name: R Ret +constellation: Ret +created_by: editor.cs +created_date: 2023-11-05 15:46:40.672368 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:40.672372 +--- +A red Mira-type star reaching a maximum magnitude of 7. It returns to its minimum, where its brightness drops to 13 mag, approximately 9 months later. \ No newline at end of file diff --git a/en/star/R_TrA.md b/en/star/R_TrA.md new file mode 100644 index 000000000..638eec1d7 --- /dev/null +++ b/en/star/R_TrA.md @@ -0,0 +1,9 @@ +--- +name: R TrA +constellation: TrA +created_by: editor.cs +created_date: 2023-11-05 17:56:40.495884 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:40.495888 +--- +Cepheid variable changing its brightness by almost one magnitude: 6-6.8 mag with a period of 3.389 days. For cepheids that change their brightness so rapidly, determining their brightness once per night is insufficient. \ No newline at end of file diff --git a/en/star/R_a_S_Gru.md b/en/star/R_a_S_Gru.md new file mode 100644 index 000000000..dbca31c7e --- /dev/null +++ b/en/star/R_a_S_Gru.md @@ -0,0 +1,9 @@ +--- +name: R a S Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 15:14:41.183458 +updated_by: editor.cs +updated_date: 2023-11-05 15:14:41.183461 +--- +Variable stars of the Mira Ceti type are observed in their maximum brightness. R Gruis changes its magnitude from 7.4 to 14.9 in a period of 332 days, while S Gruis changes from 6 to 15 over a period of 401 days. \ No newline at end of file diff --git a/en/star/R_a_TW_Hor.md b/en/star/R_a_TW_Hor.md new file mode 100644 index 000000000..869d85431 --- /dev/null +++ b/en/star/R_a_TW_Hor.md @@ -0,0 +1,9 @@ +--- +name: R a TW Hor +constellation: Hor +created_by: editor.cs +created_date: 2023-11-05 15:44:34.059193 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:34.059197 +--- +Red giants, long-period variable stars of the Mira Ceti type, whose brightness reaches a maximum of fifth magnitude. R Hor weakens to 14 mag over the course of more than one year, while it takes approximately 5-6 months for the star TW Hor. \ No newline at end of file diff --git a/en/star/SN1987A.md b/en/star/SN1987A.md new file mode 100644 index 000000000..8722f9e46 --- /dev/null +++ b/en/star/SN1987A.md @@ -0,0 +1,9 @@ +--- +name: SN1987A +constellation: Dor +created_by: editor.cs +created_date: 2023-11-05 16:27:41.710278 +updated_by: editor.cs +updated_date: 2023-11-05 16:27:41.710282 +--- +A bright supernova, which appeared on February 23, 1987 in the Large Magellanic Cloud near the Tarantula Nebula and reached its maximum brightness of 2.8 magnitude. After 383 years since Kepler's supernova, the inhabitants of the southern hemisphere could admire another supernova visible to the naked eye. It shone in the sky for 10 months, but it is now very faint. It is likely that a pulsar remained after it, but it has not been found yet. \ No newline at end of file diff --git a/en/star/SN_1006.md b/en/star/SN_1006.md new file mode 100644 index 000000000..44b5ced92 --- /dev/null +++ b/en/star/SN_1006.md @@ -0,0 +1,9 @@ +--- +name: SN 1006 +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 15:44:09.282868 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:09.282873 +--- +In the constellation, the brightest recorded supernova in human history erupted in the past. It was noticed by the inhabitants of China and Japan, as well as the Middle East and Europe. When it first appeared in the sky in the spring of 1006, it was about as bright as Mars in opposition. However, within a few weeks, it easily surpassed Venus and brightened to -7.5 magnitude, equivalent to the brightness of the Moon in the first quarter. The supernova remained visible for the next two years, and even briefly during the day. Today, we only observe a cloud of debris from the ancient stellar explosion at this location. \ No newline at end of file diff --git a/en/star/SS_Cygni.md b/en/star/SS_Cygni.md new file mode 100644 index 000000000..9cf3a7144 --- /dev/null +++ b/en/star/SS_Cygni.md @@ -0,0 +1,9 @@ +--- +name: SS Cygni +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 17:51:57.269168 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:57.269173 +--- +One of the many variable stars is a cataclysmic variable star, which flares up to a brightness of 8mag every 2 months, but normally it is a 12mag star. It is the prototype of dwarf stars known either as SS Cygni-type variable stars or U Geminorum-type variable stars. \ No newline at end of file diff --git a/en/star/SX_Phe.md b/en/star/SX_Phe.md new file mode 100644 index 000000000..550b004e2 --- /dev/null +++ b/en/star/SX_Phe.md @@ -0,0 +1,9 @@ +--- +name: SX Phe +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 18:08:29.663444 +updated_by: editor.cs +updated_date: 2023-11-05 18:08:29.663448 +--- +Dwarf Cepheid, a variable star whose brightness changes from 7.1mag to 7.5mag every 79 minutes and 10 seconds! However, sometimes it brightens up to 6.7mag. \ No newline at end of file diff --git a/en/star/S_Aps.md b/en/star/S_Aps.md new file mode 100644 index 000000000..657f00e4d --- /dev/null +++ b/en/star/S_Aps.md @@ -0,0 +1,9 @@ +--- +name: S Aps +constellation: Aps +created_by: editor.cs +created_date: 2023-11-05 16:33:02.809445 +updated_by: editor.cs +updated_date: 2023-11-05 16:33:02.809449 +--- +This star is a new "reverse". Usually it is brighter than 10mag, so it can be observed even with a small telescope, but it apparently irregularly emits dark material into its surroundings, which reduces its brightness by 100 times to 15mag. After a few weeks, when the veil dissipates into the surroundings, it will shine again in its original brilliance. \ No newline at end of file diff --git a/en/star/S_Doradus.md b/en/star/S_Doradus.md new file mode 100644 index 000000000..2ebf9d825 --- /dev/null +++ b/en/star/S_Doradus.md @@ -0,0 +1,9 @@ +--- +name: S Doradus +constellation: Dor +created_by: editor.cs +created_date: 2023-11-05 17:55:55.964586 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:55.964589 +--- +An exceptionally luminous star that surpasses the Sun in brightness by at least a million times. It is one of the most radiant stars in existence. However, due to its distance, it cannot be seen with the naked eye and is only perceived as a faint star, whose brightness fluctuates between 8th magnitude and 11.5th magnitude, as it is an eclipsing variable star. Its components have diameters 1,400 and 1,200 times larger than our Sun. Its absolute brightness is approximately -11. \ No newline at end of file diff --git a/en/star/Struve_1095.md b/en/star/Struve_1095.md new file mode 100644 index 000000000..a12bb28b9 --- /dev/null +++ b/en/star/Struve_1095.md @@ -0,0 +1,9 @@ +--- +name: Struve 1095 +constellation: CMi +created_by: editor.cs +created_date: 2023-11-05 16:36:40.117477 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:40.117494 +--- +A binary star for a smaller telescope, two stars with magnitudes of 8.4 and 8.9 are located in the sky at a distance of 10.1". Although it is relatively faint, it can be easily found as it is located 12' SW of γ Canis Minoris and 25' north of β Canis Minoris. When using a magnification of 100x, it appears as a charming small pair with a white primary and a blue secondary component. \ No newline at end of file diff --git a/en/star/Struve_1104.md b/en/star/Struve_1104.md new file mode 100644 index 000000000..f78ff9a17 --- /dev/null +++ b/en/star/Struve_1104.md @@ -0,0 +1,9 @@ +--- +name: Struve 1104 +constellation: Pup +created_by: editor.cs +created_date: 2023-11-05 15:40:24.898728 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:24.898732 +--- +A beautiful, but tight pair of golden yellow stars, which however requires good seeing for clear resolution. The brightness components of 6.4mag and 7.5mag are separated by 2.1". \ No newline at end of file diff --git a/en/star/Struve_1149.md b/en/star/Struve_1149.md new file mode 100644 index 000000000..b53b026d4 --- /dev/null +++ b/en/star/Struve_1149.md @@ -0,0 +1,9 @@ +--- +name: Struve 1149 +constellation: CMi +created_by: editor.cs +created_date: 2023-11-05 16:41:47.788095 +updated_by: editor.cs +updated_date: 2023-11-05 16:41:47.788099 +--- +Double star observed 3 degrees southeast of Procyon, at the western end of the V-Z band of bright stars. In small telescopes, a nice yellow 7.6 magnitude and a blue component of 9.6 magnitude will be visible, a fainter copy of the star Eta in Cassiopeia. In larger magnifications, the companion may take on a purplish hue. Separation is 21.7". \ No newline at end of file diff --git a/en/star/Struve_1441.md b/en/star/Struve_1441.md new file mode 100644 index 000000000..5c131e696 --- /dev/null +++ b/en/star/Struve_1441.md @@ -0,0 +1,9 @@ +--- +name: Struve 1441 +constellation: Sex +created_by: editor.cs +created_date: 2023-11-05 17:49:58.453446 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:58.453450 +--- +A tight, attractive pair that can be resolved with a telescope with an objective diameter of around 100mm at a separation of 2.6". The brighter orange component has a magnitude of 6.4, while the fainter blue component has a magnitude of 9.9. \ No newline at end of file diff --git a/en/star/Struve_1788.md b/en/star/Struve_1788.md new file mode 100644 index 000000000..c482d7374 --- /dev/null +++ b/en/star/Struve_1788.md @@ -0,0 +1,9 @@ +--- +name: Struve 1788 +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 15:01:36.791634 +updated_by: editor.cs +updated_date: 2023-11-05 15:01:36.791639 +--- +quadruple star, close pair of two beautiful yellow stars (6.5mag and 7.7mag) with a separation of 3.4 ", accompanied by two additional, much fainter components with magnitudes of 10.3 and 10.9mag. Recommendation: 100-150 mm and at least 100x magnification. \ No newline at end of file diff --git a/en/star/Struve_2303.md b/en/star/Struve_2303.md new file mode 100644 index 000000000..8f2d23bb5 --- /dev/null +++ b/en/star/Struve_2303.md @@ -0,0 +1,9 @@ +--- +name: Struve 2303 +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 17:52:41.912984 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:41.912988 +--- +A close binary star observed in the field of the Milky Way interwoven with dark nebulae. Components of 6.6mag and 9.1mag at a separation of 2.1" are a very good test of quality for small telescopes and require a minimum of 150x magnification. \ No newline at end of file diff --git a/en/star/Struve_2306.md b/en/star/Struve_2306.md new file mode 100644 index 000000000..f3f171d72 --- /dev/null +++ b/en/star/Struve_2306.md @@ -0,0 +1,9 @@ +--- +name: Struve 2306 +constellation: Sct +created_by: editor.cs +created_date: 2023-11-05 16:43:34.429567 +updated_by: editor.cs +updated_date: 2023-11-05 16:43:34.429571 +--- +The asterism is observed 1.75 degrees WSW from the star γ Scuti. The AB pair consists of a golden component (7.9 mag) and a blue component (8.6 mag), which are separated by 10.2". The companion is also a close pair that requires a relatively high magnification for resolution. \ No newline at end of file diff --git a/en/star/Struve_2373.md b/en/star/Struve_2373.md new file mode 100644 index 000000000..2dccba9a2 --- /dev/null +++ b/en/star/Struve_2373.md @@ -0,0 +1,9 @@ +--- +name: Struve 2373 +constellation: Sct +created_by: editor.cs +created_date: 2023-11-05 17:53:20.173370 +updated_by: editor.cs +updated_date: 2023-11-05 17:53:20.173374 +--- +Double star located in a rich field of stars in the Milky Way. It consists of two yellow components with magnitudes of 7.2 and 8.2, which are separated by a distance of 4.2". A reasonable minimum for resolution will be a telescope with a 10 cm objective diameter. \ No newline at end of file diff --git a/en/star/Struve_2455.md b/en/star/Struve_2455.md new file mode 100644 index 000000000..62c67151c --- /dev/null +++ b/en/star/Struve_2455.md @@ -0,0 +1,9 @@ +--- +name: Struve 2455 +constellation: Vul +created_by: editor.cs +created_date: 2023-11-05 17:14:38.000151 +updated_by: editor.cs +updated_date: 2023-11-05 17:14:38.000156 +--- +In a 100 mm telescope, the triple star is an attractive pair of one white and two bluish components. The brightest components (7.4 mag and 8.5 mag) are separated by 6.6". Half a degree to the NNE, in the same field of view, there is the double star Struve 2457, consisting of a white 7.5 mag component and a bluish 9 mag component, separated by 10.3". \ No newline at end of file diff --git a/en/star/Struve_2540.md b/en/star/Struve_2540.md new file mode 100644 index 000000000..0f09a55cb --- /dev/null +++ b/en/star/Struve_2540.md @@ -0,0 +1,9 @@ +--- +name: Struve 2540 +constellation: Vul +created_by: editor.cs +created_date: 2023-11-05 18:08:11.030595 +updated_by: editor.cs +updated_date: 2023-11-05 18:08:11.030599 +--- +Constellation. In a 100/150 mm instrument, a relatively close pair (5.1") consists of unequally bright white component of magnitude 7.3 and a blue component of magnitude 8.8. The companion of magnitude 12.4 is located 147" away. \ No newline at end of file diff --git a/en/star/Struve_2653.md b/en/star/Struve_2653.md new file mode 100644 index 000000000..c812fb6a7 --- /dev/null +++ b/en/star/Struve_2653.md @@ -0,0 +1,9 @@ +--- +name: Struve 2653 +constellation: Vul +created_by: editor.cs +created_date: 2023-11-05 15:40:33.190048 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:33.190051 +--- +A binary star, in a telescope with an objective diameter of up to 150 mm, is a very close pair of unequally bright yellow-white stars (6.9 mag, 9.7 mag), which require appropriate magnification for resolution. They are separated by only 2.6". \ No newline at end of file diff --git a/en/star/Struve_2793.md b/en/star/Struve_2793.md new file mode 100644 index 000000000..0eaadbb31 --- /dev/null +++ b/en/star/Struve_2793.md @@ -0,0 +1,9 @@ +--- +name: Struve 2793 +constellation: Equ +created_by: editor.cs +created_date: 2023-11-05 17:55:49.698690 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:49.698693 +--- +An easily distinguishable double star, even for small telescopes. The primary component is yellow (7.8 mag) and the companion is blue (8.5 mag). They are separated by 26.6". The primary star has another companion at a distance of only 0.4", but it cannot be resolved using high magnification. \ No newline at end of file diff --git a/en/star/Struve_2902.md b/en/star/Struve_2902.md new file mode 100644 index 000000000..17c334962 --- /dev/null +++ b/en/star/Struve_2902.md @@ -0,0 +1,9 @@ +--- +name: Struve 2902 +constellation: Lac +created_by: editor.cs +created_date: 2023-11-05 15:40:02.485472 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:02.485477 +--- +Multiple star, brighter 6.4" close pair consists of a yellow component (7.6mag) and a white component (8.5mag). The second pair is located northeast and consists of two components with brightness of 12.1mag and 12.9mag at a separation of 5". In the same field of view, there are two more pairs. One in a closer separation, the other in a wider separation. To explore the surroundings, a telescope with a 150mm objective diameter is needed. \ No newline at end of file diff --git a/en/star/Struve_475.md b/en/star/Struve_475.md new file mode 100644 index 000000000..3e1c706fd --- /dev/null +++ b/en/star/Struve_475.md @@ -0,0 +1,9 @@ +--- +name: Struve 475 +constellation: Lac +created_by: editor.cs +created_date: 2023-11-05 16:48:45.359638 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:45.359642 +--- +nice unequally bright double star (6.8mag and 10.8mag). The brighter star has a white color, the fainter companion located at a separation of 15.5" is bluish. Immediately southwest, there is a faint pair of two components. \ No newline at end of file diff --git a/en/star/Sualocin_a_Rotanev.md b/en/star/Sualocin_a_Rotanev.md new file mode 100644 index 000000000..324b36c87 --- /dev/null +++ b/en/star/Sualocin_a_Rotanev.md @@ -0,0 +1,9 @@ +--- +name: Sualocin a Rotanev +constellation: Del +created_by: editor.cs +created_date: 2023-11-05 15:28:03.011565 +updated_by: editor.cs +updated_date: 2023-11-05 15:28:03.011571 +--- +The two brightest stars of the constellation, α (3.77 mag) and β Del (3.63 mag), are an example of the unquenchable human desire to leave something lasting behind. If we read the names of these stars backwards, we discover the words Nicolaus Venator, the Latin name of the Palermo astronomer Niccola Cacciatore, a long-time assistant to the famous Italian astronomer Giuseppe Piazzi. He greatly desired for his name to be preserved in the sky. He used a trick and gave his own name to these two stars, even though no one has the right to name a star after themselves. However, this lie was discovered too late, and the names had already become established. Even today, some atlases list them as names of unknown origin. They are the only stars in the sky that bear the name of a real person. \ No newline at end of file diff --git a/en/star/Sírius_B.md b/en/star/Sírius_B.md new file mode 100644 index 000000000..a62dff1fb --- /dev/null +++ b/en/star/Sírius_B.md @@ -0,0 +1,9 @@ +--- +name: Sírius B +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 17:14:25.606203 +updated_by: editor.cs +updated_date: 2023-11-05 17:14:25.606207 +--- +In 1834, Friedrich Bessel discovered that Sirius periodically deviates from its position, which could only mean one thing: the star is accompanied by an invisible companion. However, the telescopes of that time were not able to detect it. The big event occurred three decades later, in 1862, when the American optician Alvan G. Clark, an excellent telescope designer, discovered a faint star near Sirius while testing his new 460 mm refractor, later designated as Sirius B - also known as the "Pup" in Anglo-Saxon regions. However, it was not until 1915 that its true physical nature was determined, making it the first ever discovered white dwarf. \ No newline at end of file diff --git a/en/star/T_Borealis.md b/en/star/T_Borealis.md new file mode 100644 index 000000000..539ef804c --- /dev/null +++ b/en/star/T_Borealis.md @@ -0,0 +1,11 @@ +--- +name: T Borealis +constellation: Boo +created_by: editor.cs +created_date: 2023-11-05 15:04:12.111636 +updated_by: editor.cs +updated_date: 2023-11-05 15:04:12.111640 +--- +In April 1860, an unknown star with a magnitude of 9.7, later designated as T Borealis, was observed in the same field of view as Arcturus. Since then, no one has seen it, but it is not excluded that it may still reappear. It is believed to be a recurrent nova or an irregular variable star. Its position is 14:11 minutes, +19.18. + +Please note that the abbreviations for cardinal directions (N, W, S, E) should not be translated into their word equivalents. The combinations of cardinal direction abbreviations should always be translated into combinations of abbreviations in English, for example, ZSJ should be translated as WNW, VJV as ESE, JV as SE, ZJZ as WSW, VSV as ENE, SZ as NW, JJZ as SSW, SSV as NNE, SV as NE. The abbreviation for IAU constellation code should not be translated. "Boční vidění" should be translated as "averted vision". \ No newline at end of file diff --git a/en/star/T_Col.md b/en/star/T_Col.md new file mode 100644 index 000000000..9b430c05b --- /dev/null +++ b/en/star/T_Col.md @@ -0,0 +1,9 @@ +--- +name: T Col +constellation: Col +created_by: editor.cs +created_date: 2023-11-05 15:40:28.641694 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:28.641699 +--- +A variable star of the Mira type with a maximum magnitude of 6.7 and a minimum magnitude of 12.6. Its period is 266 days. \ No newline at end of file diff --git a/en/star/T_Pyxidis.md b/en/star/T_Pyxidis.md new file mode 100644 index 000000000..155fb03a9 --- /dev/null +++ b/en/star/T_Pyxidis.md @@ -0,0 +1,9 @@ +--- +name: T Pyxidis +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 17:13:16.565597 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:16.565601 +--- +One of the most famous objects in the constellation, a recurrent nova with a minimum magnitude of 16. During unexpected outbursts that occur every 12 to 25 years, its brightness increases to 6-7 magnitude. Such outbursts were recorded in 1890, 1902, 1920, 1944, and 1966. \ No newline at end of file diff --git a/en/star/T_Tauri.md b/en/star/T_Tauri.md new file mode 100644 index 000000000..4bbd64a9b --- /dev/null +++ b/en/star/T_Tauri.md @@ -0,0 +1,9 @@ +--- +name: T Tauri +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:48:33.674462 +updated_by: editor.cs +updated_date: 2023-11-05 17:48:33.674467 +--- +The observed 1.8 degrees west of ε Tauri, a star at the northern tip of the "V" of the Hyades, is a faint variable star of irregular period, with a mysterious emission / reflection nebula called Hind's Variable Nebula (NGC 1554-55). The brightness of the star changes unpredictably from 8.4 mag to 13.5 mag. T Tauri is a very young star, and NGC 1555 is likely a remnant of the cloud from which it was born. T Tauri and NGC 1555 are located within a relatively close complex of dark clouds in Taurus, about 450-500 light-years away, where other much fainter similar stars are found. \ No newline at end of file diff --git a/en/star/Trapéz.md b/en/star/Trapéz.md new file mode 100644 index 000000000..23c2a26ee --- /dev/null +++ b/en/star/Trapéz.md @@ -0,0 +1,9 @@ +--- +name: Trapéz +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 16:48:58.717559 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:58.717565 +--- +The "Theta system" is located in the heart of the Great Nebula in Orion and is one of the most famous multiple stars in the entire sky. Its four stars, ranging in brightness from 5th magnitude to 8th magnitude, form a quadrilateral called the Trapezium. Several 11th magnitude stars inside and around the quadrilateral undoubtedly belong physically to the Trapezium system. What's more, within a 5' area of the Trapezium, over 400 very faint stars are hidden, extremely young objects recently born from massive clouds of gas and dust. The stars of the Trapezium are exceptionally young, approximately 30,000 years old. \ No newline at end of file diff --git a/en/star/Tychova_hviezda.md b/en/star/Tychova_hviezda.md new file mode 100644 index 000000000..899aff740 --- /dev/null +++ b/en/star/Tychova_hviezda.md @@ -0,0 +1,9 @@ +--- +name: Tychova hviezda +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 17:46:54.753508 +updated_by: editor.cs +updated_date: 2023-11-05 17:46:54.753512 +--- +Supernova 1572, one of the three observed and documented supernovae that erupted in our Galaxy in the distant past. It was named after the Danish astronomer Tycho de Brahe, who observed its explosion on November 11, 1572, and the course of its brightness until it disappeared from the sky (it was also observed by Tadeáš Hájek z Hájku). At that time, he did not know that the star had exploded at a distance of 8,000 light-years. The star shone in close proximity to the northwest of the star κ Cas. At its peak, it reached an apparent magnitude equal to Venus, reaching a maximum brightness of -4.0 mag and was visible even during the day. Then its brightness decreased, but it could still be seen with the naked eye for a period of 16 months. Today, it is once again a star with an apparent brightness of less than 19 mag, with an expanding nebula, a radio and X-ray source of radiation. \ No newline at end of file diff --git a/en/star/UV_Aur.md b/en/star/UV_Aur.md new file mode 100644 index 000000000..f335aa895 --- /dev/null +++ b/en/star/UV_Aur.md @@ -0,0 +1,9 @@ +--- +name: UV Aur +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 17:13:48.350631 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:48.350635 +--- +Variable star, which changes its brightness between 7.4mag and 10.6mag over a period of 394.4 days. At a separation of 3.4", there is a companion of 11.5mag. It is a beautiful example of a combination of orange and blue components. \ No newline at end of file diff --git a/en/star/U_Ara.md b/en/star/U_Ara.md new file mode 100644 index 000000000..6714edbfa --- /dev/null +++ b/en/star/U_Ara.md @@ -0,0 +1,9 @@ +--- +name: U Ara +constellation: Ara +created_by: editor.cs +created_date: 2023-11-05 18:08:16.468740 +updated_by: editor.cs +updated_date: 2023-11-05 18:08:16.468744 +--- +A variable star of the Mira type, whose brightness is sufficient even for smaller telescopes - at maximum it reaches 8mag. However, in minimum its brightness decreases by a whole five magnitudes. It exhibits changes in a period of seven months. \ No newline at end of file diff --git a/en/star/U_Cep.md b/en/star/U_Cep.md new file mode 100644 index 000000000..d80f341e9 --- /dev/null +++ b/en/star/U_Cep.md @@ -0,0 +1,9 @@ +--- +name: U Cep +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 17:31:13.107784 +updated_by: editor.cs +updated_date: 2023-11-05 17:31:13.107790 +--- +The interesting short-period variable star. The brighter B-type component is eclipsed by a larger, but fainter G-type giant every 2.5 days. It changes in brightness from 6.7 mag to 9.2 mag, with a four-hour descent to minimum followed by two hours of total eclipse. Due to the close true separation, the brighter component pulls a significant amount of mass from the outer layer of the faint giant, resulting in a shortening of the orbital period by 4 minutes over the past century. The nearby third component appears to be part of the system as well, but it does not orbit along this path. \ No newline at end of file diff --git a/en/star/VW_Hyi.md b/en/star/VW_Hyi.md new file mode 100644 index 000000000..98c8fd031 --- /dev/null +++ b/en/star/VW_Hyi.md @@ -0,0 +1,9 @@ +--- +name: VW Hyi +constellation: Hyi +created_by: editor.cs +created_date: 2023-11-05 17:11:28.679082 +updated_by: editor.cs +updated_date: 2023-11-05 17:11:28.679086 +--- +The star, well known to observers of the southern sky as a cataclysmic variable. During its quiet period, it shines with a brightness of 13th magnitude, but during its brightening, which occurs once a month, it brightens to 8th magnitude. \ No newline at end of file diff --git a/en/star/V_Hya.md b/en/star/V_Hya.md new file mode 100644 index 000000000..8688d7ce0 --- /dev/null +++ b/en/star/V_Hya.md @@ -0,0 +1,9 @@ +--- +name: V Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 18:12:28.283714 +updated_by: editor.cs +updated_date: 2023-11-05 18:12:28.283718 +--- +A rare example of a carbon star. It is a red giant with a low temperature that produces carbon. The star is very red, so it cannot be confused with any other. However, it has one catch: it irregularly changes its brightness between 6th and 12th magnitude in two main periods - 18 months and 18 years. \ No newline at end of file diff --git a/en/star/V_Sge.md b/en/star/V_Sge.md new file mode 100644 index 000000000..ea6fa5d6b --- /dev/null +++ b/en/star/V_Sge.md @@ -0,0 +1,9 @@ +--- +name: V Sge +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 17:55:00.666682 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:00.666684 +--- +Probably once a "new star", today almost at the limit of visibility in a telescope. It is almost always different in brightness every night, its magnitude unpredictably ranging from 8.6 to 13.9. \ No newline at end of file diff --git a/en/star/Van_Maanenova_hviezda.md b/en/star/Van_Maanenova_hviezda.md new file mode 100644 index 000000000..a683ae8fd --- /dev/null +++ b/en/star/Van_Maanenova_hviezda.md @@ -0,0 +1,9 @@ +--- +name: Van Maanenova hviezda +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 15:27:38.026141 +updated_by: editor.cs +updated_date: 2023-11-05 15:27:38.026146 +--- +Wolf 28, a rare example of a relatively well-visible white dwarf, which requires a 200 mm telescope at its brightness of 12.3 mag. This one of the first discovered white dwarfs can be found near the star δ Psc. It is located in close proximity to our Sun, at a distance of 13.8 ly. \ No newline at end of file diff --git a/en/star/W_a_X_Sgr.md b/en/star/W_a_X_Sgr.md new file mode 100644 index 000000000..da4085fd2 --- /dev/null +++ b/en/star/W_a_X_Sgr.md @@ -0,0 +1,9 @@ +--- +name: W a X Sgr +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 15:17:15.323929 +updated_by: editor.cs +updated_date: 2023-11-05 15:17:15.323933 +--- +Cepheids, which change their brightness with a weekly period from the fourth to the fifth magnitude. X SGR is located near the border with the constellation of Sagittarius. It reaches a maximum of 4.3 mag and a minimum of 4.9 mag. Its period is 7.012 days. W SGR fluctuates between 4.3 mag and 5 mag in a period of 7.595 days. \ No newline at end of file diff --git a/en/star/Wolf_359.md b/en/star/Wolf_359.md new file mode 100644 index 000000000..59313c2f9 --- /dev/null +++ b/en/star/Wolf_359.md @@ -0,0 +1,9 @@ +--- +name: Wolf 359 +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 15:41:51.047775 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:51.047779 +--- +A faint star with a magnitude of 13.7, named after Max Wolf, who worked at Heidelberg University in the early 20th century and discovered its proper motion. It moves by 4.71" annually across the sky. One of the reasons for this apparent motion is its proximity to us. It is located at a distance of only 7.86 light-years from the Sun, making it our third closest star after Proxima Centauri and Barnard's Star in Ophiuchus. \ No newline at end of file diff --git a/en/star/Wolf_457.md b/en/star/Wolf_457.md new file mode 100644 index 000000000..dd53aa7de --- /dev/null +++ b/en/star/Wolf_457.md @@ -0,0 +1,9 @@ +--- +name: Wolf 457 +constellation: Dra +created_by: editor.cs +created_date: 2023-11-05 15:45:49.315329 +updated_by: editor.cs +updated_date: 2023-11-05 15:45:49.315333 +--- +White dwarf, one of the smallest known stars - its diameter is only 380 km. It is located 48.9 light-years away and from Earth, we see it as a 13mag object. \ No newline at end of file diff --git a/en/star/Z_Cam.md b/en/star/Z_Cam.md new file mode 100644 index 000000000..f6a6e039a --- /dev/null +++ b/en/star/Z_Cam.md @@ -0,0 +1,9 @@ +--- +name: Z Cam +constellation: Cam +created_by: editor.cs +created_date: 2023-11-05 17:43:12.879653 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:12.879657 +--- +A cataclysmic variable star, which jumps every two to three weeks from a minimum around 13mag to a maximum with a magnitude of 9.6mag. However, its similarity to other variable stars of this type ends there. Its magnitude can actually stop decreasing and remain at a medium brightness level for a very long time. It stays like this for several months before its magnitude starts increasing again - the star is therefore weakening. \ No newline at end of file diff --git a/en/star/Z_Cha.md b/en/star/Z_Cha.md new file mode 100644 index 000000000..fabdb7f6e --- /dev/null +++ b/en/star/Z_Cha.md @@ -0,0 +1,9 @@ +--- +name: Z Cha +constellation: Cha +created_by: editor.cs +created_date: 2023-11-05 16:29:47.696706 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:47.696711 +--- +A weaker variable star, which shines only as a 16.2 magnitude star at its minimum, so it can only be seen in a large telescope. However, every three to four months, it suddenly brightens and within a few hours its brightness increases to 11.5 magnitude. For several days, it can then be seen even in a 150 mm telescope. \ No newline at end of file diff --git a/en/star/h3945.md b/en/star/h3945.md new file mode 100644 index 000000000..072ecb0d7 --- /dev/null +++ b/en/star/h3945.md @@ -0,0 +1,9 @@ +--- +name: h3945 +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 15:43:07.924323 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:07.924330 +--- +Winter Albireo or Alamak. A beautiful double star composed of an orange 4.8 magnitude component and a blue component with a magnitude of 6.8. It can be resolved with a small telescope at a separation of 26.6". \ No newline at end of file diff --git a/en/star/hr1010.md b/en/star/hr1010.md new file mode 100644 index 000000000..10053fcdf --- /dev/null +++ b/en/star/hr1010.md @@ -0,0 +1,9 @@ +--- +name: ζ Ret +constellation: Ret +created_by: editor.cs +created_date: 2023-11-05 16:29:58.891920 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:58.891924 +--- +Optical binary star, whose components are similar to our Sun. Their brightness is 5.2mag and 5.5mag. At a distance of approximately 39 light years, we can distinguish them even with the naked eye. \ No newline at end of file diff --git a/en/star/hr1084.md b/en/star/hr1084.md new file mode 100644 index 000000000..71dc7b98f --- /dev/null +++ b/en/star/hr1084.md @@ -0,0 +1,9 @@ +--- +name: ε Eri +constellation: Eri +created_by: editor.cs +created_date: 2023-11-05 15:42:16.430554 +updated_by: editor.cs +updated_date: 2023-11-05 15:42:16.430558 +--- +This solitary dwarf star (3.7 mag) is essentially similar to our Sun in size, spectral type, and luminosity. It has a small rotational velocity, suggesting the possibility of having planets around it. ε Eri is the third closest star, visible to the naked eye at a distance of 10.76 light-years. Radio telescopes are monitoring it in search of potential signals from a civilization that could potentially inhabit one of the presumed planets. \ No newline at end of file diff --git a/en/star/hr1175.md b/en/star/hr1175.md new file mode 100644 index 000000000..d3c281dbb --- /dev/null +++ b/en/star/hr1175.md @@ -0,0 +1,9 @@ +--- +name: β Ret +constellation: Ret +created_by: editor.cs +created_date: 2023-11-05 15:01:12.884776 +updated_by: editor.cs +updated_date: 2023-11-05 15:01:12.884779 +--- +The main component has a brightness of 3.85 mag and its companion with a magnitude of 8.1 mag is located at a distance of 14". It is located at a distance of 100 light years. \ No newline at end of file diff --git a/en/star/hr1203.md b/en/star/hr1203.md new file mode 100644 index 000000000..5f25015e3 --- /dev/null +++ b/en/star/hr1203.md @@ -0,0 +1,9 @@ +--- +name: ζ Per +constellation: Per +created_by: editor.cs +created_date: 2023-11-05 17:53:08.867541 +updated_by: editor.cs +updated_date: 2023-11-05 17:53:08.867546 +--- +A binary star in an interesting setting. The companion, with a magnitude of 9.5, is located at a distance of 12.9" from the main pale blue component with a brightness of 2.9 magnitude, and there are two other stars nearby in the same field of view. The first star, with a magnitude of 11, is located at a separation of 33", while the second star, with a magnitude of 9.5, is at a distance of 94". It is located 750 light-years away. The closest star shares a common proper motion with the main component. \ No newline at end of file diff --git a/en/star/hr1208.md b/en/star/hr1208.md new file mode 100644 index 000000000..d7a7de950 --- /dev/null +++ b/en/star/hr1208.md @@ -0,0 +1,9 @@ +--- +name: γ Hyi +constellation: Hyi +created_by: editor.cs +created_date: 2023-11-05 15:41:47.892930 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:47.892934 +--- +The red giant of spectral class M2, which has a brightness of 3.2 mag, is located 214 light-years away from us. \ No newline at end of file diff --git a/en/star/hr1220.md b/en/star/hr1220.md new file mode 100644 index 000000000..1920cd2d7 --- /dev/null +++ b/en/star/hr1220.md @@ -0,0 +1,9 @@ +--- +name: ε Per +constellation: Per +created_by: editor.cs +created_date: 2023-11-05 16:40:49.298814 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:49.298818 +--- +The binary star, with a brightness companion of 8.1 magnitude, is located at a distance of 8.8" from the primary component (2.9 magnitude). The primary component is 2,500 times brighter than our Sun. It can be resolved with a telescope with a 6cm objective diameter. It is located 640 light-years away. \ No newline at end of file diff --git a/en/star/hr1239.md b/en/star/hr1239.md new file mode 100644 index 000000000..82422fcd6 --- /dev/null +++ b/en/star/hr1239.md @@ -0,0 +1,9 @@ +--- +name: λ Tau +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:48:20.214112 +updated_by: editor.cs +updated_date: 2023-11-05 17:48:20.214116 +--- +An eclipsing variable star of Algol type, with a magnitude fluctuation from 3.3 to 3.8 in a period of 3.95 days. Suitable comparison stars are γ (3.6 mag), μ (4.3 mag), ο (3.6 mag), and ζ (3.7 mag). λ Tau is actually much brighter than Algol, but it is located at a much greater distance (480 light years). Its light variations were first observed by J. Baxendell from England in 1848. \ No newline at end of file diff --git a/en/star/hr126.md b/en/star/hr126.md new file mode 100644 index 000000000..d70006f65 --- /dev/null +++ b/en/star/hr126.md @@ -0,0 +1,9 @@ +--- +name: β Tuc +constellation: Tuc +created_by: editor.cs +created_date: 2023-11-05 16:45:27.566735 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:27.566739 +--- +not only an optical, but also a physical binary star. Two almost equally bright components with magnitudes of 4.4 and 4.5 are separated by 27.1", so we can distinguish them well in a good binocular. Both are further doubled, which we can only perceive in a telescope. Additionally, at a distance of 9.3' to the southeast, we can observe a third component with a magnitude of 5.1, which is actually also a close binary star. \ No newline at end of file diff --git a/en/star/hr1298.md b/en/star/hr1298.md new file mode 100644 index 000000000..14070f9b1 --- /dev/null +++ b/en/star/hr1298.md @@ -0,0 +1,9 @@ +--- +name: Keid (ο2 Eri) +constellation: Eri +created_by: editor.cs +created_date: 2023-11-05 15:44:59.671930 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:59.671935 +--- +Interesting triple star system, consisting of a yellow star (4.4 mag) similar to our Sun, and another component at a separation of 83.4", which can be clearly resolved into two stars in a larger telescope: a red star (11.2 mag) and a white dwarf (9.4 mag), currently separated by 7.6". Try to distinguish them with a 100 mm telescope. \ No newline at end of file diff --git a/en/star/hr1311.md b/en/star/hr1311.md new file mode 100644 index 000000000..6d9b3e003 --- /dev/null +++ b/en/star/hr1311.md @@ -0,0 +1,9 @@ +--- +name: 47 Tau +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:52:35.269836 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:35.269841 +--- +A close binary star, even for a telescope with a 200mm objective diameter. Up to 200x magnification will reveal two yellow stars with magnitudes of 4.9 and 7.4, located at a separation of only 1.1". Another star with a magnitude of 12 is located 30" away. \ No newline at end of file diff --git a/en/star/hr1326.md b/en/star/hr1326.md new file mode 100644 index 000000000..c2eaaecd8 --- /dev/null +++ b/en/star/hr1326.md @@ -0,0 +1,9 @@ +--- +name: α Hor +constellation: Hor +created_by: editor.cs +created_date: 2023-11-05 16:33:10.410332 +updated_by: editor.cs +updated_date: 2023-11-05 16:33:10.410335 +--- +The brightest star of the constellation is colored orange and has an apparent magnitude of 3.83. It marks the pendulum in the sky. It is 1,500 Kelvin cooler than our Sun. Therefore, its spectrum contains a large number of metal lines and molecular absorption bands that are only found in the spectra of cool stars. It is located at a distance of 117 light-years. \ No newline at end of file diff --git a/en/star/hr1336.md b/en/star/hr1336.md new file mode 100644 index 000000000..9bf7a88fc --- /dev/null +++ b/en/star/hr1336.md @@ -0,0 +1,9 @@ +--- +name: α Ret +constellation: Ret +created_by: editor.cs +created_date: 2023-11-05 14:50:12.837439 +updated_by: editor.cs +updated_date: 2023-11-05 14:50:12.837443 +--- +The brightest star of the constellation has an apparent magnitude of 3.36. It belongs to the spectral class G6 and is faintly yellowish. At an angular distance of 48.5", there is a companion of magnitude 12. It is located 163 light-years away. \ No newline at end of file diff --git a/en/star/hr1348.md b/en/star/hr1348.md new file mode 100644 index 000000000..4d6381ebd --- /dev/null +++ b/en/star/hr1348.md @@ -0,0 +1,9 @@ +--- +name: φ Tau +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:12:52.671519 +updated_by: editor.cs +updated_date: 2023-11-05 17:12:52.671522 +--- +It consists of two stars with magnitudes 5 and 8.4 at a mutual distance of 52.1". A good binocular is sufficient to resolve both components. In a small telescope, we can also observe a yellow or blue tint. \ No newline at end of file diff --git a/en/star/hr1355.md b/en/star/hr1355.md new file mode 100644 index 000000000..bc88aa4f2 --- /dev/null +++ b/en/star/hr1355.md @@ -0,0 +1,9 @@ +--- +name: ε Ret +constellation: Ret +created_by: editor.cs +created_date: 2023-11-05 16:42:50.745023 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:50.745027 +--- +Double star composed of a primary component with a brightness of 4.4 magnitude and a faint companion with a magnitude of 12.5, which is located at a separation of 13.7". The system is located at a distance of 60 light years. \ No newline at end of file diff --git a/en/star/hr1412.md b/en/star/hr1412.md new file mode 100644 index 000000000..7be98a3a6 --- /dev/null +++ b/en/star/hr1412.md @@ -0,0 +1,9 @@ +--- +name: θ Tau +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 16:42:08.135819 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:08.135823 +--- +A wide double star in the Hyades visible to the naked eye. It consists of two bright components with magnitudes of 3.6 and 4, separated by 337". The brighter component is white, and the companion is orange. They are separated by 15 light-years, but it is highly likely that they have a common origin. \ No newline at end of file diff --git a/en/star/hr1457.md b/en/star/hr1457.md new file mode 100644 index 000000000..78fd1c6c2 --- /dev/null +++ b/en/star/hr1457.md @@ -0,0 +1,9 @@ +--- +name: Aldebaran (α Tau) +constellation: Tau +created_by: editor.cs +created_date: 2023-11-05 17:55:05.701246 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:05.701250 +--- +The brightest star of the constellation (0.85 mag). An orange giant of spectral class K5, its name is of Arabic origin and means "another" - because it appears after the Pleiades and follows them in their daily motion from east to west. It is located 65 light-years away from us and represents the eye of the Bull in the sky. Its actual luminosity reaches 125 times the luminosity of the Sun. It coincidentally appears to be projected onto the open star cluster Hyades, which actually lies beyond it. \ No newline at end of file diff --git a/en/star/hr1465.md b/en/star/hr1465.md new file mode 100644 index 000000000..06dc779c4 --- /dev/null +++ b/en/star/hr1465.md @@ -0,0 +1,9 @@ +--- +name: α Dor +constellation: Dor +created_by: editor.cs +created_date: 2023-11-05 15:44:04.067453 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:04.067456 +--- +The brightest star of the constellation has an apparent magnitude of 3.47. In reality, it is a close binary star, as there is a companion with a magnitude of 9.8 located 77.7" away from the primary component. It is located at a distance of 176 light-years. \ No newline at end of file diff --git a/en/star/hr15.md b/en/star/hr15.md new file mode 100644 index 000000000..20843e67c --- /dev/null +++ b/en/star/hr15.md @@ -0,0 +1,9 @@ +--- +name: Sirrah +constellation: Peg +created_by: editor.cs +created_date: 2023-11-05 17:45:19.049007 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:19.049010 +--- +The blue-white star on the border of Andromeda and Pegasus. It is interesting in that in the past it belonged to two constellations and had dual designations: α Andromedae (Sirrah) and δ Pegasi (Alpherratz). Today, it is classified in the constellation of Andromeda, although with its brightness of 2.06 mag, it is also the brightest star in the Pegasus Square. It is located 97 light-years away. \ No newline at end of file diff --git a/en/star/hr1502.md b/en/star/hr1502.md new file mode 100644 index 000000000..f9f07cd04 --- /dev/null +++ b/en/star/hr1502.md @@ -0,0 +1,9 @@ +--- +name: α Cae +constellation: Cae +created_by: editor.cs +created_date: 2023-11-05 16:24:50.799990 +updated_by: editor.cs +updated_date: 2023-11-05 16:24:50.799994 +--- +The brightest star of the constellation, although it only reaches a magnitude of 4.52. In reality, it is a binary star, with a companion of magnitude 12.4 located at a separation of 6.6". However, we would need a larger telescope to verify this. The system is located at a distance of 66 light-years from us. \ No newline at end of file diff --git a/en/star/hr154.md b/en/star/hr154.md new file mode 100644 index 000000000..a320dcafb --- /dev/null +++ b/en/star/hr154.md @@ -0,0 +1,9 @@ +--- +name: π Andromedae +constellation: And +created_by: editor.cs +created_date: 2023-11-05 17:16:07.836629 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:07.836633 +--- +A binary star (with stars of 4.4 magnitude and 8.6 magnitude, angular separation of 35.9'') can be resolved with a small telescope with a 6 cm objective diameter. The primary component has an absolute magnitude of -1.1, is 170 times more luminous than the Sun, and is located at a distance of 600 light-years. In a telescope with a 200mm objective diameter, it appears as a bright white star with a faint bluish companion. A faint star of magnitude 13 is also projected in the vicinity. \ No newline at end of file diff --git a/en/star/hr1542.md b/en/star/hr1542.md new file mode 100644 index 000000000..40e13ff6d --- /dev/null +++ b/en/star/hr1542.md @@ -0,0 +1,9 @@ +--- +name: α Cam +constellation: Cam +created_by: editor.cs +created_date: 2023-11-05 17:12:30.708950 +updated_by: editor.cs +updated_date: 2023-11-05 17:12:30.708954 +--- +In the sky, it appears as a 4.3 magnitude star. However, in reality, this blue supergiant of spectral class O is 620,000 times brighter than the Sun. It is located approximately 6,000 thousand light-years away from us. \ No newline at end of file diff --git a/en/star/hr1563.md b/en/star/hr1563.md new file mode 100644 index 000000000..ce9f4b566 --- /dev/null +++ b/en/star/hr1563.md @@ -0,0 +1,9 @@ +--- +name: ι Pic +constellation: Pic +created_by: editor.cs +created_date: 2023-11-05 14:48:41.687868 +updated_by: editor.cs +updated_date: 2023-11-05 14:48:41.687871 +--- +Double star easily distinguishable with a small telescope. It consists of components with magnitudes 5.6 and 6.4, separated by 12.3 arcseconds. \ No newline at end of file diff --git a/en/star/hr1603.md b/en/star/hr1603.md new file mode 100644 index 000000000..bf3ad2099 --- /dev/null +++ b/en/star/hr1603.md @@ -0,0 +1,9 @@ +--- +name: β Cam +constellation: Cam +created_by: editor.cs +created_date: 2023-11-05 17:57:24.078985 +updated_by: editor.cs +updated_date: 2023-11-05 17:57:24.078989 +--- +The brightest star of the constellation has an apparent magnitude of 4.22. This yellow supergiant of spectral class G0 is located 870 light-years away and shines 1,600 times brighter than our Sun. The surface temperature reaches 30,000 Kelvin. \ No newline at end of file diff --git a/en/star/hr1605.md b/en/star/hr1605.md new file mode 100644 index 000000000..838f2c540 --- /dev/null +++ b/en/star/hr1605.md @@ -0,0 +1,9 @@ +--- +name: Al Anz (ε Aur) +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 17:16:27.640974 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:27.640978 +--- +One of the three stars of the Goat, which belongs to the remarkable eclipsing variable stars of the Algol type. It consists of a bright white giant, 37,000 times more luminous than the Sun, and a dark companion, which is not visually observable. Both stars are in mutual orbit. Every 27 years - 9,883 days - the dark component passes in front of the giant and obscures a large part of its light, causing the star ε Aur to significantly darken in the sky - from 3.1 magnitude to 3.8 magnitude. This dimming lasts for several months - about 190 days, then the star remains at a minimum for about half a year, and in the next 190 days it grows from the minimum to the maximum. This suggests that the companion must be surrounded by a dark cloud of gas and dust. The last such eclipse occurred in 2009. Among the known eclipsing variables, it exhibits one of the longest periods. \ No newline at end of file diff --git a/en/star/hr1612.md b/en/star/hr1612.md new file mode 100644 index 000000000..d3ea38ef9 --- /dev/null +++ b/en/star/hr1612.md @@ -0,0 +1,9 @@ +--- +name: Sadatoni (ζ Aur) +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 17:18:30.768106 +updated_by: editor.cs +updated_date: 2023-11-05 17:18:30.768109 +--- +The next eclipsing variable star from the constellation of the Kids, with a magnitude change from 3.9mag to 4.2mag in a period of 2.66 years - 972.18 days, with the second longest known period. The brightness decrease from maximum to minimum, or the increase from minimum to maximum, lasts only a few days, and the star remains at minimum for 38 days. The main component is red, the secondary component is blue. Sometimes, faint blue stars come to us through the outer layers of a red giant, creating interesting spectroscopic phenomena. \ No newline at end of file diff --git a/en/star/hr1629.md b/en/star/hr1629.md new file mode 100644 index 000000000..a1e8088cc --- /dev/null +++ b/en/star/hr1629.md @@ -0,0 +1,9 @@ +--- +name: η Men +constellation: Men +created_by: editor.cs +created_date: 2023-11-05 16:47:01.843178 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:01.843183 +--- +A star with an apparent magnitude of 5.5, which is located 700 light-years away from us. \ No newline at end of file diff --git a/en/star/hr1652.md b/en/star/hr1652.md new file mode 100644 index 000000000..77f58dac7 --- /dev/null +++ b/en/star/hr1652.md @@ -0,0 +1,9 @@ +--- +name: γ Cae +constellation: Cae +created_by: editor.cs +created_date: 2023-11-05 16:31:15.640926 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:15.640931 +--- +Double star distinguishable only with a larger telescope. The main yellow-orange star with a brightness of 4.7mag has a companion at a separation of 2.9 arcseconds with a brightness of 8.5mag. \ No newline at end of file diff --git a/en/star/hr167.md b/en/star/hr167.md new file mode 100644 index 000000000..b618bdd98 --- /dev/null +++ b/en/star/hr167.md @@ -0,0 +1,9 @@ +--- +name: 55 Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 16:40:34.859821 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:34.859825 +--- +A nice double star, in which the primary component has a brightness of 5.6 mag and the companion 8.8 mag. Since they are separated by 6.6", we need a telescope with an objective diameter of at least 6 cm to resolve them. The contrast is intense, with one component having a yellow-orange color and the other a blue color. \ No newline at end of file diff --git a/en/star/hr1677.md b/en/star/hr1677.md new file mode 100644 index 000000000..e76ffc406 --- /dev/null +++ b/en/star/hr1677.md @@ -0,0 +1,9 @@ +--- +name: β Men +constellation: Men +created_by: editor.cs +created_date: 2023-11-05 16:44:47.193471 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:47.193476 +--- +A star with a magnitude of 5.3 on the edge of the Large Magellanic Cloud, but it belongs to our galaxy. It is located 200 light-years away. \ No newline at end of file diff --git a/en/star/hr168.md b/en/star/hr168.md new file mode 100644 index 000000000..80921bc1f --- /dev/null +++ b/en/star/hr168.md @@ -0,0 +1,9 @@ +--- +name: Schedar (α Cassiopeiae) +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 17:44:46.365163 +updated_by: editor.cs +updated_date: 2023-11-05 17:44:46.365166 +--- +This orange star, located 228 light years away, is 676 times brighter than our Sun, but it appears only as a 2.23 magnitude star in the sky (the actual magnitude varies by a few tenths). \ No newline at end of file diff --git a/en/star/hr1705.md b/en/star/hr1705.md new file mode 100644 index 000000000..4ad8ede1c --- /dev/null +++ b/en/star/hr1705.md @@ -0,0 +1,9 @@ +--- +name: κ Lep +constellation: Lep +created_by: editor.cs +created_date: 2023-11-05 17:45:45.677212 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:45.677215 +--- +This binary star is composed of components with magnitudes 4.5 and 7.4, which are separated by an angular distance of 2.6". To resolve them, a telescope with an objective diameter of at least 15 cm is needed. At approximately 115x magnification, both components appear white. Only in a larger telescope will the companion acquire a blue color. \ No newline at end of file diff --git a/en/star/hr1706.md b/en/star/hr1706.md new file mode 100644 index 000000000..286293028 --- /dev/null +++ b/en/star/hr1706.md @@ -0,0 +1,9 @@ +--- +name: 14 Aur +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 17:55:37.405440 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:37.405443 +--- +The asterism, main, bright yellow component with a magnitude of 5.2mag is located at a separation of 14.6 arcseconds from a pale blue companion with a magnitude of 7.4mag. In a larger telescope, a third, fainter companion located in a sparse star field is also visible. \ No newline at end of file diff --git a/en/star/hr1708.md b/en/star/hr1708.md new file mode 100644 index 000000000..e8950ffa0 --- /dev/null +++ b/en/star/hr1708.md @@ -0,0 +1,9 @@ +--- +name: Capella (α Aur) +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 16:28:28.560775 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:28.560780 +--- +The brightest star of the constellation and the sixth brightest star in the sky (0.1mag). It never sets in our location. It is the northernmost star in the Winter Hexagon of bright stars. We can easily spot its yellow hue with the naked eye. It is located 43 light-years away and its actual luminosity is 160 times greater than that of the Sun. It is one of the most well-known spectroscopic binary stars, orbiting around a common center, with a period of 108 days. In terms of spectrum and surface temperature, they are comparable to our Sun. The mass reaches 2.5 times, respectively, the mass of the Sun, with one star being 78 times and the other 72 times brighter than the Sun. \ No newline at end of file diff --git a/en/star/hr183.md b/en/star/hr183.md new file mode 100644 index 000000000..e99e626d9 --- /dev/null +++ b/en/star/hr183.md @@ -0,0 +1,9 @@ +--- +name: ξ Phe +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 15:04:06.085350 +updated_by: editor.cs +updated_date: 2023-11-05 15:04:06.085354 +--- +A well-resolvable double star for a telescope with an objective diameter of around 100 mm. The primary component has a brightness of 6 mag, while the companion is at a separation of 13.2" and has a brightness of 10 mag. \ No newline at end of file diff --git a/en/star/hr1852.md b/en/star/hr1852.md new file mode 100644 index 000000000..71c8395d2 --- /dev/null +++ b/en/star/hr1852.md @@ -0,0 +1,9 @@ +--- +name: Mintaka (δ Ori) +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 17:12:36.664112 +updated_by: editor.cs +updated_date: 2023-11-05 17:12:36.664115 +--- +The right blue-white star of the belt near the celestial equator. It is one of the easiest distinguishable pairs - a telescope with a diameter of at least 5 cm will be sufficient. We will see the pale blue guide of magnitude 6.9 next to the main component at a separation of 52.6". It is likely a true binary star, even though the components are separated by half a light-year. Their mutual orbital period could therefore last up to a million years. The system is located at a distance of 2,350 light-years. Additionally, the main component is a variable star, but with a very small change in brightness (around 2.2 mag). \ No newline at end of file diff --git a/en/star/hr1865.md b/en/star/hr1865.md new file mode 100644 index 000000000..c53e26f07 --- /dev/null +++ b/en/star/hr1865.md @@ -0,0 +1,9 @@ +--- +name: Arneb (α Lep) +constellation: Lep +created_by: editor.cs +created_date: 2023-11-05 15:16:35.413123 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:35.413127 +--- +The brightest star in the constellation (2.58mag) is located 2200 light-years away. It is a supergiant 32,000 times brighter than the Sun. At an angular distance of 36", it contains a faint companion of magnitude 11. \ No newline at end of file diff --git a/en/star/hr1879.md b/en/star/hr1879.md new file mode 100644 index 000000000..ee9ce39a4 --- /dev/null +++ b/en/star/hr1879.md @@ -0,0 +1,9 @@ +--- +name: λ Ori +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 17:45:28.532682 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:28.532686 +--- +The white companions have magnitudes of 3.5 and 5.6, with a separation of 4.4". Two additional, bluish companions are located at distances of 28" and 78" from this pair, respectively. λ Ori designates the head of Orion and forms an interesting triangle with π-1 and π-2 Ori. Both of them have a magnitude of 4. \ No newline at end of file diff --git a/en/star/hr1899.md b/en/star/hr1899.md new file mode 100644 index 000000000..340bce4d3 --- /dev/null +++ b/en/star/hr1899.md @@ -0,0 +1,9 @@ +--- +name: ι Ori +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 17:46:32.952611 +updated_by: editor.cs +updated_date: 2023-11-05 17:46:32.952616 +--- +nice triple star suitable even for small telescopes. Next to the main white component (2.8mag) there is a faint blue companion (7.3mag) at a separation of 11.3". Another, reddish companion (11mag) is observed at a distance of 50" from this pair. The finder also shows a wide double star Struve 747, consisting of bright components with magnitudes 4.8 and 5.7. \ No newline at end of file diff --git a/en/star/hr191.md b/en/star/hr191.md new file mode 100644 index 000000000..fc4785f2a --- /dev/null +++ b/en/star/hr191.md @@ -0,0 +1,9 @@ +--- +name: η Phe +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 16:38:47.854080 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:47.854084 +--- +A binary star, whose components have a brightness difference of 19.8". The brighter one reaches a magnitude of 4.5, while the companion exhibits an 11th magnitude. \ No newline at end of file diff --git a/en/star/hr1922.md b/en/star/hr1922.md new file mode 100644 index 000000000..c2138b583 --- /dev/null +++ b/en/star/hr1922.md @@ -0,0 +1,9 @@ +--- +name: β Dor +constellation: Dor +created_by: editor.cs +created_date: 2023-11-05 17:31:24.635692 +updated_by: editor.cs +updated_date: 2023-11-05 17:31:24.635696 +--- +The variable Cepheid, which reaches a maximum brightness of 3.8mag and decreases to 4.6mag at minimum with a period of 9.84 days. This yellow-white supergiant is located at a distance of approximately 1,000 light-years. The suitable comparison star is delta Dor, which has a magnitude of 4.35mag. \ No newline at end of file diff --git a/en/star/hr1931.md b/en/star/hr1931.md new file mode 100644 index 000000000..a37c06fec --- /dev/null +++ b/en/star/hr1931.md @@ -0,0 +1,9 @@ +--- +name: σ Ori +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 17:17:52.183121 +updated_by: editor.cs +updated_date: 2023-11-05 17:17:52.183126 +--- +With a telescope with a 5 cm objective diameter, we can detect two companions to the main white component with a magnitude of 3.81. The first companion has a magnitude of 6 and is located at a separation of 41". The second companion has a magnitude of 7 and is separated by 13". In a telescope with an objective diameter of around 15 cm, a companion with a magnitude of 10 is added at a separation of 11". Another companion with a magnitude of 6 is located very close to the main component, at a distance of 0.2", but only it is physically associated with the main component. \ No newline at end of file diff --git a/en/star/hr1948.md b/en/star/hr1948.md new file mode 100644 index 000000000..7fe09e694 --- /dev/null +++ b/en/star/hr1948.md @@ -0,0 +1,9 @@ +--- +name: Alnitak (ζ Ori) +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 16:27:12.772617 +updated_by: editor.cs +updated_date: 2023-11-05 16:27:12.772621 +--- +The left star of Orion's belt is actually a triple star system. Close to the main component with a brightness of 1.9 magnitude, there is a companion with a brightness of 4.2 magnitude at a separation of 2.7 arcseconds. At an angular distance of 57 arcseconds, there is another star with a brightness of 9 magnitude, which is likely only projected near Alnitak. All components have a blue-white color. \ No newline at end of file diff --git a/en/star/hr1953.md b/en/star/hr1953.md new file mode 100644 index 000000000..17b80a6ad --- /dev/null +++ b/en/star/hr1953.md @@ -0,0 +1,9 @@ +--- +name: γ Men +constellation: Men +created_by: editor.cs +created_date: 2023-11-05 17:47:28.315118 +updated_by: editor.cs +updated_date: 2023-11-05 17:47:28.315122 +--- +The brightest star of the constellation has a magnitude of 5.06. It is a giant star of spectral class K4 located 100 light years away. \ No newline at end of file diff --git a/en/star/hr1956.md b/en/star/hr1956.md new file mode 100644 index 000000000..6dd3a5e04 --- /dev/null +++ b/en/star/hr1956.md @@ -0,0 +1,9 @@ +--- +name: Phakt (α Col) +constellation: Col +created_by: editor.cs +created_date: 2023-11-05 17:16:21.634991 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:21.634995 +--- +The brightest star of the constellation. The main pale blue component with a magnitude of 2.64 has a companion of 11 magnitude at a separation of 13.5 arcseconds, which can be seen with a 100mm telescope. The system is located 145 light-years away. \ No newline at end of file diff --git a/en/star/hr1983.md b/en/star/hr1983.md new file mode 100644 index 000000000..32cf22395 --- /dev/null +++ b/en/star/hr1983.md @@ -0,0 +1,9 @@ +--- +name: γ Lep +constellation: Lep +created_by: editor.cs +created_date: 2023-11-05 15:45:08.934608 +updated_by: editor.cs +updated_date: 2023-11-05 15:45:08.934613 +--- +This binary star system splits into two components, one reaching 3.7 magnitude (yellow) and the other 6.3 magnitude (orange). The components are separated by 96.3" and are roughly 29 light-years away from Earth. The star belongs to the stellar cluster of Ursa Major. \ No newline at end of file diff --git a/en/star/hr1992.md b/en/star/hr1992.md new file mode 100644 index 000000000..d34833f67 --- /dev/null +++ b/en/star/hr1992.md @@ -0,0 +1,9 @@ +--- +name: 29 Cam +constellation: Cam +created_by: editor.cs +created_date: 2023-11-05 16:40:22.563328 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:22.563332 +--- +A binary star suitable for a 100mm telescope. That it is a binary star is evident at 100x magnification. It appears as an unequal (6.5mag, 9.5mag) and contrasting pair of yellow and pale blue components. Their mutual distance is 25.1". \ No newline at end of file diff --git a/en/star/hr1996.md b/en/star/hr1996.md new file mode 100644 index 000000000..460a18198 --- /dev/null +++ b/en/star/hr1996.md @@ -0,0 +1,9 @@ +--- +name: μ Col +constellation: Col +created_by: editor.cs +created_date: 2023-11-05 15:02:40.205453 +updated_by: editor.cs +updated_date: 2023-11-05 15:02:40.205457 +--- +A very interesting star, one of a trio diverging from the constellation Orion. Along with the stars 53 Ari and AE Aur, it likely once formed a stellar system in the constellation Orion, with its fourth component exploding as a supernova 2-3 billion years ago, disrupting the stability of the remaining three, which are gradually moving away from their original position. In our Galaxy, μ Col moves at a speed of about 100 km/s. \ No newline at end of file diff --git a/en/star/hr2020.md b/en/star/hr2020.md new file mode 100644 index 000000000..b9f66780a --- /dev/null +++ b/en/star/hr2020.md @@ -0,0 +1,9 @@ +--- +name: β Pic +constellation: Pic +created_by: editor.cs +created_date: 2023-11-05 17:46:16.971164 +updated_by: editor.cs +updated_date: 2023-11-05 17:46:16.971168 +--- +One of the stars, which was found to be surrounded by a disk of cold matter - mainly dust and ice - according to the records of the IRAS satellite from 1983. The disk was later photographed from the Las Campanas Observatory in Chile using the 2.5-meter Irénée du Pond reflector. The disk is composed of similar material to that found during the formation of planets, and therefore this star could be a suitable center for a forming planetary system. On the other hand, its luminosity exceeds that of the Sun by up to 60 times. It is located at a distance of 78 light years. In the sky, it shines as a blue-white star of magnitude 4. \ No newline at end of file diff --git a/en/star/hr2061.md b/en/star/hr2061.md new file mode 100644 index 000000000..d1750e8fc --- /dev/null +++ b/en/star/hr2061.md @@ -0,0 +1,9 @@ +--- +name: Betelgeuse (α Ori) +constellation: Ori +created_by: editor.cs +created_date: 2023-11-05 15:43:16.741778 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:16.741781 +--- +This glowing red supergiant is a semi-regular variable star, with its brightness ranging from 0.4mag to 1.3mag in a period of approximately 5.7 years. However, it appears more orange in color. Betelgeuse is one of the largest stars visible to the naked eye. If it were located at the position of the Sun, its outer edge would extend all the way to the asteroid belt. It is located at a distance of 500-600 light-years. \ No newline at end of file diff --git a/en/star/hr2095.md b/en/star/hr2095.md new file mode 100644 index 000000000..97c88750d --- /dev/null +++ b/en/star/hr2095.md @@ -0,0 +1,9 @@ +--- +name: θ Aur +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 15:16:11.310509 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:11.310514 +--- +The triple star system, with components of brightness 2.6mag and 7.1mag, is separated by 3.6". In the field of view, there is also a third star at a separation of 45". To resolve the entire system, we need a telescope with an 8 cm diameter objective. \ No newline at end of file diff --git a/en/star/hr2176.md b/en/star/hr2176.md new file mode 100644 index 000000000..a58b6c387 --- /dev/null +++ b/en/star/hr2176.md @@ -0,0 +1,9 @@ +--- +name: 41 Aur +constellation: Aur +created_by: editor.cs +created_date: 2023-11-05 16:13:59.993317 +updated_by: editor.cs +updated_date: 2023-11-05 16:13:59.993321 +--- +A nice pair of white (6.3mag) and pale blue (7mag) components separated by 7.7" is distinguishable in a small telescope. The surroundings are complemented by the variable star 46 Aur, located 3 degrees to the ENE, which is distinctly orange. \ No newline at end of file diff --git a/en/star/hr2216.md b/en/star/hr2216.md new file mode 100644 index 000000000..5594904ee --- /dev/null +++ b/en/star/hr2216.md @@ -0,0 +1,9 @@ +--- +name: Tejat Prior (η Gem) +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 17:29:37.598236 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:37.598241 +--- +Red giant, a bright semi-regular variable star with a magnitude change from 3.1 to 3.9 in a period of approximately 223 days. It has a companion with a magnitude of 8.8 at a distance of 1.4". A good comparison star is μ Gem. It is located at a distance of 700 light years. \ No newline at end of file diff --git a/en/star/hr2261.md b/en/star/hr2261.md new file mode 100644 index 000000000..80a10a13a --- /dev/null +++ b/en/star/hr2261.md @@ -0,0 +1,9 @@ +--- +name: α Men +constellation: Men +created_by: editor.cs +created_date: 2023-11-05 17:52:14.767492 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:14.767497 +--- +The yellow dwarf similar to the Sun, located relatively close to us, is 28 light-years away. In the sky, we see it as a shining point with a magnitude of 5.1. \ No newline at end of file diff --git a/en/star/hr2293.md b/en/star/hr2293.md new file mode 100644 index 000000000..922da8431 --- /dev/null +++ b/en/star/hr2293.md @@ -0,0 +1,9 @@ +--- +name: 5 Lyn +constellation: Lyn +created_by: editor.cs +created_date: 2023-11-05 16:43:43.566424 +updated_by: editor.cs +updated_date: 2023-11-05 16:43:43.566427 +--- +The asterism, even in a smaller telescope, is a nice, wide pair of yellow 5.3 magnitude and blue 9.8 magnitude components, which are separated by 31.4". The third component, with a magnitude of 7.9, is separated by 96". Nearby, there is the double star 6 Lyn and two other wide pairs. The one located one degree northeast of 5 Lyn is composed of an orange and blue component, while the second one consists of two white components. \ No newline at end of file diff --git a/en/star/hr2356.md b/en/star/hr2356.md new file mode 100644 index 000000000..245fe8e1c --- /dev/null +++ b/en/star/hr2356.md @@ -0,0 +1,9 @@ +--- +name: β Mon +constellation: Mon +created_by: editor.cs +created_date: 2023-11-05 16:00:31.551896 +updated_by: editor.cs +updated_date: 2023-11-05 16:00:31.551900 +--- +The brightest star of the constellation has an apparent magnitude of 3.95. It belongs to a beautiful triple star system discovered by W. Herschel in 1781, whose all blue-white components can be resolved even with small telescopes as a small triangle. Two components with magnitudes of 4.7 and 5.2 are located at a separation of 7.3 arcseconds. A companion with a magnitude of 6.1 is situated at a distance of 2.8 arcseconds from the first component. The system is approximately 700 light-years away. With a larger telescope, we can also discover a star with a magnitude of 12 at a separation of 25.9 arcseconds. This entire system is designated as 11 Mon. \ No newline at end of file diff --git a/en/star/hr2451.md b/en/star/hr2451.md new file mode 100644 index 000000000..64c29c08e --- /dev/null +++ b/en/star/hr2451.md @@ -0,0 +1,9 @@ +--- +name: ν Pup +constellation: Pup +created_by: editor.cs +created_date: 2023-11-05 17:47:18.068595 +updated_by: editor.cs +updated_date: 2023-11-05 17:47:18.068598 +--- +An easily distinguishable double star is located just 26' NE of σ Puppis. The components of this pair have magnitudes of 4.7 and 5.1, with a separation of 4'. \ No newline at end of file diff --git a/en/star/hr2470.md b/en/star/hr2470.md new file mode 100644 index 000000000..14983d527 --- /dev/null +++ b/en/star/hr2470.md @@ -0,0 +1,9 @@ +--- +name: 12 Lyn +constellation: Lyn +created_by: editor.cs +created_date: 2023-11-05 16:42:23.964949 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:23.964953 +--- +A physical binary star composed of relatively equally bright components - 5.4mag and 6mag. They are separated by 1.8" and their orbital period is 907 years. At a distance of about 8.5" from the brighter component, there is another companion with a brightness of 7.5mag. \ No newline at end of file diff --git a/en/star/hr2491.md b/en/star/hr2491.md new file mode 100644 index 000000000..ceae784a5 --- /dev/null +++ b/en/star/hr2491.md @@ -0,0 +1,9 @@ +--- +name: Sírius (α CMa) +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 16:39:05.523944 +updated_by: editor.cs +updated_date: 2023-11-05 16:39:05.523947 +--- +The brightest star in the sky, known to almost all ancient civilizations, is Sirius. Orion's belt points towards Sirius, extending downwards. There, near the horizon, especially on cold winter nights, we can see a bright blue-white star flickering due to the restless atmosphere. After all, the Greek word "Sirios" means flickering, sparkling. Sirius has a magnitude of -1.5, but compared to other stars, it is not exceptionally luminous. It owes its brightness to its relatively close distance from us - 8.7 light-years, which ranks it fifth in the list of our closest stars (excluding companions). Its luminosity is 23 times greater, its diameter is 1.8 times larger, and its mass is 2.35 times greater than our Sun. Its surface temperature of 10,000 K gives it its blue-white color. \ No newline at end of file diff --git a/en/star/hr2550.md b/en/star/hr2550.md new file mode 100644 index 000000000..9fb18605a --- /dev/null +++ b/en/star/hr2550.md @@ -0,0 +1,9 @@ +--- +name: α Pic +constellation: Pic +created_by: editor.cs +created_date: 2023-11-05 17:12:49.726714 +updated_by: editor.cs +updated_date: 2023-11-05 17:12:49.726718 +--- +The brightest star of the constellation, shining as a point with a magnitude of 3.3. It is located 99 light-years away. \ No newline at end of file diff --git a/en/star/hr2564.md b/en/star/hr2564.md new file mode 100644 index 000000000..d20ad52be --- /dev/null +++ b/en/star/hr2564.md @@ -0,0 +1,9 @@ +--- +name: 38 Gem +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 15:46:44.209184 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:44.209188 +--- +The companions have a brightness of 4.7 mag and 7.7 mag and orbit each other once every approximately 3,190 years. At the turn of the century, their mutual separation was approximately 7.1", which can be comfortably separated by a telescope with an 8 cm objective diameter. One has a yellow color, the other has a light blue color. \ No newline at end of file diff --git a/en/star/hr258.md b/en/star/hr258.md new file mode 100644 index 000000000..dbc82beb7 --- /dev/null +++ b/en/star/hr258.md @@ -0,0 +1,9 @@ +--- +name: 36 Andromedae +constellation: And +created_by: editor.cs +created_date: 2023-11-05 16:44:36.468510 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:36.468514 +--- +A tight binary star (components 6mag and 6.4mag with a separation of 0.6"-1.4" over 165 years), which serves as a test for larger amateur telescopes. It is located 124 light-years away. The primary component is a giant many times brighter than our Sun. The companion, on the other hand, is very similar to the Sun. It has the same spectral type and the same color - a beautiful yellow. \ No newline at end of file diff --git a/en/star/hr2588.md b/en/star/hr2588.md new file mode 100644 index 000000000..25b6b9477 --- /dev/null +++ b/en/star/hr2588.md @@ -0,0 +1,9 @@ +--- +name: 17 CMa +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 17:01:06.219145 +updated_by: editor.cs +updated_date: 2023-11-05 17:01:06.219149 +--- +A very beautiful multiple star, even for a small telescope! A low magnification will reveal a stunning wide triple star with a white primary component of magnitude 5.8 and two orange companions forming a right-angled triangle. In the same field of view, a companion of magnitude 9.5 and the double star π Canis Majoris are observed. \ No newline at end of file diff --git a/en/star/hr2593.md b/en/star/hr2593.md new file mode 100644 index 000000000..f9fdb1a25 --- /dev/null +++ b/en/star/hr2593.md @@ -0,0 +1,9 @@ +--- +name: μ CMa +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 15:47:15.062443 +updated_by: editor.cs +updated_date: 2023-11-05 15:47:15.062446 +--- +In a small telescope, there is an unequally bright pair of stars in mutual contact, with a sparkling contrast of orange and blue color. In a larger telescope, we can separate them with a magnification of 175 times. The yellow component has a brightness of 5.3 magnitude, while the blue component with a brightness of 8.6 magnitude is located at a separation of 3 arcseconds. Two companions with a magnitude of 10 are located slightly further away. \ No newline at end of file diff --git a/en/star/hr2618.md b/en/star/hr2618.md new file mode 100644 index 000000000..b3a93660e --- /dev/null +++ b/en/star/hr2618.md @@ -0,0 +1,9 @@ +--- +name: Adara (ε CMa) +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 15:03:33.707973 +updated_by: editor.cs +updated_date: 2023-11-05 15:03:33.707976 +--- +A binary star, with its companion of magnitude 8.1 lying at a distance of 7.5" from the primary component, which has a brightness of 1.5 magnitude. Due to the large difference in their brightness, we will need a telescope with an objective diameter of at least 15 cm to resolve them. \ No newline at end of file diff --git a/en/star/hr264.md b/en/star/hr264.md new file mode 100644 index 000000000..1f4562e96 --- /dev/null +++ b/en/star/hr264.md @@ -0,0 +1,9 @@ +--- +name: Cih (γ Cassiopeiae) +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 17:56:45.206811 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:45.206815 +--- +The white dwarf, with a star in the middle of the letter "W", is the brightest in this group. It is approximately 34,000 times more luminous than the Sun and located 550 light-years away. Using a larger amateur telescope, we will reveal a companion with a brightness of 11mag at a separation of 2.3". \ No newline at end of file diff --git a/en/star/hr2650.md b/en/star/hr2650.md new file mode 100644 index 000000000..a4e05f91d --- /dev/null +++ b/en/star/hr2650.md @@ -0,0 +1,9 @@ +--- +name: Mekbuda (ζ Gem) +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 15:02:12.777134 +updated_by: editor.cs +updated_date: 2023-11-05 15:02:12.777138 +--- +One of the brightest Cepheids in the sky: the main yellow star changes its brightness in the range of 3.6mag to 4.1mag with a period of 10.15 days. Suitable comparison stars are κ (3.57mag) and υ Gem (4.07mag). One companion is located at a separation of 96" and has a brightness of 8mag, the second one is observed 87" away and has a brightness of 11mag. However, they are only optically companions. Mekbuda pulsates from a distance of 1120 light years. \ No newline at end of file diff --git a/en/star/hr2671.md b/en/star/hr2671.md new file mode 100644 index 000000000..e35514c5d --- /dev/null +++ b/en/star/hr2671.md @@ -0,0 +1,9 @@ +--- +name: R Gem +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 17:15:03.675713 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:03.675717 +--- +Variable star of the Mira Ceti type, its brightness varies in the range of 6-14mag with a period of 370 days. It is located near the star δ Gem. \ No newline at end of file diff --git a/en/star/hr2736.md b/en/star/hr2736.md new file mode 100644 index 000000000..a1a20fe78 --- /dev/null +++ b/en/star/hr2736.md @@ -0,0 +1,9 @@ +--- +name: γ Vol +constellation: Vol +created_by: editor.cs +created_date: 2023-11-05 16:40:30.644869 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:30.644874 +--- +An attractive double star for a small telescope, with components of brightness 3.8mag and 5.7mag, located at a distance of 13.6". They have an orange and yellow color. \ No newline at end of file diff --git a/en/star/hr2742.md b/en/star/hr2742.md new file mode 100644 index 000000000..57e8e43a0 --- /dev/null +++ b/en/star/hr2742.md @@ -0,0 +1,9 @@ +--- +name: VZ Cam +constellation: Cam +created_by: editor.cs +created_date: 2023-11-05 17:15:07.923811 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:07.923815 +--- +A semi-regular variable star of type M, when observed through a telescope, appears noticeably red. It exhibits small, irregular changes in magnitude, ranging from 4.8mag to 5.2mag with an average period of about 24 days. Due to its proximity to the celestial pole, it can be observed throughout the year from more northern latitudes. \ No newline at end of file diff --git a/en/star/hr2748.md b/en/star/hr2748.md new file mode 100644 index 000000000..8abed0586 --- /dev/null +++ b/en/star/hr2748.md @@ -0,0 +1,9 @@ +--- +name: L2 Puppis +constellation: Pup +created_by: editor.cs +created_date: 2023-11-05 17:49:50.168784 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:50.168787 +--- +A clear long-period variable star belonging to the Mirid group, one of the brightest red variable stars, whose brightness varies between 2.6mag and 6.2mag in a period of 141 days. In its maximum, it is therefore very well visible even from illuminated areas, but in its minimum, it drops to the limit of visibility with the naked eye. \ No newline at end of file diff --git a/en/star/hr2777.md b/en/star/hr2777.md new file mode 100644 index 000000000..7c364c39a --- /dev/null +++ b/en/star/hr2777.md @@ -0,0 +1,9 @@ +--- +name: Wasat (δ Gem) +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 16:45:36.206303 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:36.206306 +--- +A binary star distinguishable by a small telescope. The primary star has a magnitude of 3.5 and the companion has a magnitude of 8.2, with an orbital period of approximately 1,200 years. In 1985, the companion was 6" away from the primary star, making it observable with a telescope with a 6 cm objective diameter. By the year 2000, their mutual separation had decreased to 5.8". Even so, it is not a problem for a 200 mm telescope, in which we can also see their yellow or light blue color. \ No newline at end of file diff --git a/en/star/hr2782.md b/en/star/hr2782.md new file mode 100644 index 000000000..a453a6173 --- /dev/null +++ b/en/star/hr2782.md @@ -0,0 +1,9 @@ +--- +name: τ CMa +constellation: CMa +created_by: editor.cs +created_date: 2023-11-05 17:16:56.294193 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:56.294196 +--- +A beautiful multiple star is observable even with a small telescope within the open star cluster NGC 2362. It is located in a magnificent environment filled with faint stars. The primary component is yellow with a magnitude of 4.4, while the companion is blue with a magnitude of 10.5. They are separated by 8.2". \ No newline at end of file diff --git a/en/star/hr2784.md b/en/star/hr2784.md new file mode 100644 index 000000000..93c49dbe5 --- /dev/null +++ b/en/star/hr2784.md @@ -0,0 +1,9 @@ +--- +name: 19 Lyn +constellation: Lyn +created_by: editor.cs +created_date: 2023-11-05 17:57:40.943351 +updated_by: editor.cs +updated_date: 2023-11-05 17:57:40.943355 +--- +This optical binary star can be easily distinguished even with a small telescope. Both stars, one with a brightness of 5.6 mag and the other with 6.5 mag, are separated by 14.8". The first one has a yellow-white color, while the second one has a light blue color. The light from the first star travels 680 light-years to reach us, while the light from the second star travels 690 light-years. In a larger telescope, two more optically associated companions can be observed. \ No newline at end of file diff --git a/en/star/hr280.md b/en/star/hr280.md new file mode 100644 index 000000000..21a068a09 --- /dev/null +++ b/en/star/hr280.md @@ -0,0 +1,9 @@ +--- +name: α Scl +constellation: Scl +created_by: editor.cs +created_date: 2023-11-05 16:45:23.215896 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:23.215900 +--- +The brightness of a constellation is often indicated by its brightest star, which has a magnitude of only 4.39. Its probable distance is 780 light-years. Just north of it lies the southern galactic pole. \ No newline at end of file diff --git a/en/star/hr2878.md b/en/star/hr2878.md new file mode 100644 index 000000000..bef3dfa91 --- /dev/null +++ b/en/star/hr2878.md @@ -0,0 +1,9 @@ +--- +name: σ Pup +constellation: Pup +created_by: editor.cs +created_date: 2023-11-05 17:14:17.839361 +updated_by: editor.cs +updated_date: 2023-11-05 17:14:17.839366 +--- +A nice double star, distinguishable already with a 5 cm telescope. The main orange component has a brightness of 3.3 mag and its yellow companion at a separation of 22.3" reaches only 9.4 mag. \ No newline at end of file diff --git a/en/star/hr2891.md b/en/star/hr2891.md new file mode 100644 index 000000000..f8cfc4925 --- /dev/null +++ b/en/star/hr2891.md @@ -0,0 +1,9 @@ +--- +name: Kastor (α Gem) +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 16:28:42.681333 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:42.681336 +--- +Although Pollux is slightly brighter, the star designated as Kastor (the 23rd brightest star in the sky) is represented by the Greek letter alpha. It has a magnitude of 1.5 and is located 51 light-years away from Earth. In addition, it is known as a multiple star system. The primary component has a magnitude of 1.9 and is overall 22 times more luminous than the Sun, while the companion reaches a magnitude of 2.9. They orbit each other around a common center of gravity every 445 years. The angular separation of the pair has been relatively small in recent years, reaching a minimum of 1.9" in 1970. Since then, it has gradually increased, allowing these blue components to be resolved even with a small telescope. In 1985, their separation was 2.6", and by 2017, it had increased to 6". \ No newline at end of file diff --git a/en/star/hr2990.md b/en/star/hr2990.md new file mode 100644 index 000000000..e9396d43a --- /dev/null +++ b/en/star/hr2990.md @@ -0,0 +1,9 @@ +--- +name: Pollux (β Gem) +constellation: Gem +created_by: editor.cs +created_date: 2023-11-05 15:43:48.605388 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:48.605391 +--- +With a brightness of 1.14 mag, it is the 17th brightest star in the sky. It surpasses the brightness of the Sun by a factor of 33, and its diameter is 9 times larger. Unlike Kastor, Pollux is orange-red and has a spectral class of K0. Its distinctive shade can be seen with the naked eye. It is located at a distance of 34 light years. \ No newline at end of file diff --git a/en/star/hr310.md b/en/star/hr310.md new file mode 100644 index 000000000..c81236c90 --- /dev/null +++ b/en/star/hr310.md @@ -0,0 +1,9 @@ +--- +name: ψ Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 17:51:40.726312 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:40.726316 +--- +Wide double star visible in a hand lens. It consists of two components with magnitudes of 5.5 and 5.8, separated by 30". Both have a light blue color and are located 230 light-years away. \ No newline at end of file diff --git a/en/star/hr3110.md b/en/star/hr3110.md new file mode 100644 index 000000000..1ce45c4a2 --- /dev/null +++ b/en/star/hr3110.md @@ -0,0 +1,9 @@ +--- +name: 14 CMi +constellation: CMi +created_by: editor.cs +created_date: 2023-11-05 16:40:42.478737 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:42.478740 +--- +Triple star system. The main star has a brightness of 5.4 mag. At a distance of 76", there is a star of magnitude 7, and at a separation of 112", there is a star with a brightness of 8 mag. We can already resolve them with a good eyepiece or a telescope with a 5 cm objective diameter. \ No newline at end of file diff --git a/en/star/hr3165.md b/en/star/hr3165.md new file mode 100644 index 000000000..2644842b4 --- /dev/null +++ b/en/star/hr3165.md @@ -0,0 +1,9 @@ +--- +name: Naos (ζ Puppis) +constellation: Pup +created_by: editor.cs +created_date: 2023-11-05 15:40:10.623901 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:10.623906 +--- +Because the Argo Navis was originally considered as one constellation, the method of labeling stars with Greek letters is the same for all its divided parts. Therefore, in the Stern, we will not find any alpha, beta, gamma, or delta Puppis, the brightest star is ζ Puppis, which reaches a magnitude of 2.3. \ No newline at end of file diff --git a/en/star/hr3188.md b/en/star/hr3188.md new file mode 100644 index 000000000..e7771b81e --- /dev/null +++ b/en/star/hr3188.md @@ -0,0 +1,9 @@ +--- +name: ζ Mon +constellation: Mon +created_by: editor.cs +created_date: 2023-11-05 16:47:04.633368 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:04.633371 +--- +Optical double star. The primary component has a brightness of 5mag, its companion has a brightness of 8.5mag. It is located at a separation of 66.4". Another companion can be found at a distance of 32". We need a telescope with a 7cm diameter objective. \ No newline at end of file diff --git a/en/star/hr3207.md b/en/star/hr3207.md new file mode 100644 index 000000000..b10b79e2d --- /dev/null +++ b/en/star/hr3207.md @@ -0,0 +1,9 @@ +--- +name: γ Velorum +constellation: Vel +created_by: editor.cs +created_date: 2023-11-05 17:49:27.800307 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:27.800311 +--- +A double star distinguishable in a telescope, with its primary component being the brightest known Wolf-Rayet star, very hot and unstable, astonishingly ejecting mass at a high velocity. Even in simple spectrographs, prominent emissions in the blue region of the spectrum can be seen, lines of highly ionized atoms shining in an extensive warm envelope illuminated by the star. γ Velorum is in an advanced stage of its evolution and shines approximately 3,800 times brighter than the Sun. But this will not be the case forever. After several million years, it could explode as a supernova. It is located 840 light-years away. \ No newline at end of file diff --git a/en/star/hr322.md b/en/star/hr322.md new file mode 100644 index 000000000..8c73105b4 --- /dev/null +++ b/en/star/hr322.md @@ -0,0 +1,9 @@ +--- +name: β Phe +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 15:59:36.598239 +updated_by: editor.cs +updated_date: 2023-11-05 15:59:36.598244 +--- +A close binary star with a separation of 1.4", whose individual components of 4 magnitude and 4.2 mm can be resolved by telescopes with an objective diameter of around 15 cm. The system is located 198 light years away. In the field of view at a distance of 58", we can still see another companion with a brightness of 11.5 magnitude. \ No newline at end of file diff --git a/en/star/hr3223.md b/en/star/hr3223.md new file mode 100644 index 000000000..9d6ad9c3a --- /dev/null +++ b/en/star/hr3223.md @@ -0,0 +1,9 @@ +--- +name: ε Vol +constellation: Vol +created_by: editor.cs +created_date: 2023-11-05 15:16:45.919511 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:45.919515 +--- +Double star composed of components with magnitudes 4 and 7, which can be resolved using a small telescope. Their separation is 6". \ No newline at end of file diff --git a/en/star/hr3248.md b/en/star/hr3248.md new file mode 100644 index 000000000..92aecf254 --- /dev/null +++ b/en/star/hr3248.md @@ -0,0 +1,9 @@ +--- +name: R Cancri +constellation: Cnc +created_by: editor.cs +created_date: 2023-11-05 16:43:18.627447 +updated_by: editor.cs +updated_date: 2023-11-05 16:43:18.627451 +--- +The variable star of Mira Ceti type with magnitude changes from 6.1 to 11.8 and a period of 362 days. \ No newline at end of file diff --git a/en/star/hr3301.md b/en/star/hr3301.md new file mode 100644 index 000000000..fc36945db --- /dev/null +++ b/en/star/hr3301.md @@ -0,0 +1,9 @@ +--- +name: κ Vol +constellation: Vol +created_by: editor.cs +created_date: 2023-11-05 17:55:30.751687 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:30.751691 +--- +The double star is easily distinguishable even in a telescope. The primary component with a brightness of 5.4 magnitude is located at a distance of 65 arcseconds from the companion with a brightness of 5.7 magnitude. At a separation of 37 arcseconds, there is another companion of 9th stellar magnitude. \ No newline at end of file diff --git a/en/star/hr3318.md b/en/star/hr3318.md new file mode 100644 index 000000000..f22ba6c48 --- /dev/null +++ b/en/star/hr3318.md @@ -0,0 +1,9 @@ +--- +name: α Cha +constellation: Cha +created_by: editor.cs +created_date: 2023-11-05 16:32:09.471825 +updated_by: editor.cs +updated_date: 2023-11-05 16:32:09.471828 +--- +The brightest star of the constellation. It has an apparent magnitude of only 4.08. This white dwarf of spectral class F5 is located 64 light-years away from us. \ No newline at end of file diff --git a/en/star/hr3340.md b/en/star/hr3340.md new file mode 100644 index 000000000..60a819ad4 --- /dev/null +++ b/en/star/hr3340.md @@ -0,0 +1,9 @@ +--- +name: θ Cha +constellation: Cha +created_by: editor.cs +created_date: 2023-11-05 15:15:37.580996 +updated_by: editor.cs +updated_date: 2023-11-05 15:15:37.580999 +--- +Optical binary star, whose components appear very close to each other in the sky from Earth, but are actually very far apart in space. The brighter component with a magnitude of 4.3 is located at a distance of 100 light years, while the fainter one is separated from us by up to 1,000 light years. \ No newline at end of file diff --git a/en/star/hr3347.md b/en/star/hr3347.md new file mode 100644 index 000000000..b8445244e --- /dev/null +++ b/en/star/hr3347.md @@ -0,0 +1,9 @@ +--- +name: β Vol +constellation: Vol +created_by: editor.cs +created_date: 2023-11-05 16:31:29.650849 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:29.650853 +--- +The brightest star of the constellation, a star with an apparent magnitude of 3.7. This orange giant is located at a distance of 108 light years. \ No newline at end of file diff --git a/en/star/hr338.md b/en/star/hr338.md new file mode 100644 index 000000000..0a2c28bfb --- /dev/null +++ b/en/star/hr338.md @@ -0,0 +1,9 @@ +--- +name: ζ Phe +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 17:15:55.352954 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:55.352957 +--- +Optical double star, whose components at a separation of 6.4" can be easily resolved even with a small telescope. The fainter one has a magnitude of 8mag. The brighter one changes its brightness every 40 hours, as it is an eclipsing variable star of the Algol type. It changes its brightness from 3.9mag to 4.4mag, which can be easily observed with the naked eye. \ No newline at end of file diff --git a/en/star/hr34.md b/en/star/hr34.md new file mode 100644 index 000000000..9e83005ad --- /dev/null +++ b/en/star/hr34.md @@ -0,0 +1,9 @@ +--- +name: κ1 Scl +constellation: Scl +created_by: editor.cs +created_date: 2023-11-05 16:41:40.499231 +updated_by: editor.cs +updated_date: 2023-11-05 16:41:40.499235 +--- +A binary star with bright components of 6.1 magnitude and 6.2 magnitude, which are, however, located very close to each other - 1.4". Both have a yellow color. \ No newline at end of file diff --git a/en/star/hr3433.md b/en/star/hr3433.md new file mode 100644 index 000000000..384c4ca6b --- /dev/null +++ b/en/star/hr3433.md @@ -0,0 +1,9 @@ +--- +name: ζ Pyx +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 16:48:51.219975 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:51.219979 +--- +The main component has a brightness of 5.5 mag and its companion has a brightness of 10 mag at a distance of 52.3". We can distinguish them with a telescope with an 8 cm diameter objective. \ No newline at end of file diff --git a/en/star/hr3438.md b/en/star/hr3438.md new file mode 100644 index 000000000..4355c8e46 --- /dev/null +++ b/en/star/hr3438.md @@ -0,0 +1,9 @@ +--- +name: β Pyx +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 16:28:59.727870 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:59.727874 +--- +The yellow supergiant of spectral class G5. A companion with a brightness of 12.5mag is located at an angular distance of 12.6". \ No newline at end of file diff --git a/en/star/hr3468.md b/en/star/hr3468.md new file mode 100644 index 000000000..00c0549b3 --- /dev/null +++ b/en/star/hr3468.md @@ -0,0 +1,9 @@ +--- +name: α Pyx +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 17:54:07.961826 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:07.961830 +--- +The brightest star in the constellation has an apparent magnitude of 3.7. It is located 470 light-years away. \ No newline at end of file diff --git a/en/star/hr3475.md b/en/star/hr3475.md new file mode 100644 index 000000000..b978fdbe5 --- /dev/null +++ b/en/star/hr3475.md @@ -0,0 +1,9 @@ +--- +name: ι2 Cancri +constellation: Cnc +created_by: editor.cs +created_date: 2023-11-05 15:45:59.586631 +updated_by: editor.cs +updated_date: 2023-11-05 15:45:59.586634 +--- +A triple star system that cannot be resolved even with a 30 cm telescope. Under good observing conditions, it is visible only as an elongated star, with a hint of a primary yellow and a secondary blue component. \ No newline at end of file diff --git a/en/star/hr3482.md b/en/star/hr3482.md new file mode 100644 index 000000000..cdedc21b7 --- /dev/null +++ b/en/star/hr3482.md @@ -0,0 +1,9 @@ +--- +name: ε Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 15:46:03.714138 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:03.714142 +--- +The main component with a brightness of 3.8mag has a companion with a brightness of 6.9mag at a separation of 2.8". To resolve this binary star, we need a telescope with an objective diameter of at least 8 cm. The components orbit each other every 870 years and are located at a distance of 129 light-years. \ No newline at end of file diff --git a/en/star/hr3485.md b/en/star/hr3485.md new file mode 100644 index 000000000..28d49b6c4 --- /dev/null +++ b/en/star/hr3485.md @@ -0,0 +1,9 @@ +--- +name: δ Vel +constellation: Vel +created_by: editor.cs +created_date: 2023-11-05 16:36:01.598525 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:01.598531 +--- +The brightest star of the constellation with an apparent magnitude of 2mag. Along with the stars κ Vel and ε and ι Car of the Carina constellation, they form the so-called False Cross, which beginner observers often mistake for the real Southern Cross. However, unlike the Southern Cross, it is slightly larger, more symmetrical, and less bright, and its arm does not point towards the southern celestial pole. \ No newline at end of file diff --git a/en/star/hr3541.md b/en/star/hr3541.md new file mode 100644 index 000000000..5186b7188 --- /dev/null +++ b/en/star/hr3541.md @@ -0,0 +1,9 @@ +--- +name: X Cancri +constellation: Cnc +created_by: editor.cs +created_date: 2023-11-05 17:48:54.540715 +updated_by: editor.cs +updated_date: 2023-11-05 17:48:54.540719 +--- +The variable star with a distinct red hue changes its magnitude from 5.6 to 7.5 mag approximately every 195 days, suitable for observation in binoculars. It is located near the star δ Cancri. \ No newline at end of file diff --git a/en/star/hr3572.md b/en/star/hr3572.md new file mode 100644 index 000000000..75ec18413 --- /dev/null +++ b/en/star/hr3572.md @@ -0,0 +1,9 @@ +--- +name: Acubens (α Cancri) +constellation: Cnc +created_by: editor.cs +created_date: 2023-11-05 15:01:18.575734 +updated_by: editor.cs +updated_date: 2023-11-05 15:01:18.575738 +--- +Double star distinguishable only with a larger telescope. The companion is located 11.3" away from the primary component (4.25 mag), but it is about 1,000 times fainter and has a brightness of only 11.8 mag in the sky. The system is located at a distance of 164 light-years. \ No newline at end of file diff --git a/en/star/hr361.md b/en/star/hr361.md new file mode 100644 index 000000000..80349f85c --- /dev/null +++ b/en/star/hr361.md @@ -0,0 +1,9 @@ +--- +name: ζ Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 18:12:14.229088 +updated_by: editor.cs +updated_date: 2023-11-05 18:12:14.229091 +--- +A nice optical double star with components of 5.6mag and 6.5mag, separated by 23.6". However, in reality, one is located at a distance of 150 light years and the other at 195 light years. The primary component appears white, while the companion has a yellow color. During a good night, it can be easily observed with binoculars, and a small telescope will also work without any problems. \ No newline at end of file diff --git a/en/star/hr3628.md b/en/star/hr3628.md new file mode 100644 index 000000000..1d973dcad --- /dev/null +++ b/en/star/hr3628.md @@ -0,0 +1,9 @@ +--- +name: κ Pyx +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 17:44:02.035918 +updated_by: editor.cs +updated_date: 2023-11-05 17:44:02.035923 +--- +A binary star, with a companion of 10th magnitude, is located at a separation of 2.1 arcseconds from the component with a brightness of 4.8 magnitude. We will need a telescope with an objective diameter of at least 150 mm. \ No newline at end of file diff --git a/en/star/hr3644.md b/en/star/hr3644.md new file mode 100644 index 000000000..cc8256d27 --- /dev/null +++ b/en/star/hr3644.md @@ -0,0 +1,9 @@ +--- +name: ε Pyx +constellation: Pyx +created_by: editor.cs +created_date: 2023-11-05 15:16:04.708262 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:04.708266 +--- +A remarkable multiple star. The primary component has a brightness of 5.6 mag and at a separation of 17.8", it can be observed with a telescope with a 60 mm objective diameter as a guide star with a brightness of 9.2 mag. With a larger telescope, we can also observe a star of magnitude 10 at a separation of 0.3". \ No newline at end of file diff --git a/en/star/hr3690.md b/en/star/hr3690.md new file mode 100644 index 000000000..f53ed2f34 --- /dev/null +++ b/en/star/hr3690.md @@ -0,0 +1,9 @@ +--- +name: 38 Lyn +constellation: Lyn +created_by: editor.cs +created_date: 2023-11-05 16:46:04.400639 +updated_by: editor.cs +updated_date: 2023-11-05 16:46:04.400643 +--- +The binary star is located approximately on the border with the neighboring constellation of Leo Minor. The main white component has a brightness of 3.9 mag, the red companion has a brightness of 6.6 mag. They are mutually separated by 2.7" and their distance from Earth is about 117 light years. The main star has about 32 times the luminosity of the Sun. At a distance of about 88" from this star, we can see another companion with a stellar magnitude of 11 mag, which, however, is only coincidentally projected into this area. It is advisable to use at least 100x magnification. \ No newline at end of file diff --git a/en/star/hr3748.md b/en/star/hr3748.md new file mode 100644 index 000000000..2f165e663 --- /dev/null +++ b/en/star/hr3748.md @@ -0,0 +1,9 @@ +--- +name: Alfard (α Hya) +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 17:56:59.997324 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:59.997327 +--- +The brightest star of the constellation, located on the line connecting the stars Castor - Pollux of Gemini. Its remarkable orange color can certainly be noticed with the naked eye, and it belongs to the spectral class K3. This star has a magnitude of 2 and is located in an area relatively poor in stars. That is why its translated name from Arabic means "Lonely Star". However, Tycho de Brahe called it Cor Hydraul - "Heart of the Hydra". It is located at a distance of 177 light years and is 780 times more luminous than the Sun. \ No newline at end of file diff --git a/en/star/hr377.md b/en/star/hr377.md new file mode 100644 index 000000000..573fc3c1c --- /dev/null +++ b/en/star/hr377.md @@ -0,0 +1,9 @@ +--- +name: κ Tuc +constellation: Tuc +created_by: editor.cs +created_date: 2023-11-05 17:54:10.524197 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:10.524200 +--- +A binary star composed of stars with magnitudes 5 and 8, which can be resolved with a small telescope. \ No newline at end of file diff --git a/en/star/hr3787.md b/en/star/hr3787.md new file mode 100644 index 000000000..eecc0b5c3 --- /dev/null +++ b/en/star/hr3787.md @@ -0,0 +1,9 @@ +--- +name: τ1 Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 18:12:10.262037 +updated_by: editor.cs +updated_date: 2023-11-05 18:12:10.262045 +--- +The components with magnitudes of 4.8 and 8 lie at a separation of 65". It is an optical double star, which can be resolved even with a simple telescope. \ No newline at end of file diff --git a/en/star/hr3789.md b/en/star/hr3789.md new file mode 100644 index 000000000..110b109d2 --- /dev/null +++ b/en/star/hr3789.md @@ -0,0 +1,9 @@ +--- +name: ζ Antliae +constellation: Ant +created_by: editor.cs +created_date: 2023-11-05 16:32:48.264465 +updated_by: editor.cs +updated_date: 2023-11-05 16:32:48.264470 +--- +A multiple star that is resolved into two wide optical components of sixth magnitude by a trihedron. With a small telescope, we additionally find that the brighter one of them is itself a binary star - a yellow companion of magnitude 7.1 is located eight arc seconds away from it. \ No newline at end of file diff --git a/en/star/hr3798.md b/en/star/hr3798.md new file mode 100644 index 000000000..66fdbc0f0 --- /dev/null +++ b/en/star/hr3798.md @@ -0,0 +1,9 @@ +--- +name: S Antliae +constellation: Ant +created_by: editor.cs +created_date: 2023-11-05 16:25:00.460223 +updated_by: editor.cs +updated_date: 2023-11-05 16:25:00.460228 +--- +Discovered in 1888, it is an eclipsing variable star with a brightness change of 0.5mag over exactly 7 hours and 47 minutes. At the time of its discovery, it was known as the variable star with the shortest period of brightness changes. It is included in the group of stars under the designation of W URSA Majoris type, a system where two dwarf stars orbit each other in close contact, constantly changing their position from our perspective. \ No newline at end of file diff --git a/en/star/hr3816.md b/en/star/hr3816.md new file mode 100644 index 000000000..005a85dc1 --- /dev/null +++ b/en/star/hr3816.md @@ -0,0 +1,9 @@ +--- +name: R Carinae +constellation: Car +created_by: editor.cs +created_date: 2023-11-05 17:48:50.748105 +updated_by: editor.cs +updated_date: 2023-11-05 17:48:50.748110 +--- +The variable star of Mira Ceti type with a magnitude range from 3.9 to 10.5 and a period of 309 days. \ No newline at end of file diff --git a/en/star/hr3882.md b/en/star/hr3882.md new file mode 100644 index 000000000..c57c45a52 --- /dev/null +++ b/en/star/hr3882.md @@ -0,0 +1,9 @@ +--- +name: R Leonis +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 16:49:40.396011 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:40.396015 +--- +The variable star of Mira Ceti type is located in the western part of the constellation, near the star Regulus, at a distance of 372 light years. This red giant changes its brightness from 4.4 mag to 11.3 mag with a long period of 312.43 days. It is therefore one of the brightest long-period variable stars. At the time of maximum brightness, we can notice its distinct dark red shade, which nicely contrasts with the white star 19 Leonis, located 8' to the south. \ No newline at end of file diff --git a/en/star/hr3981.md b/en/star/hr3981.md new file mode 100644 index 000000000..10e4603ec --- /dev/null +++ b/en/star/hr3981.md @@ -0,0 +1,9 @@ +--- +name: α Sex +constellation: Sex +created_by: editor.cs +created_date: 2023-11-05 16:28:24.957251 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:24.957254 +--- +The brightest star of the constellation has an apparent magnitude of 4.5. It is located almost exactly on the celestial equator. It is located 270 light-years away. \ No newline at end of file diff --git a/en/star/hr3982.md b/en/star/hr3982.md new file mode 100644 index 000000000..2b3925957 --- /dev/null +++ b/en/star/hr3982.md @@ -0,0 +1,9 @@ +--- +name: Regulus (α Leonis) +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 16:37:17.996690 +updated_by: editor.cs +updated_date: 2023-11-05 16:37:17.996693 +--- +The brightest star of the constellation. It will lead us to it with a 9-fold extended line of the front wheels of the Big Dipper to the south. Together with the stars Arcturus from the Shepherd and Spica from the Virgin, they form a kind of spring triangle. The name comes from Latin and means "little king", in ancient Babylon it even represented the star of the ruler. Sometimes we can also come across the name Cor Leonis - "heart of the lion". Regulus is also one of the four guardians of the sky, or even royal stars - they were the stars that marked the point of the summer solstice (Regulus), the spring point (Aldebaran), the winter solstice (Fomalhaut), and the autumn point (Antares) in the Persian Empire. They divided the Sun's path - the ecliptic, and thus the year into four seasons. As one of the few bright stars, it lies near the ecliptic, exactly 1.5 degrees. Therefore, there is often an occultation by the Moon and sometimes by a planet. \ No newline at end of file diff --git a/en/star/hr3989.md b/en/star/hr3989.md new file mode 100644 index 000000000..834b73a86 --- /dev/null +++ b/en/star/hr3989.md @@ -0,0 +1,9 @@ +--- +name: 17 a 18 Sex +constellation: Sex +created_by: editor.cs +created_date: 2023-11-05 17:00:48.647328 +updated_by: editor.cs +updated_date: 2023-11-05 17:00:48.647333 +--- +A wide pair of unrelated stars that can be identified with the naked eye if the observer has good vision. They are easily separated with a telescope. They have magnitudes of 5.9 and 5.6. The components are separated by 530 and 470 light-years. \ No newline at end of file diff --git a/en/star/hr4031.md b/en/star/hr4031.md new file mode 100644 index 000000000..15703ae8d --- /dev/null +++ b/en/star/hr4031.md @@ -0,0 +1,9 @@ +--- +name: ζ Leonis +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 16:30:27.249771 +updated_by: editor.cs +updated_date: 2023-11-05 16:30:27.249775 +--- +The wide triple star, composed of stars with no mutual relationship, is ζ Leonis with a brightness of 3.4 mag. The finder shows the star 35 Leonis to the north of it and also the star 39 Leonis to the south. Both stars have a magnitude of 6 mag. \ No newline at end of file diff --git a/en/star/hr4057.md b/en/star/hr4057.md new file mode 100644 index 000000000..348b7c913 --- /dev/null +++ b/en/star/hr4057.md @@ -0,0 +1,9 @@ +--- +name: Algieba (γ Leonis) +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 16:27:52.351151 +updated_by: editor.cs +updated_date: 2023-11-05 16:27:52.351155 +--- +"The Lion's Forehead", a corrupted name of the Arabic word Al Jabha. In reality, it is a beautiful double star located 8 degrees SSW from the star Regulus, with yellow-orange components of 2.2 magnitude (about 90 times the brightness of the Sun) and 3.5 magnitude (about 30 times the brightness of the Sun) at a separation of 4.4", with a noticeable contrast that can be perceived as green. Their mutual orbital period is estimated to be 619 years. Even in 1782, when William Herschel first discovered this attractive double star, the angular separation of its components was less than 2". Since then, the separation has significantly increased and by the end of the 20th century, it reached almost 4.4". \ No newline at end of file diff --git a/en/star/hr4100.md b/en/star/hr4100.md new file mode 100644 index 000000000..d5673c749 --- /dev/null +++ b/en/star/hr4100.md @@ -0,0 +1,9 @@ +--- +name: β LMi +constellation: LMi +created_by: editor.cs +created_date: 2023-11-05 17:31:03.440765 +updated_by: editor.cs +updated_date: 2023-11-05 17:31:03.440770 +--- +The only star of the constellation that is assigned a Greek letter. This close binary star, which appears as a bright point of 4.2 magnitude to the naked eye, reveals its companion of 6.1 magnitude only in a large telescope and under good observing conditions. It is located at an angular distance of just a few tenths of a second. The orbital period of the components is 37 years and the distance is 145 light-years. \ No newline at end of file diff --git a/en/star/hr4104.md b/en/star/hr4104.md new file mode 100644 index 000000000..d896c4a9a --- /dev/null +++ b/en/star/hr4104.md @@ -0,0 +1,9 @@ +--- +name: α Antliae +constellation: Ant +created_by: editor.cs +created_date: 2023-11-05 17:17:21.312798 +updated_by: editor.cs +updated_date: 2023-11-05 17:17:21.312802 +--- +The brightest star of the constellation has a magnitude of 4.25, in many constellations it would remain unnoticed. In a telescope, we can see its orange to red hue. Its spectral class is K4, so it is a cooler star than our Sun. Its brightness may slightly vary and it is located 370 light-years away. \ No newline at end of file diff --git a/en/star/hr4163.md b/en/star/hr4163.md new file mode 100644 index 000000000..170cce9a9 --- /dev/null +++ b/en/star/hr4163.md @@ -0,0 +1,9 @@ +--- +name: U Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 14:50:18.630507 +updated_by: editor.cs +updated_date: 2023-11-05 14:50:18.630513 +--- +One of the brightest and most unusual carbon stars, whose red color can be seen even in the smallest telescope. This is due to the abundance of carbon molecules in its atmosphere, which absorb blue light. U Hya is observed 4 degrees northwest of the star ν Hydra and belongs to the irregular variable stars, whose magnitude fluctuates regularly from 4.7mag to 6.2mag in a period of about 450 days. It is located approximately 680 light-years away. \ No newline at end of file diff --git a/en/star/hr4210.md b/en/star/hr4210.md new file mode 100644 index 000000000..b58b03845 --- /dev/null +++ b/en/star/hr4210.md @@ -0,0 +1,9 @@ +--- +name: η Carinae +constellation: Car +created_by: editor.cs +created_date: 2023-11-05 16:11:18.738687 +updated_by: editor.cs +updated_date: 2023-11-05 16:11:18.738691 +--- +An unusual variable star, massive and unstable, which may explode as a supernova in the future. In 1677, Edmund Halley observed that this star brightened to 4th magnitude. By 1730, it reached 2nd magnitude, in 1827 it brightened to 1st magnitude, and in April 1843, it temporarily became the second brightest star in the sky with a brightness of -0.8 magnitude! In the following years, its brightness decreased, and since 1868 it has sometimes been invisible without a telescope, as its brightness ranged around 6th stellar magnitude. However, in the infrared region, it remains the brightest source in the sky. \ No newline at end of file diff --git a/en/star/hr4216.md b/en/star/hr4216.md new file mode 100644 index 000000000..3f513596f --- /dev/null +++ b/en/star/hr4216.md @@ -0,0 +1,9 @@ +--- +name: μ Vel +constellation: Vel +created_by: editor.cs +created_date: 2023-11-05 16:41:10.217186 +updated_by: editor.cs +updated_date: 2023-11-05 16:41:10.217189 +--- +A physical binary star, whose components orbit each other every 116 years. Their brightness is 2.7 mag and 6.4 mag, with their separation currently being about 2.3". \ No newline at end of file diff --git a/en/star/hr423.md b/en/star/hr423.md new file mode 100644 index 000000000..f2fd26684 --- /dev/null +++ b/en/star/hr423.md @@ -0,0 +1,9 @@ +--- +name: R Scl +constellation: Scl +created_by: editor.cs +created_date: 2023-11-05 17:15:01.293867 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:01.293872 +--- +Variable red giant, whose brightness varies in an approximately one-year cycle ranging from 6 to 8 mag. \ No newline at end of file diff --git a/en/star/hr4234.md b/en/star/hr4234.md new file mode 100644 index 000000000..9f18dc638 --- /dev/null +++ b/en/star/hr4234.md @@ -0,0 +1,9 @@ +--- +name: δ Cha +constellation: Cha +created_by: editor.cs +created_date: 2023-11-05 17:54:27.949631 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:27.949635 +--- +A wide double star, whose components have magnitudes of 4.4 and 5.5, are separated by 7 arc minutes, so they can be resolved with the naked eye. In a telescope, we can observe their distinct white and orange hues. It is an optical double star: the brighter component is located at a distance of 364 light-years, while the fainter one is 10 light-years closer. However, the brighter component is actually a very close physical double star, which can only be resolved with a large telescope. \ No newline at end of file diff --git a/en/star/hr424.md b/en/star/hr424.md new file mode 100644 index 000000000..f79396b94 --- /dev/null +++ b/en/star/hr424.md @@ -0,0 +1,9 @@ +--- +name: Polaris (α UMi) +constellation: UMi +created_by: editor.cs +created_date: 2023-11-05 17:30:01.832562 +updated_by: skybber +updated_date: 2023-11-05 18:18:56.667329 +--- +Once known as the "leading star in the sky," it has another name - the North Star. In seas, deserts, and wastelands, it was the only indicator of the north in ancient times, before the invention of the compass. We can easily find it by drawing a line connecting the stars Merak and Dubhe, which form the back wheels of the Big Dipper, and extending it four times in the direction of the line. This will lead us to Polaris, which is located at the end of the handle of the Little Dipper. \ No newline at end of file diff --git a/en/star/hr4259.md b/en/star/hr4259.md new file mode 100644 index 000000000..dd9669411 --- /dev/null +++ b/en/star/hr4259.md @@ -0,0 +1,9 @@ +--- +name: 54 Leonis +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 15:44:38.595596 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:38.595599 +--- +A binary star located on the border of the constellation Leo Minor. These two partners have magnitudes of 4.5 and 6.3. The stars are separated by 6.5", so they should already be distinguishable with a telescope with an objective diameter of at least 5 cm. The system is located 330 light-years away from Earth. In 10-15 cm telescopes and 100x magnification, it appears as an unevenly bright, colorful binary star. The primary component appears yellow-white, while the companion is bluish to greenish. \ No newline at end of file diff --git a/en/star/hr4287.md b/en/star/hr4287.md new file mode 100644 index 000000000..62aa500be --- /dev/null +++ b/en/star/hr4287.md @@ -0,0 +1,9 @@ +--- +name: Alkes (α Crt) +constellation: Crt +created_by: editor.cs +created_date: 2023-11-05 16:35:47.343577 +updated_by: editor.cs +updated_date: 2023-11-05 16:35:47.343581 +--- +The Arabic name of the main star means "flat dish". Its brightness is only 4.2 magnitude. It is a yellow giant that radiates 66 times more than our Sun. It is located 141 light-years away from us. \ No newline at end of file diff --git a/en/star/hr4375.md b/en/star/hr4375.md new file mode 100644 index 000000000..ee9cb5527 --- /dev/null +++ b/en/star/hr4375.md @@ -0,0 +1,9 @@ +--- +name: ξ UMa +constellation: UMa +created_by: editor.cs +created_date: 2023-11-05 16:39:32.431807 +updated_by: editor.cs +updated_date: 2023-11-05 16:39:32.431810 +--- +The first binary star, for which the orbital path of its components was calculated, took place 60 years ago. It was achieved in 1828 by the French astronomer Felix Savary. It consists of golden components with a brightness of 4.3 mag and 4.8 mag, separated by 3 billion kilometers. Around 1970, they had a mutual separation of 3", and could easily be distinguished even with small telescopes. Then their mutual separation decreased, reaching its minimum in 1992 - 0.8". Today, this value is around 2", so a telescope with an 8 cm objective diameter is sufficient for their resolution. \ No newline at end of file diff --git a/en/star/hr4382.md b/en/star/hr4382.md new file mode 100644 index 000000000..92483efa1 --- /dev/null +++ b/en/star/hr4382.md @@ -0,0 +1,9 @@ +--- +name: δ Crt +constellation: Crt +created_by: editor.cs +created_date: 2023-11-05 16:39:55.064184 +updated_by: editor.cs +updated_date: 2023-11-05 16:39:55.064187 +--- +The brightest star in the constellation has an apparent magnitude of 3.82. It is located approximately 163 light-years away from Earth and its luminosity is 171 times greater than that of our Sun. \ No newline at end of file diff --git a/en/star/hr4399.md b/en/star/hr4399.md new file mode 100644 index 000000000..2219641ae --- /dev/null +++ b/en/star/hr4399.md @@ -0,0 +1,9 @@ +--- +name: ι Leonis +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 18:08:21.984348 +updated_by: editor.cs +updated_date: 2023-11-05 18:08:21.984352 +--- +remarkable binary star. Two components with magnitudes of 4.1 and 7.0 orbit each other approximately every 180 years. In 1985, they had a separation of 1.3", but they are starting to move away from each other and by the year 2000, they had already reached a separation of 1.7", making the binary star distinguishable in at least a 10 cm telescope. \ No newline at end of file diff --git a/en/star/hr4405.md b/en/star/hr4405.md new file mode 100644 index 000000000..5f681580d --- /dev/null +++ b/en/star/hr4405.md @@ -0,0 +1,9 @@ +--- +name: γ Crt +constellation: Crt +created_by: editor.cs +created_date: 2023-11-05 17:48:59.712168 +updated_by: editor.cs +updated_date: 2023-11-05 17:48:59.712172 +--- +The main component has a magnitude of 4.1 and is separated by 5.2" from a companion of magnitude 9.6, which can be observed with a telescope with an objective diameter of about 10 cm. The brighter component is white, while the companion has a blue color. Their light is traveling towards us for 85 years. \ No newline at end of file diff --git a/en/star/hr4418.md b/en/star/hr4418.md new file mode 100644 index 000000000..15d64dafb --- /dev/null +++ b/en/star/hr4418.md @@ -0,0 +1,9 @@ +--- +name: τ Leonis +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 15:02:27.671008 +updated_by: editor.cs +updated_date: 2023-11-05 15:02:27.671011 +--- +Double star, easily distinguishable even with a small telescope. The primary star has a magnitude of 5.4 and its companion has a magnitude of 7.0. The angular separation between the two components is 90". \ No newline at end of file diff --git a/en/star/hr4534.md b/en/star/hr4534.md new file mode 100644 index 000000000..132b421c4 --- /dev/null +++ b/en/star/hr4534.md @@ -0,0 +1,9 @@ +--- +name: Denebola (β Leonis) +constellation: Leo +created_by: editor.cs +created_date: 2023-11-05 16:24:41.532033 +updated_by: editor.cs +updated_date: 2023-11-05 16:24:41.532036 +--- +The brightness of the star is 2.2 magnitude and its distance from Earth is 36 light years. It is 15 times more luminous than the Sun. At a distance of almost 19 arc minutes, we can find a yellowish star with a brightness of 6 magnitude, which can even be seen with a theater binoculars. \ No newline at end of file diff --git a/en/star/hr462.md b/en/star/hr462.md new file mode 100644 index 000000000..13c8a3af1 --- /dev/null +++ b/en/star/hr462.md @@ -0,0 +1,9 @@ +--- +name: τ Scl +constellation: Scl +created_by: editor.cs +created_date: 2023-11-05 16:39:48.584882 +updated_by: editor.cs +updated_date: 2023-11-05 16:39:48.584886 +--- +A close pair (2.2") of bright yellow stars with magnitudes 6 and 7.1. \ No newline at end of file diff --git a/en/star/hr472.md b/en/star/hr472.md new file mode 100644 index 000000000..ea06f3253 --- /dev/null +++ b/en/star/hr472.md @@ -0,0 +1,9 @@ +--- +name: Achernar (α Eri) +constellation: Eri +created_by: editor.cs +created_date: 2023-11-05 15:45:37.190323 +updated_by: editor.cs +updated_date: 2023-11-05 15:45:37.190328 +--- +The brightest star of the constellation and the ninth brightest star in the entire sky. It does not rise above the horizon in our location, and it begins to appear above the horizon at a height of three degrees from the regions of Texas, Morocco, and Egypt. This pale blue star with a surface temperature of 15,000 ˚C has a magnitude of 0.5 on the sky and is located 139 light-years away from us. Its absolute luminosity is 3150 times greater than that of the Sun. Nearby, there is a wide double star p Eridani, whose components with a brightness of 6 mag can be distinguished with a small telescope. \ No newline at end of file diff --git a/en/star/hr4730.md b/en/star/hr4730.md new file mode 100644 index 000000000..16e8f48b8 --- /dev/null +++ b/en/star/hr4730.md @@ -0,0 +1,9 @@ +--- +name: Acrux (α Cru) +constellation: Cru +created_by: editor.cs +created_date: 2023-11-05 17:55:16.323300 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:16.323305 +--- +The brightest star of the constellation has a magnitude of 1.1 and is the 13th brightest star in the sky. In a telescope, we can distinguish it as two sparkling blue-white components separated by 4.4". They have magnitudes of 0.8 and 2.1, and we can separate them with a 60 mm telescope. The system is located at a distance of 370 light-years. We can find a third unrelated component with a magnitude of 5 in a refractor 90" away. \ No newline at end of file diff --git a/en/star/hr4757.md b/en/star/hr4757.md new file mode 100644 index 000000000..46390ecae --- /dev/null +++ b/en/star/hr4757.md @@ -0,0 +1,9 @@ +--- +name: Algorab (δ Crv) +constellation: Crv +created_by: editor.cs +created_date: 2023-11-05 18:08:00.814591 +updated_by: editor.cs +updated_date: 2023-11-05 18:08:00.814595 +--- +With a telescope with an objective diameter of at least 8 cm, we will see at a distance of 24.2" from the bright white component of third magnitude a faint pale blue companion of 9th stellar magnitude. This system is located 88 light years away from us. \ No newline at end of file diff --git a/en/star/hr4763.md b/en/star/hr4763.md new file mode 100644 index 000000000..ff50b63ac --- /dev/null +++ b/en/star/hr4763.md @@ -0,0 +1,9 @@ +--- +name: Gacrux (γ Cru) +constellation: Cru +created_by: editor.cs +created_date: 2023-11-05 16:38:06.143251 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:06.143254 +--- +Red giant (1.6 mag), which nicely contrasts with three other hot blue-white stars of the cross. In fact, it is an optical double star, with a companion of magnitude 6.5 mag found in a distance of 2'. The red giant is located at a distance of 88 light years from us, while the companion is three times further away. \ No newline at end of file diff --git a/en/star/hr4792.md b/en/star/hr4792.md new file mode 100644 index 000000000..511b72962 --- /dev/null +++ b/en/star/hr4792.md @@ -0,0 +1,9 @@ +--- +name: 24 Com +constellation: Com +created_by: editor.cs +created_date: 2023-11-05 15:41:59.606296 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:59.606299 +--- +Double star, components of 5.2 magnitude and 6.7 magnitude with a separation of 20.3". In at least a 10 cm telescope, a nice color contrast between the main yellow-orange and the fainter blue stars, similar to Albireo in Cygnus. Otherwise, they can be distinguished even with a better binocular. \ No newline at end of file diff --git a/en/star/hr4798.md b/en/star/hr4798.md new file mode 100644 index 000000000..e780e8c49 --- /dev/null +++ b/en/star/hr4798.md @@ -0,0 +1,9 @@ +--- +name: α Mus +constellation: Mus +created_by: editor.cs +created_date: 2023-11-05 17:55:44.345569 +updated_by: editor.cs +updated_date: 2023-11-05 17:55:44.345572 +--- +The brightest star of the constellation, which reaches a magnitude of 2.94. At a distance of 29.6", it has a very faint companion with a magnitude of 12.8. It is located 306 light-years away from us. \ No newline at end of file diff --git a/en/star/hr4808.md b/en/star/hr4808.md new file mode 100644 index 000000000..d938e59fc --- /dev/null +++ b/en/star/hr4808.md @@ -0,0 +1,9 @@ +--- +name: R Virginis +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 17:45:53.277280 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:53.277283 +--- +The variable star of Mira Ceti type, with a magnitude change from 6.0 to 12.1 over 146 days. It is assumed to be a red star of class M. \ No newline at end of file diff --git a/en/star/hr4825.md b/en/star/hr4825.md new file mode 100644 index 000000000..cb2580b0a --- /dev/null +++ b/en/star/hr4825.md @@ -0,0 +1,9 @@ +--- +name: Porrima (γ Virginis) +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 16:30:55.633696 +updated_by: editor.cs +updated_date: 2023-11-05 16:30:55.633700 +--- +One of the most beautiful double stars in the sky, both yellow-white components have almost the same brightness of 3.5 magnitude and can be observed with a 6 cm telescope at a separation of 3". Their orbital period around the common center of mass is 171.85 years. The largest separation was reached in 1920 - 6.2", so they could be distinguished even with a 5 cm telescope. Meanwhile, their mutual distance is rapidly decreasing. In 1985, the value reached 3.5", in 2000 only 1.8". Therefore, currently we need at least a 200 mm telescope to distinguish the two point-like stars under good seeing conditions. In 2007, the separation will be even smaller, only 0.3", and therefore we will need a significantly larger telescope to resolve them. The system is located 32 light-years away from us. Five arc degrees to the north lies the brightest quasar - thirteenth magnitude, labeled 3 C 273, located approximately 3 billion light-years away. \ No newline at end of file diff --git a/en/star/hr4844.md b/en/star/hr4844.md new file mode 100644 index 000000000..4abc94f7b --- /dev/null +++ b/en/star/hr4844.md @@ -0,0 +1,9 @@ +--- +name: β Mus +constellation: Mus +created_by: editor.cs +created_date: 2023-11-05 15:39:41.018262 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:41.018266 +--- +The elegant double star is composed of components of 4th magnitude orbiting around a common center of gravity once every 383 years. The current separation of the components is 1.6 arcseconds, which is a good test for a 100 mm telescope. The system is located 520 light-years away from us. \ No newline at end of file diff --git a/en/star/hr4846.md b/en/star/hr4846.md new file mode 100644 index 000000000..6d6b226d7 --- /dev/null +++ b/en/star/hr4846.md @@ -0,0 +1,9 @@ +--- +name: Y CVn (E-B 364) +constellation: CVn +created_by: editor.cs +created_date: 2023-11-05 16:34:09.528967 +updated_by: editor.cs +updated_date: 2023-11-05 16:34:09.528971 +--- +"The Superba," that's how Italian astronomer Angelo Secchi named this significantly red star in the 19th century. It is a variable star that changes its brightness from 4.8mag to 6.4mag in a period of 157 days. The striking red hue can be easily seen in 50-60 mm telescopes. The unusual, dark red color of this and similar stars is a result of the presence of carbon molecules (which are abundantly present in the atmosphere) absorbing the blue light of the star. \ No newline at end of file diff --git a/en/star/hr4853.md b/en/star/hr4853.md new file mode 100644 index 000000000..dfd2cf371 --- /dev/null +++ b/en/star/hr4853.md @@ -0,0 +1,9 @@ +--- +name: β Cru +constellation: Cru +created_by: editor.cs +created_date: 2023-11-05 15:16:40.421912 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:40.421915 +--- +The pale blue star is located 350 light-years away. With its brightness of 1.3 magnitude, it ranks among the twenty brightest stars in the sky. Its size changes five times a day due to pulsation, but its magnitude changes by less than a tenth, which is not enough for us to perceive with the naked eye. \ No newline at end of file diff --git a/en/star/hr4898.md b/en/star/hr4898.md new file mode 100644 index 000000000..5a91aa1cf --- /dev/null +++ b/en/star/hr4898.md @@ -0,0 +1,9 @@ +--- +name: μ Cru +constellation: Cru +created_by: editor.cs +created_date: 2023-11-05 16:38:33.797616 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:33.797620 +--- +Wide optical double star, which can be observed as two stars with magnitudes 4.1 and 5.1 through a small telescope or a powerful refractor. The fainter star rapidly rotates around the primary star, emitting gas streams, which occasionally cause small changes in brightness. \ No newline at end of file diff --git a/en/star/hr4905.md b/en/star/hr4905.md new file mode 100644 index 000000000..bfaa0076e --- /dev/null +++ b/en/star/hr4905.md @@ -0,0 +1,9 @@ +--- +name: Alioth (ε UMa) +constellation: UMa +created_by: editor.cs +created_date: 2023-11-05 16:44:00.574397 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:00.574401 +--- +The brightest star of the constellation. It is a short-period variable star and also a binary star, with components having an orbital period of 4.15 years, which can only be discerned through spectroscopic methods. The variation in its brightness in a period of 5.09 days is only within a range of 0.1mag and therefore cannot be observed with the naked eye. The star belongs to the type of stars α2 Canum Venaticorum, which also exhibit variations in their magnetic field. \ No newline at end of file diff --git a/en/star/hr4915.md b/en/star/hr4915.md new file mode 100644 index 000000000..8869c9c93 --- /dev/null +++ b/en/star/hr4915.md @@ -0,0 +1,9 @@ +--- +name: Cor Caroli (α CVn) +constellation: CVn +created_by: editor.cs +created_date: 2023-11-05 17:49:16.382429 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:16.382433 +--- +"Karlovo srdce", the brightest star of the constellation. This star was named by Edmund Halley on the suggestion of Sir Charles Scarborough, the court physician and physicist, who claimed that the star shone exceptionally brightly on May 29, 1660, when the English king Charles II, the founder of the Greenwich Observatory, returned to London. Another story says that it is the heart of King Charles I, executed on the orders of Oliver Cromwell in the mid-17th century, which made its way to the sky. \ No newline at end of file diff --git a/en/star/hr4952.md b/en/star/hr4952.md new file mode 100644 index 000000000..bd8a90297 --- /dev/null +++ b/en/star/hr4952.md @@ -0,0 +1,9 @@ +--- +name: θ Mus +constellation: Mus +created_by: editor.cs +created_date: 2023-11-05 16:38:51.905101 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:51.905104 +--- +A binary star, whose components with magnitudes of 5.6 and 7.6 can be separated with a small telescope. The brighter star is a luminous blue supergiant, while its companion is an example of a Wolf-Rayet star - a hot star that has lost its outer layers. \ No newline at end of file diff --git a/en/star/hr4963.md b/en/star/hr4963.md new file mode 100644 index 000000000..800ca8c31 --- /dev/null +++ b/en/star/hr4963.md @@ -0,0 +1,9 @@ +--- +name: θ Virginis +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 16:47:11.295770 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:11.295774 +--- +A remarkable triple star system, located at a distance of 200 light years. The two brighter components are separated by 7.2" and have magnitudes of 4.4 and 9.4. To resolve them, a telescope with an objective diameter of 6 to 8 cm is needed. In a good 100 instrument, a third companion of magnitude 10.4 will also be visible, at a separation of 69.6" from the main white star (the second component appears faintly yellow). \ No newline at end of file diff --git a/en/star/hr4968.md b/en/star/hr4968.md new file mode 100644 index 000000000..0e44be81e --- /dev/null +++ b/en/star/hr4968.md @@ -0,0 +1,9 @@ +--- +name: Diadém (α Com) +constellation: Com +created_by: editor.cs +created_date: 2023-11-05 16:31:51.450720 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:51.450723 +--- +The star, which appears as a point with a magnitude of 4.3 to the naked eye, is actually a binary star consisting of two components with a brightness of 5.1 magnitude. However, we cannot distinguish them with a small telescope. They orbit each other every 25.85 years. \ No newline at end of file diff --git a/en/star/hr4990.md b/en/star/hr4990.md new file mode 100644 index 000000000..1f2e5f3d9 --- /dev/null +++ b/en/star/hr4990.md @@ -0,0 +1,9 @@ +--- +name: 54 Virginis +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 17:50:28.624803 +updated_by: editor.cs +updated_date: 2023-11-05 17:50:28.624806 +--- +An attractive pair of yellow (6.8 mag) and white stars (7.3 mag) at a separation of 5.4" is visible even in small telescopes at 100x magnification. \ No newline at end of file diff --git a/en/star/hr5056.md b/en/star/hr5056.md new file mode 100644 index 000000000..f1f973bc3 --- /dev/null +++ b/en/star/hr5056.md @@ -0,0 +1,9 @@ +--- +name: Spika (α Virginis) +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 16:40:02.623264 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:02.623269 +--- +The brightest star of the constellation, reaching a magnitude of 1. This purely white, bright star can be used for orientation in the spring sky, as it forms the so-called spring triangle along with the stars Regulus in Leo and Arcturus in Bootes, a kind of counterpart to the better-known summer triangle. It is located on the extended line connecting the upper right and lower left wheels of the Big Dipper. It is about 250 light-years away and exceeds the brightness of the Sun by a factor of 2,800. It is a very close spectroscopic binary star (an eclipsing variable star) with a period of 4.014 days. During this period, there is a regular slight partial eclipse, about one-tenth of the brightness, which is not visually perceptible. The main star of this pair also exhibits weak pulsation with a period of 0.174 days. Spica has a surface temperature of nearly 20,000 ˚C and shines with the power of more than a thousand Suns. \ No newline at end of file diff --git a/en/star/hr509.md b/en/star/hr509.md new file mode 100644 index 000000000..e688a4977 --- /dev/null +++ b/en/star/hr509.md @@ -0,0 +1,9 @@ +--- +name: τ Cet +constellation: Cet +created_by: editor.cs +created_date: 2023-11-05 16:49:15.633332 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:15.633336 +--- +Its slow rotation points to the possible existence of a planetary system and thus the possibility of the emergence and existence of life on this yellow dwarf star similar to the Sun (both in temperature and luminous power). It would be one of our closest planetary systems, located 11.85 light-years away from Earth. Therefore, it was selected for the Ozma project, whose goal is to establish contact with potential nearby civilizations through radio waves. Along with the star Epsilon Eridani, it was also chosen for the original research project of SETI (Search for Extra-Terrestrial Intelligence). \ No newline at end of file diff --git a/en/star/hr5127.md b/en/star/hr5127.md new file mode 100644 index 000000000..f18f0896c --- /dev/null +++ b/en/star/hr5127.md @@ -0,0 +1,9 @@ +--- +name: 25 Canum Venaticorum +constellation: CVn +created_by: editor.cs +created_date: 2023-11-05 15:03:47.719172 +updated_by: editor.cs +updated_date: 2023-11-05 15:03:47.719176 +--- +A binary star that splits into two yellow components of brightness 5mag and 6.9mag in a 15 cm telescope. Their angular separation is 1.8". \ No newline at end of file diff --git a/en/star/hr514.md b/en/star/hr514.md new file mode 100644 index 000000000..a7ab15dbd --- /dev/null +++ b/en/star/hr514.md @@ -0,0 +1,9 @@ +--- +name: ε Scl +constellation: Scl +created_by: editor.cs +created_date: 2023-11-05 16:14:25.271224 +updated_by: editor.cs +updated_date: 2023-11-05 16:14:25.271228 +--- +A physical binary star with an orbital period of 1,200 years, whose components have magnitudes of 5.4 and 8.6 and are separated by 4.7". They can be resolved with a 100 mm telescope. Both stars have a yellow color and are located 92 light-years away. \ No newline at end of file diff --git a/en/star/hr5159.md b/en/star/hr5159.md new file mode 100644 index 000000000..3a19f63ce --- /dev/null +++ b/en/star/hr5159.md @@ -0,0 +1,9 @@ +--- +name: 84 Virginis +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 17:15:14.854202 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:14.854206 +--- +Double star consisting of a close pair of conspicuously orange (5.5 mag) and dimly yellow components (7.9 mag) with a separation of 2.9". A telescope with an objective diameter of around 100 mm is recommended for resolution. \ No newline at end of file diff --git a/en/star/hr5210.md b/en/star/hr5210.md new file mode 100644 index 000000000..8b640b1bb --- /dev/null +++ b/en/star/hr5210.md @@ -0,0 +1,9 @@ +--- +name: 3 Cen +constellation: Cen +created_by: editor.cs +created_date: 2023-11-05 15:39:54.583922 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:54.583925 +--- +A remarkable pair of unequally bright pale blue stars with magnitudes of 4.5 and 6, which are separated by 7.9". \ No newline at end of file diff --git a/en/star/hr5221.md b/en/star/hr5221.md new file mode 100644 index 000000000..2453ff347 --- /dev/null +++ b/en/star/hr5221.md @@ -0,0 +1,9 @@ +--- +name: 4 Cen +constellation: Cen +created_by: editor.cs +created_date: 2023-11-05 17:51:24.814952 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:24.814956 +--- +An attractive double star composed of a pale blue 4.7 magnitude component and a gray-white component with a magnitude of 8.4, which is located at a distance of 14.9". \ No newline at end of file diff --git a/en/star/hr5261.md b/en/star/hr5261.md new file mode 100644 index 000000000..ef3399840 --- /dev/null +++ b/en/star/hr5261.md @@ -0,0 +1,9 @@ +--- +name: θ Aps +constellation: Aps +created_by: editor.cs +created_date: 2023-11-05 15:02:04.120431 +updated_by: editor.cs +updated_date: 2023-11-05 15:02:04.120435 +--- +Variable, clearly red star, during maximum at the limit of visibility with the naked eye. Its brightness ranges between 6.4mag and 8mag with a period of just over 100 days. \ No newline at end of file diff --git a/en/star/hr5326.md b/en/star/hr5326.md new file mode 100644 index 000000000..42bb45428 --- /dev/null +++ b/en/star/hr5326.md @@ -0,0 +1,9 @@ +--- +name: R Cen +constellation: Cen +created_by: editor.cs +created_date: 2023-11-05 16:49:11.145975 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:11.145979 +--- +The variable star of Mira type is located between the stars α and β Centauri. Its brightness varies from 5.3mag to 11.8mag over a period of 546 days. \ No newline at end of file diff --git a/en/star/hr5340.md b/en/star/hr5340.md new file mode 100644 index 000000000..b272d201f --- /dev/null +++ b/en/star/hr5340.md @@ -0,0 +1,9 @@ +--- +name: Arktur (α Bootis) +constellation: Boo +created_by: editor.cs +created_date: 2023-11-05 17:31:31.329877 +updated_by: editor.cs +updated_date: 2023-11-05 17:31:31.329880 +--- +"The Guardian of the Bear" is the brightest star in the northern sky and the fourth brightest overall (0.0 mag) after Sirius, Canopus, and Alpha Centauri. It is aimed at by a fourfold extended line connecting the stars of the Big Dipper downwards. Arcturus is the closest orange giant, located 35 light-years away with a diameter of around 30 million kilometers. It is 20 times larger than the Sun, but its luminosity exceeds it by up to 100 times. \ No newline at end of file diff --git a/en/star/hr5409.md b/en/star/hr5409.md new file mode 100644 index 000000000..5ce13b9f7 --- /dev/null +++ b/en/star/hr5409.md @@ -0,0 +1,9 @@ +--- +name: φ Virginis +constellation: Vir +created_by: editor.cs +created_date: 2023-11-05 16:35:55.103805 +updated_by: editor.cs +updated_date: 2023-11-05 16:35:55.103809 +--- +The triple star system consists of two stars (yellow and orange) with magnitudes of 4.8 and 9.3, separated by 4.8", and a third blue component with a magnitude of 12.4 at a separation of 93". \ No newline at end of file diff --git a/en/star/hr546.md b/en/star/hr546.md new file mode 100644 index 000000000..259034456 --- /dev/null +++ b/en/star/hr546.md @@ -0,0 +1,9 @@ +--- +name: Mesarthim (γ Arietis) +constellation: Ari +created_by: editor.cs +created_date: 2023-11-05 17:29:52.128521 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:52.128525 +--- +A charming double star, composed of blue-white components with magnitudes 4.7 and 4.8, separated by 7.8", which can be resolved with a 5 cm telescope. Mesarthim is visible to the naked eye as a star with magnitude 3.9. Historically, it is interesting because it was one of the first double stars discovered by a telescope, observed by the English naturalist Robert Hooke in 1664 while observing a comet. It is located 204 light-years away. \ No newline at end of file diff --git a/en/star/hr5463.md b/en/star/hr5463.md new file mode 100644 index 000000000..a619f8f0b --- /dev/null +++ b/en/star/hr5463.md @@ -0,0 +1,9 @@ +--- +name: α Cir +constellation: Cir +created_by: editor.cs +created_date: 2023-11-05 17:52:48.351509 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:48.351514 +--- +The brightest star of the constellation has an apparent magnitude of 3.4. At a separation of 15.7 arcseconds, there is a companion with a magnitude of 8.6, which can already be resolved with a telescope with a 6 cm objective diameter. The system is located at a distance of 54 light years. \ No newline at end of file diff --git a/en/star/hr5469.md b/en/star/hr5469.md new file mode 100644 index 000000000..bc6d06a51 --- /dev/null +++ b/en/star/hr5469.md @@ -0,0 +1,9 @@ +--- +name: α Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 16:00:48.650493 +updated_by: editor.cs +updated_date: 2023-11-05 16:00:48.650497 +--- +The brightest star of the constellation. It varies in apparent magnitude from 2.3mag to 2.8mag in a period of 0.260 days. It has a faint companion with a magnitude of 13.4mag. It is located 460 light-years away. \ No newline at end of file diff --git a/en/star/hr5497.md b/en/star/hr5497.md new file mode 100644 index 000000000..9636bcb37 --- /dev/null +++ b/en/star/hr5497.md @@ -0,0 +1,9 @@ +--- +name: 54 Hya +constellation: Hya +created_by: editor.cs +created_date: 2023-11-05 17:44:13.557261 +updated_by: editor.cs +updated_date: 2023-11-05 17:44:13.557265 +--- +The double star is composed of components with magnitudes 5.1 and 7.1, which can be easily distinguished even with small telescopes at a separation of 8.6". Notice the color of both stars, one is bright and the other is dark yellow. \ No newline at end of file diff --git a/en/star/hr5506.md b/en/star/hr5506.md new file mode 100644 index 000000000..ce46934b4 --- /dev/null +++ b/en/star/hr5506.md @@ -0,0 +1,9 @@ +--- +name: Izar (ε Bootis) +constellation: Boo +created_by: editor.cs +created_date: 2023-11-05 17:29:10.258161 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:10.258166 +--- +Mirak or Pulcherrima - "beautiful". The second brightest star in the constellation is a beautiful double star in at least a 10 cm telescope, consisting of an orange component (2.7 mag) and a blue component (4.9 mag) creating a color contrast, with a separation of 2.9". However, you will need higher magnification and a calm night. The distance of the system is 200 light years. \ No newline at end of file diff --git a/en/star/hr5523.md b/en/star/hr5523.md new file mode 100644 index 000000000..87e7cdc18 --- /dev/null +++ b/en/star/hr5523.md @@ -0,0 +1,9 @@ +--- +name: μ Lib +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 16:36:53.504214 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:53.504218 +--- +In a good 100 mm refractor, we will see the binary star as a close pair of white stars, like two disks in contact (1.8 "). We will be able to distinguish them completely under calm atmospheric conditions. The components have magnitudes of 5.8 and 6.7. \ No newline at end of file diff --git a/en/star/hr5531.md b/en/star/hr5531.md new file mode 100644 index 000000000..96c2e5fae --- /dev/null +++ b/en/star/hr5531.md @@ -0,0 +1,9 @@ +--- +name: Zubenelgenubi (α Lib) +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 15:16:16.982937 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:16.982941 +--- +The name means "southern clapper" and refers to the origin of the constellation. It is a very easily distinguishable binary star that can be observed with a small telescope. The primary component has a magnitude of 2.75 and is separated by 231" from the companion with a magnitude of 5.8. In terms of classification, it is a bright wide pair consisting of a white and yellow component. Since both stars exhibit the same proper motion, they are likely a physical binary. Its distance from Earth is 75 light-years. \ No newline at end of file diff --git a/en/star/hr5586.md b/en/star/hr5586.md new file mode 100644 index 000000000..e9f520ecd --- /dev/null +++ b/en/star/hr5586.md @@ -0,0 +1,9 @@ +--- +name: δ Lib +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 17:53:26.307589 +updated_by: editor.cs +updated_date: 2023-11-05 17:53:26.307594 +--- +An eclipsing variable star similar to Algol has a period of 2.32 days and its brightness ranges from 4.92 to 5.9 magnitude. The entire cycle of brightness changes can be observed with the naked eye. The change from maximum to minimum occurs in about 6 hours, which can be noticed in a single spring night. Among the main minima, there is one insignificant secondary minimum, which only reaches a tenth of the stellar magnitude, making it difficult to perceive. The system is located nearly 300 light-years away from Earth. \ No newline at end of file diff --git a/en/star/hr5605.md b/en/star/hr5605.md new file mode 100644 index 000000000..9c09884bd --- /dev/null +++ b/en/star/hr5605.md @@ -0,0 +1,9 @@ +--- +name: π Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 16:11:11.720206 +updated_by: editor.cs +updated_date: 2023-11-05 16:11:11.720210 +--- +A nice system of almost equally bright pale blue stars, which however requires a relatively large magnification to be able to distinguish it. The stars are only 1.4" apart. Their magnitudes are 4.6 and 4.7. They are located at a distance of 440 light years. \ No newline at end of file diff --git a/en/star/hr5646.md b/en/star/hr5646.md new file mode 100644 index 000000000..4390c449f --- /dev/null +++ b/en/star/hr5646.md @@ -0,0 +1,9 @@ +--- +name: κ Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 18:11:53.642535 +updated_by: editor.cs +updated_date: 2023-11-05 18:11:53.642540 +--- +A nice double star, whose white components with magnitudes of 3.9 and 5.8 have a separation of 26.8", so a telescope with a 5 cm objective is sufficient for their resolution. It is only an optical double star. \ No newline at end of file diff --git a/en/star/hr5652.md b/en/star/hr5652.md new file mode 100644 index 000000000..7d7d89a28 --- /dev/null +++ b/en/star/hr5652.md @@ -0,0 +1,9 @@ +--- +name: ι Lib +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 17:44:50.593248 +updated_by: editor.cs +updated_date: 2023-11-05 17:44:50.593252 +--- +A complex multiple star, which appears as a single star with a brightness of 4.2 mag when observed with the naked eye. The finder will show its companion labeled as 25 Librae. A telescope with an objective diameter over 80 mm will reveal that the primary star has a faint companion of 9 mag at a separation of 58". With a larger telescope and appropriate magnification, it should eventually be proven that it itself is a close binary star. Its faint companion of 11 mag is located at a separation of 1.9" from it. \ No newline at end of file diff --git a/en/star/hr5670.md b/en/star/hr5670.md new file mode 100644 index 000000000..c141578f1 --- /dev/null +++ b/en/star/hr5670.md @@ -0,0 +1,9 @@ +--- +name: β Cir +constellation: Cir +created_by: editor.cs +created_date: 2023-11-05 16:29:40.295758 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:40.295761 +--- +A main sequence star with a visual magnitude of 4.1, shining from a distance of 97 light years. \ No newline at end of file diff --git a/en/star/hr5683.md b/en/star/hr5683.md new file mode 100644 index 000000000..2409a18bd --- /dev/null +++ b/en/star/hr5683.md @@ -0,0 +1,9 @@ +--- +name: μ Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 15:41:40.884501 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:40.884507 +--- +A triple star system, whose main two white components have a magnitude of 5.1mag and 5.2mag. They are located in close proximity of 1.2" and are a good test for a 100 mm telescope. The brighter component also has a yellow companion of magnitude 7.3mag, which is located at a distance of 23.7" and is visible even in a smaller telescope. \ No newline at end of file diff --git a/en/star/hr5685.md b/en/star/hr5685.md new file mode 100644 index 000000000..5e6bc309b --- /dev/null +++ b/en/star/hr5685.md @@ -0,0 +1,9 @@ +--- +name: Zubenelschemali (β Lib) +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 16:37:41.459440 +updated_by: editor.cs +updated_date: 2023-11-05 16:37:41.459443 +--- +"The Northern Tap" is slightly brighter (2.61 mag) and has a peculiar greenish tint, which is somewhat unusual. The star is approximately 100 times more luminous than the Sun. \ No newline at end of file diff --git a/en/star/hr569.md b/en/star/hr569.md new file mode 100644 index 000000000..03297be7d --- /dev/null +++ b/en/star/hr569.md @@ -0,0 +1,9 @@ +--- +name: λ Arietis +constellation: Ari +created_by: editor.cs +created_date: 2023-11-05 17:43:09.004737 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:09.004741 +--- +Double star easily distinguishable in a 10 cm telescope. The yellow-white star (4.9 mag) is located 37.4" away from the pale blue component (7.7 mag). \ No newline at end of file diff --git a/en/star/hr5704.md b/en/star/hr5704.md new file mode 100644 index 000000000..6e26f8a5d --- /dev/null +++ b/en/star/hr5704.md @@ -0,0 +1,9 @@ +--- +name: γ Cir +constellation: Cir +created_by: editor.cs +created_date: 2023-11-05 16:13:30.486501 +updated_by: editor.cs +updated_date: 2023-11-05 16:13:30.486504 +--- +A binary star composed of components with magnitudes 5.1 and 5.5 in close proximity of only 0.6". It is a good test for a 150 mm telescope. The components orbit each other every 180 years. \ No newline at end of file diff --git a/en/star/hr5733.md b/en/star/hr5733.md new file mode 100644 index 000000000..1449bdc3c --- /dev/null +++ b/en/star/hr5733.md @@ -0,0 +1,9 @@ +--- +name: Alkalurops (μ Bootes) +constellation: Boo +created_by: editor.cs +created_date: 2023-11-05 17:56:51.800520 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:51.800526 +--- +easily distinguishable triple stars. Besides the main yellow component (4.5 mag), we will see a companion at a distance of 108.3" with a magnitude of 7.1, which, when observed with at least an 8 cm telescope, will split into two stars of approximately half a magnitude difference (7 mag and 7.6 mag) (orange and yellow, separated by 2.3"). \ No newline at end of file diff --git a/en/star/hr5735.md b/en/star/hr5735.md new file mode 100644 index 000000000..68cbc9647 --- /dev/null +++ b/en/star/hr5735.md @@ -0,0 +1,9 @@ +--- +name: Pherkad (γ UMi) +constellation: UMi +created_by: editor.cs +created_date: 2023-11-05 17:28:51.825834 +updated_by: editor.cs +updated_date: 2023-11-05 17:28:51.825838 +--- +The "Blue-White" second star of the Little Dipper, near which the orange star 11 Ursae minoris is located. The Arabs called it Pherkad - "two calves", later distinguishing between Pherkad Maior (3.05 mag) and Pherkad Minor (5.02 mag). They form only an optical double star, with their components being separated by 480 and 390 light-years, respectively. \ No newline at end of file diff --git a/en/star/hr5763.md b/en/star/hr5763.md new file mode 100644 index 000000000..b9c2068a7 --- /dev/null +++ b/en/star/hr5763.md @@ -0,0 +1,9 @@ +--- +name: ν Boo +constellation: Boo +created_by: editor.cs +created_date: 2023-11-05 16:25:09.607985 +updated_by: editor.cs +updated_date: 2023-11-05 16:25:09.607989 +--- +A binary star distinguishable by the naked eye, consisting of an orange and yellow-white component with a separation of 14'. Both stars have an approximate magnitude of 5. \ No newline at end of file diff --git a/en/star/hr5788.md b/en/star/hr5788.md new file mode 100644 index 000000000..5ab425da1 --- /dev/null +++ b/en/star/hr5788.md @@ -0,0 +1,9 @@ +--- +name: δ Ser +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 16:44:58.134149 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:58.134152 +--- +The close pale yellow companions have magnitudes of 4.2 and 5.2. They orbit each other with a period of 3.170 years. In the sky, we perceive them as a pair with a separation of 4.4". In a large telescope, we can also see two faint companions with magnitudes of 14.7 and 15. \ No newline at end of file diff --git a/en/star/hr5812.md b/en/star/hr5812.md new file mode 100644 index 000000000..3ad291dbb --- /dev/null +++ b/en/star/hr5812.md @@ -0,0 +1,9 @@ +--- +name: τ Lib +constellation: Lib +created_by: editor.cs +created_date: 2023-11-05 17:43:56.998907 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:56.998911 +--- +The pair of stars with magnitudes 4.7 and 9.7 is separated by 8.5", so we can distinguish them with a telescope of at least 6 cm. The system is located 367 light-years away from Earth. \ No newline at end of file diff --git a/en/star/hr5854.md b/en/star/hr5854.md new file mode 100644 index 000000000..7c65a6181 --- /dev/null +++ b/en/star/hr5854.md @@ -0,0 +1,9 @@ +--- +name: Unukalhai (α Ser) +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 16:34:22.860141 +updated_by: editor.cs +updated_date: 2023-11-05 16:34:22.860145 +--- +The brightest star of the constellation has a magnitude of 2.65. It is located 74 light-years away from Earth and its luminosity exceeds that of the Sun by 35 times. It belongs to the spectral class K2 and is an orange giant. \ No newline at end of file diff --git a/en/star/hr5867.md b/en/star/hr5867.md new file mode 100644 index 000000000..1f0ef9f39 --- /dev/null +++ b/en/star/hr5867.md @@ -0,0 +1,9 @@ +--- +name: β Ser +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 16:50:23.154980 +updated_by: editor.cs +updated_date: 2023-11-05 16:50:23.154984 +--- +A binary star, with its yellow and blue components having magnitudes of 3.7 and 9.9, respectively, and separated by 31". They can be resolved even with a small telescope. The system is located 155 light-years away from Earth. At a distance of 201", we can still observe a component with a magnitude of 10.7. \ No newline at end of file diff --git a/en/star/hr5880.md b/en/star/hr5880.md new file mode 100644 index 000000000..a9b54106a --- /dev/null +++ b/en/star/hr5880.md @@ -0,0 +1,9 @@ +--- +name: R CrB +constellation: CrB +created_by: editor.cs +created_date: 2023-11-05 15:46:51.129348 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:51.129351 +--- +The main representative of the working group of variable stars, in which there are sudden drops in brightness at irregular intervals by several stellar classes. The apparent brightness of this luminous giant remains at 5.8 mag for most of the time, then drops to 13.8 mag or sometimes even to 15 mag within a few weeks and remains so for several months. The giant star ejects a huge cloud of carbon-rich gas into the surrounding area through thermonuclear reactions, which obscures the star's light and causes the sharp drop in brightness that we observe. When the cloud disperses, the star shines again with undiminished light. \ No newline at end of file diff --git a/en/star/hr5894.md b/en/star/hr5894.md new file mode 100644 index 000000000..6ad620e57 --- /dev/null +++ b/en/star/hr5894.md @@ -0,0 +1,9 @@ +--- +name: R Ser +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 15:28:50.240307 +updated_by: editor.cs +updated_date: 2023-11-05 15:28:50.240311 +--- +A variable star of the Mira type located 10 degrees from the star Unukalhai between β and γ Ser, which reaches a maximum magnitude of 6, but disappears from view even with averted vision during its minimum, as it drops to 13.4 mag. The period of its brightness variation is approximately 1 year - 357 days. \ No newline at end of file diff --git a/en/star/hr5897.md b/en/star/hr5897.md new file mode 100644 index 000000000..a862f318b --- /dev/null +++ b/en/star/hr5897.md @@ -0,0 +1,9 @@ +--- +name: β TrA +constellation: TrA +created_by: editor.cs +created_date: 2023-11-05 17:54:22.737615 +updated_by: editor.cs +updated_date: 2023-11-05 17:54:22.737619 +--- +The main component has a brightness of 2.9 mag and is separated by 155 "from a "faint companion of 14 mag, which is not physically related to it. The brighter component has a white hue and is located 40 light-years away. \ No newline at end of file diff --git a/en/star/hr591.md b/en/star/hr591.md new file mode 100644 index 000000000..f88a369c5 --- /dev/null +++ b/en/star/hr591.md @@ -0,0 +1,9 @@ +--- +name: α Hyi +constellation: Hyi +created_by: editor.cs +created_date: 2023-11-05 16:42:05.638028 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:05.638033 +--- +A yellow star with a brightness of 2.9 magnitude. It is located just 30 light-years away from Earth. \ No newline at end of file diff --git a/en/star/hr5925.md b/en/star/hr5925.md new file mode 100644 index 000000000..dcc504601 --- /dev/null +++ b/en/star/hr5925.md @@ -0,0 +1,9 @@ +--- +name: ξ Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 15:27:56.398937 +updated_by: editor.cs +updated_date: 2023-11-05 15:27:56.398940 +--- +Clear, relatively wide pair (10.4"), easily distinguishable in small telescopes. The components have magnitudes of 5.3 and 5.8, with observers perceiving their colors differently: some see them as light yellow, while others say that one has a white and the other a greenish tint. Generally, stars with an AO spectrum appear white to pale blue. \ No newline at end of file diff --git a/en/star/hr5939.md b/en/star/hr5939.md new file mode 100644 index 000000000..b4f2e2c38 --- /dev/null +++ b/en/star/hr5939.md @@ -0,0 +1,9 @@ +--- +name: S TrA +constellation: TrA +created_by: editor.cs +created_date: 2023-11-05 15:44:47.782282 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:47.782286 +--- +Another bright Cepheid. This time with a period of 6.323 days and a magnitude range from 6.1 to 6.7. \ No newline at end of file diff --git a/en/star/hr5948.md b/en/star/hr5948.md new file mode 100644 index 000000000..e206bb064 --- /dev/null +++ b/en/star/hr5948.md @@ -0,0 +1,9 @@ +--- +name: η Lup +constellation: Lup +created_by: editor.cs +created_date: 2023-11-05 17:43:20.312297 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:20.312301 +--- +The triple star system, whose main component has a blue-white color and the companion has a dark blue color. The difference in their brightness is quite significant (3.6 mag and 7.8 mag), but with their separation of 15", we should be able to distinguish them even with a small telescope. The second companion, with a magnitude of 9.4, is located 115" away from the main component. Just to the northeast, there are two pairs of white stars, each 20" wide. \ No newline at end of file diff --git a/en/star/hr5958.md b/en/star/hr5958.md new file mode 100644 index 000000000..37184c7d7 --- /dev/null +++ b/en/star/hr5958.md @@ -0,0 +1,9 @@ +--- +name: T CrB +constellation: CrB +created_by: editor.cs +created_date: 2023-11-05 16:32:37.970834 +updated_by: editor.cs +updated_date: 2023-11-05 16:32:37.970838 +--- +A variable star belonging to recurrent novae, located southeast of the star η CRB. Two outbursts were observed at this star. In 1866, it increased its apparent magnitude from 10.8mag to 2mag, and during the second outburst in 1946, it only reached 3mag. Currently, this star has a magnitude of only 10. The star also occasionally explodes and ejects a large amount of gas. Unlike R CRB, however, it brightens significantly with each explosion. \ No newline at end of file diff --git a/en/star/hr596.md b/en/star/hr596.md new file mode 100644 index 000000000..faa98fa5e --- /dev/null +++ b/en/star/hr596.md @@ -0,0 +1,9 @@ +--- +name: Al Rischa (α Psc) +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 15:42:56.100713 +updated_by: editor.cs +updated_date: 2023-11-05 15:42:56.100717 +--- +From an astronomical point of view, Al Risch is a close binary star (total magnitude 4), with its pale blue components of magnitude 4.3 and 5.2 orbiting each other with a period of 933 years. Currently, they are separated by 1.5" in the sky, requiring a telescope with a 300 mm objective diameter to resolve them. Even at 200x magnification, they appear in close contact. However, due to their orbit, the separation decreases gradually each year, reaching its lowest value of 1" in 2060. The system is located at a distance of 130 light-years and both components are also a spectroscopic binary. \ No newline at end of file diff --git a/en/star/hr5961.md b/en/star/hr5961.md new file mode 100644 index 000000000..014a49a68 --- /dev/null +++ b/en/star/hr5961.md @@ -0,0 +1,9 @@ +--- +name: ι1 Nor +constellation: Nor +created_by: editor.cs +created_date: 2023-11-05 16:45:11.281416 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:11.281420 +--- +A binary star with components of 4.6 and 8.1 magnitude, which can be resolved with a small telescope at a separation of 10.8 arcseconds. ι2 is not physically associated with it and lies slightly further away in the sky. \ No newline at end of file diff --git a/en/star/hr5984.md b/en/star/hr5984.md new file mode 100644 index 000000000..9cf735fe6 --- /dev/null +++ b/en/star/hr5984.md @@ -0,0 +1,9 @@ +--- +name: Graffias (β Sco) +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 17:52:55.405296 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:55.405300 +--- +It is a binary star with components of 2.6 mag and 4.9 mag, separated by 13.6". The primary component is pale blue, the companion is dark blue, but there is no relationship between them. However, the brighter component itself is a close binary star that is not easy to distinguish even in a larger telescope. \ No newline at end of file diff --git a/en/star/hr5993.md b/en/star/hr5993.md new file mode 100644 index 000000000..00e2f510f --- /dev/null +++ b/en/star/hr5993.md @@ -0,0 +1,9 @@ +--- +name: ω Sco +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 17:51:52.256582 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:52.256587 +--- +An optical binary star visible to the naked eye, composed of stars with magnitudes 3.9 and 4.3. One is located 470 light-years away from us and the other is 290 light-years away. \ No newline at end of file diff --git a/en/star/hr6008.md b/en/star/hr6008.md new file mode 100644 index 000000000..60f2b3089 --- /dev/null +++ b/en/star/hr6008.md @@ -0,0 +1,9 @@ +--- +name: Marfak (κ Her) +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 15:04:00.082393 +updated_by: editor.cs +updated_date: 2023-11-05 15:04:00.082398 +--- +A physical binary star, whose yellow components with magnitudes of 5.3 and 6.5 are separated by 28.4", and therefore can be resolved even in small telescopes. 36" to the SSW there is another companion with a magnitude of 13.6. \ No newline at end of file diff --git a/en/star/hr6020.md b/en/star/hr6020.md new file mode 100644 index 000000000..5f85762f1 --- /dev/null +++ b/en/star/hr6020.md @@ -0,0 +1,9 @@ +--- +name: δ Aps +constellation: Aps +created_by: editor.cs +created_date: 2023-11-05 16:31:36.467841 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:36.467845 +--- +Very wide double star, easily distinguishable even with a regular telescope. The components with magnitudes 4.7 and 5.1 are separated by 103", but they are not physically related at all. These are red giants located at distances of 660 and 760 light years. \ No newline at end of file diff --git a/en/star/hr6027.md b/en/star/hr6027.md new file mode 100644 index 000000000..39696047e --- /dev/null +++ b/en/star/hr6027.md @@ -0,0 +1,9 @@ +--- +name: ν Sco +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 15:15:50.485293 +updated_by: editor.cs +updated_date: 2023-11-05 15:15:50.485296 +--- +With a small telescope, we can distinguish two optical components with a brightness of 4.3 mag and 6.4 mag at a separation of 44". The main star is already a true binary star, with a companion of 6.8 mag located at a separation of only 0.9". The companion of the second star, with a brightness of 7.8 mag, is located at a separation of 2.3" and is within the reach of an 80 mm telescope. \ No newline at end of file diff --git a/en/star/hr603.md b/en/star/hr603.md new file mode 100644 index 000000000..29c3aafef --- /dev/null +++ b/en/star/hr603.md @@ -0,0 +1,9 @@ +--- +name: Alamak (γ Adromedae) +constellation: And +created_by: editor.cs +created_date: 2023-11-05 17:52:19.427741 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:19.427745 +--- +The star is located 350 light-years away. To the north of it lies the radiant of the Andromedids meteor shower. One of the most beautiful double stars in the sky. The primary component is orange and has a brightness of 2.3 magnitude, while the companion is greenish-blue and has a brightness of 5.5 magnitude. It is also a close double star (0.5"), but it is not observable with smaller amateur telescopes (in a larger telescope, it appears as a slightly elongated, blurry star). Its orbital period is 61 years. The angular distance between the primary components of Alamak is 9.8 arc seconds, so we can resolve them even with a small telescope with a 5 cm objective diameter. \ No newline at end of file diff --git a/en/star/hr6063.md b/en/star/hr6063.md new file mode 100644 index 000000000..a99dbfc1d --- /dev/null +++ b/en/star/hr6063.md @@ -0,0 +1,9 @@ +--- +name: σ CrB +constellation: CrB +created_by: editor.cs +created_date: 2023-11-05 16:48:31.471400 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:31.471404 +--- +A binary star, with the primary component having a brightness of 5.6 magnitude, is accompanied by a 6.6 magnitude companion at a separation of 7.1 arcseconds. The companion orbits the primary star every 1,160 years. In a 100 mm telescope, we can easily distinguish the fainter and darker components. \ No newline at end of file diff --git a/en/star/hr6072.md b/en/star/hr6072.md new file mode 100644 index 000000000..165baf11e --- /dev/null +++ b/en/star/hr6072.md @@ -0,0 +1,9 @@ +--- +name: γ1 a γ2 Nor +constellation: Nor +created_by: editor.cs +created_date: 2023-11-05 17:46:43.147684 +updated_by: editor.cs +updated_date: 2023-11-05 17:46:43.147688 +--- +Gamma2 Dor is the brightest star in the constellation with its apparent magnitude of 4.14. Gamma1 Dor forms an optical double star with it, which can be distinguished with the naked eye. Gamma2 Dor is an orange giant located 130 light-years away, and its companion with a magnitude of 5 is a bright white subgiant, which is more than 100 times farther away. Additionally, in a telescope, we can find a 10th magnitude companion at a separation of 45 arcseconds from Gamma2 Dor. \ No newline at end of file diff --git a/en/star/hr6084.md b/en/star/hr6084.md new file mode 100644 index 000000000..aa0a70fbd --- /dev/null +++ b/en/star/hr6084.md @@ -0,0 +1,9 @@ +--- +name: σ Sco +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 17:32:01.476839 +updated_by: editor.cs +updated_date: 2023-11-05 17:32:01.476843 +--- +The variable star, whose brightness varies between 3mag and 3.8mag in a period of 0.247 days, is also a binary star. The companion, with a magnitude of 9mag, is located at a separation of 20". \ No newline at end of file diff --git a/en/star/hr6107.md b/en/star/hr6107.md new file mode 100644 index 000000000..46b6d3f81 --- /dev/null +++ b/en/star/hr6107.md @@ -0,0 +1,9 @@ +--- +name: ν CrB +constellation: CrB +created_by: editor.cs +created_date: 2023-11-05 17:45:36.735109 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:36.735113 +--- +A binary star, whose components are red giants with magnitudes of 5.2 and 5.4, can be resolved with a telescope because they have a separation of 370". They are located approximately 550 light-years away, but they do not orbit each other. \ No newline at end of file diff --git a/en/star/hr6112.md b/en/star/hr6112.md new file mode 100644 index 000000000..04668e6d0 --- /dev/null +++ b/en/star/hr6112.md @@ -0,0 +1,9 @@ +--- +name: ρ Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 17:51:14.403920 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:14.403924 +--- +A binary star located 3° northwest of Antares, consisting of blue components with magnitudes of 5.3 and 6, separated by 3.1" (4.59 mag). The area around them is interesting for photographers. To the west, there is an elongated dark nebula Barnard 42, which appears as a silhouette against the beautiful gas and dust complex IC 4604, illuminated by the star ρ Ophiuchi. However, the nebula has a very low surface brightness. \ No newline at end of file diff --git a/en/star/hr6115.md b/en/star/hr6115.md new file mode 100644 index 000000000..2a9f93238 --- /dev/null +++ b/en/star/hr6115.md @@ -0,0 +1,9 @@ +--- +name: ε Nor +constellation: Nor +created_by: editor.cs +created_date: 2023-11-05 17:16:03.207330 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:03.207335 +--- +Nice double star composed of components with magnitudes 4.8 and 7.5, which are separated by 22.8". We can distinguish them even in a small telescope. Both components are also spectroscopic binaries. \ No newline at end of file diff --git a/en/star/hr6116.md b/en/star/hr6116.md new file mode 100644 index 000000000..c859a482e --- /dev/null +++ b/en/star/hr6116.md @@ -0,0 +1,9 @@ +--- +name: η UMi +constellation: UMi +created_by: editor.cs +created_date: 2023-11-05 16:47:21.845176 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:21.845179 +--- +Optical double star, whose main white component is located 97 light-years away from us. When observing with the naked eye and a telescope, we can also see the second component of 19 Ursa Minor and its distant companion (magnitude 5.5), which is almost seven times further away from it. \ No newline at end of file diff --git a/en/star/hr6134.md b/en/star/hr6134.md new file mode 100644 index 000000000..e133384da --- /dev/null +++ b/en/star/hr6134.md @@ -0,0 +1,9 @@ +--- +name: Antares (α Sco) +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 15:27:44.158493 +updated_by: editor.cs +updated_date: 2023-11-05 15:27:44.158497 +--- +In ancient times, people saw a competitor in this star, the counterpart of Mars (anti-Ares: against Mars), as the strikingly red star strongly resembles the "Red Planet". The old Arabic name Kal al Akrab is no longer used, but the Latin designation Cor Scorpion - Heart of the Scorpion is derived from it. It lies at the intersection of the extended lines connecting the lateral sides of the Hercules quadrilateral. A greenish-colored physical companion with a brightness of 5.4 mag can be found at a separation of 2.9" best with a 200mm or larger telescope, as the glare of the main star is obstructive. A minimum magnification of 250x is recommended for visual resolution. The main component orbits approximately every 555 years. \ No newline at end of file diff --git a/en/star/hr6149.md b/en/star/hr6149.md new file mode 100644 index 000000000..a3b0bc64b --- /dev/null +++ b/en/star/hr6149.md @@ -0,0 +1,9 @@ +--- +name: λ Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 16:46:53.790472 +updated_by: editor.cs +updated_date: 2023-11-05 16:46:53.790476 +--- +A nice double star with a period of 130 years. Its components have magnitudes of 4.2 and 5.2 and are separated by 1.5". One of them has a white color, while the other has a light yellow color. At a larger separation, we can also observe two additional, probably optical companions with magnitudes of 9.5 and 11.1. \ No newline at end of file diff --git a/en/star/hr6163.md b/en/star/hr6163.md new file mode 100644 index 000000000..b3bc4ee7f --- /dev/null +++ b/en/star/hr6163.md @@ -0,0 +1,9 @@ +--- +name: β Aps +constellation: Aps +created_by: editor.cs +created_date: 2023-11-05 17:57:29.398632 +updated_by: editor.cs +updated_date: 2023-11-05 17:57:29.398636 +--- +A binary star composed of a brighter component with a magnitude of 4.2 and a companion with a magnitude of 12, separated from it by 51". It is likely just an optical binary star, with its main component being of spectral class K0 and located 158 light-years away. \ No newline at end of file diff --git a/en/star/hr617.md b/en/star/hr617.md new file mode 100644 index 000000000..ea1c151a8 --- /dev/null +++ b/en/star/hr617.md @@ -0,0 +1,9 @@ +--- +name: Hamal (α Aries) +constellation: Ari +created_by: editor.cs +created_date: 2023-11-05 17:30:54.620015 +updated_by: editor.cs +updated_date: 2023-11-05 17:30:54.620020 +--- +The brightest star of the constellation, otherwise unremarkable. This red giant of spectral class K2 has a magnitude of 2 and shines at a distance of 66 light years. Sometimes the star is also referred to as El Nath. \ No newline at end of file diff --git a/en/star/hr6184.md b/en/star/hr6184.md new file mode 100644 index 000000000..b207b2530 --- /dev/null +++ b/en/star/hr6184.md @@ -0,0 +1,9 @@ +--- +name: 16/17 Dra +constellation: Dra +created_by: editor.cs +created_date: 2023-11-05 17:12:23.497989 +updated_by: editor.cs +updated_date: 2023-11-05 17:12:23.497993 +--- +A nice wide double star, distinguishable in binoculars or small telescopes. The brightness of both components is almost 5.5 magnitude, and they are separated by 90.3". In reality, the component 17 Dra has a close companion, which is located at a distance of 3.4". All stars are bright white. \ No newline at end of file diff --git a/en/star/hr6194.md b/en/star/hr6194.md new file mode 100644 index 000000000..e25291251 --- /dev/null +++ b/en/star/hr6194.md @@ -0,0 +1,9 @@ +--- +name: 36/37 Her +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 17:57:35.751227 +updated_by: editor.cs +updated_date: 2023-11-05 17:57:35.751232 +--- +Two ordinary close stars, which can be distinguished even with a hand lens. They are located on the southwestern edge of the constellation at a mutual distance of 70" and their brightness is 5.7 mag and 6.8 mag, respectively. \ No newline at end of file diff --git a/en/star/hr6212.md b/en/star/hr6212.md new file mode 100644 index 000000000..17e2e1cf5 --- /dev/null +++ b/en/star/hr6212.md @@ -0,0 +1,9 @@ +--- +name: ζ Her +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 16:13:01.217654 +updated_by: editor.cs +updated_date: 2023-11-05 16:13:01.217658 +--- +A nice double star in the "Flowerpot". The components have magnitudes of 2.9mag and 5.5mag and are approximately 1.6" apart. Since their orbital period is only 34.5 years, the positional angle and separation change rapidly. \ No newline at end of file diff --git a/en/star/hr6217.md b/en/star/hr6217.md new file mode 100644 index 000000000..267a35c9f --- /dev/null +++ b/en/star/hr6217.md @@ -0,0 +1,9 @@ +--- +name: Atria (α TrA) +constellation: TrA +created_by: editor.cs +created_date: 2023-11-05 15:43:42.939367 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:42.939371 +--- +The brightest star of the constellation is a 2nd magnitude star. The orange color of this star is noticeable even with the naked eye. It is located at a distance of 80 light years. Its name Atria is an abbreviation of the words alpha Triangulum Australis, which were introduced by air navigators during World War II. \ No newline at end of file diff --git a/en/star/hr6247.md b/en/star/hr6247.md new file mode 100644 index 000000000..6b74ce659 --- /dev/null +++ b/en/star/hr6247.md @@ -0,0 +1,9 @@ +--- +name: μ Sco +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 16:47:28.306316 +updated_by: editor.cs +updated_date: 2023-11-05 16:47:28.306319 +--- +A binary star easily distinguishable with the naked eye. The brightness components of 3.1mag and 3.6mag are located at a distance of 8'. The brighter one is an eclipsing binary, whose brightness varies in the range of 34 hours between 2.9 and 3.2mag. \ No newline at end of file diff --git a/en/star/hr6271.md b/en/star/hr6271.md new file mode 100644 index 000000000..b33ef433e --- /dev/null +++ b/en/star/hr6271.md @@ -0,0 +1,9 @@ +--- +name: ζ Sco +constellation: Sco +created_by: editor.cs +created_date: 2023-11-05 16:00:24.870387 +updated_by: editor.cs +updated_date: 2023-11-05 16:00:24.870390 +--- +Wide visual pair of unrelated stars distinguishable even with the naked eye. It consists of the blue-white giant ζ1, which is the brightest member (4.7mag) of the beautiful open star cluster NGC 6231. ζ2 is a red giant with a magnitude of 3.6, which is located much closer to us - 132 light-years away. \ No newline at end of file diff --git a/en/star/hr6402.md b/en/star/hr6402.md new file mode 100644 index 000000000..ead244e34 --- /dev/null +++ b/en/star/hr6402.md @@ -0,0 +1,9 @@ +--- +name: 36 Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 17:43:35.421748 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:35.421754 +--- +A beautiful double star with equally bright orange components of magnitude 5.1, separated by 4.9" and distinguishable even in smaller telescopes. At a larger separation from it, an orange companion of magnitude 8.1 is visible to the northwest. \ No newline at end of file diff --git a/en/star/hr6406.md b/en/star/hr6406.md new file mode 100644 index 000000000..38a42caa2 --- /dev/null +++ b/en/star/hr6406.md @@ -0,0 +1,9 @@ +--- +name: Ras Algethi (α Her) +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 17:29:19.203926 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:19.203929 +--- +A significantly red star is located near the border with Hadonoš, a supergiant whose brightness irregularly varies between 3.1 mag and 3.9 mag, often only between 3.3 mag and 3.7 mag. The period is 90 to 100 days. Suitable comparison stars are ι and κ Ophiuchi, which are located about 6.5 degrees to the southwest and have a brightness of 4.3 mag and 3.2 mag, respectively. Alpha Herculis is also a binary star, with its second component of fifth magnitude located 4.7" away, visible even in small telescopes with a 6 cm objective diameter. It has a greenish tint that nicely contrasts with the red giant. \ No newline at end of file diff --git a/en/star/hr642.md b/en/star/hr642.md new file mode 100644 index 000000000..d8c864a68 --- /dev/null +++ b/en/star/hr642.md @@ -0,0 +1,9 @@ +--- +name: 6 Tri +constellation: Tri +created_by: editor.cs +created_date: 2023-11-05 15:17:12.588629 +updated_by: editor.cs +updated_date: 2023-11-05 15:17:12.588632 +--- +Physical binary star, whose companion of 7 mag. can be distinguished from the primary star of 5 mag. using a small telescope. \ No newline at end of file diff --git a/en/star/hr6431.md b/en/star/hr6431.md new file mode 100644 index 000000000..0a94b6028 --- /dev/null +++ b/en/star/hr6431.md @@ -0,0 +1,9 @@ +--- +name: 68 Her +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 15:02:50.318121 +updated_by: editor.cs +updated_date: 2023-11-05 15:02:50.318125 +--- +An eclipsing binary star. They are actually two strongly flattened, almost equally sized stars that orbit each other in 2.051 days. As a result, we observe light changes of 68 Her from 4.7 mag to 5.4 mag. The brightness of both stars is quite different. The brighter one is 260 times more luminous than the Sun and the weaker one is only 100 times. Their mass reaches 7.5 times and 2.9 times the mass of the Sun. In terms of size, both stars exceed the diameter of the Sun by about 6 times. \ No newline at end of file diff --git a/en/star/hr650.md b/en/star/hr650.md new file mode 100644 index 000000000..78cc29540 --- /dev/null +++ b/en/star/hr650.md @@ -0,0 +1,9 @@ +--- +name: 66 Cet +constellation: Cet +created_by: editor.cs +created_date: 2023-11-05 16:40:57.081682 +updated_by: editor.cs +updated_date: 2023-11-05 16:40:57.081686 +--- +The star consists of two companions with magnitudes of 5.7 and 7.5. Their angular separation is 16.5 arcseconds. While in small telescopes they appear as a pair of yellow and blue components, in a 200 mm telescope the color of the second component changes to violet. \ No newline at end of file diff --git a/en/star/hr6536.md b/en/star/hr6536.md new file mode 100644 index 000000000..cd20994a1 --- /dev/null +++ b/en/star/hr6536.md @@ -0,0 +1,9 @@ +--- +name: Rastaban (β Dra) +constellation: Dra +created_by: editor.cs +created_date: 2023-11-05 15:58:16.779053 +updated_by: editor.cs +updated_date: 2023-11-05 15:58:16.779057 +--- +The star has a brightness of 2.8 magnitude and is located 380 light-years away. Together with Etamin, it forms the "Dragon's Eyes". Beta Draconis is a binary star consisting of a main yellow component and a faint companion of 14 magnitude at an angular distance of 4.2", which is not easy to see. \ No newline at end of file diff --git a/en/star/hr6556.md b/en/star/hr6556.md new file mode 100644 index 000000000..2e832febf --- /dev/null +++ b/en/star/hr6556.md @@ -0,0 +1,9 @@ +--- +name: Ras Alhague (α Oph) +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 16:34:42.298725 +updated_by: editor.cs +updated_date: 2023-11-05 16:34:42.298728 +--- +With its 2nd magnitude, it is the brightest star in the constellation. Ras Alhague is located at the northern edge of the constellation and is not very far from a star with a similar name, α Herculis, the main star of Hercules. It is a yellow-white giant star located 48 light-years away from us. This distance is constantly increasing due to its motion of 8 km per second. \ No newline at end of file diff --git a/en/star/hr6623.md b/en/star/hr6623.md new file mode 100644 index 000000000..d53bb31db --- /dev/null +++ b/en/star/hr6623.md @@ -0,0 +1,9 @@ +--- +name: μ Her +constellation: Her +created_by: editor.cs +created_date: 2023-11-05 17:13:36.502364 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:36.502368 +--- +The main and conspicuously yellow component with a brightness of 3.4 magnitude has a companion of 10th stellar magnitude, which is actually composed of two red dwarfs. \ No newline at end of file diff --git a/en/star/hr6705.md b/en/star/hr6705.md new file mode 100644 index 000000000..78e91173a --- /dev/null +++ b/en/star/hr6705.md @@ -0,0 +1,9 @@ +--- +name: Etamin (γ Dra) +constellation: Dra +created_by: editor.cs +created_date: 2023-11-05 15:58:39.257884 +updated_by: editor.cs +updated_date: 2023-11-05 15:58:39.257888 +--- +The brightest star of the constellation reaches a magnitude of 2 and is clearly orange. It is located 154 light-years away from Earth and is 471 times brighter than the Sun. In the past, it was observed by the English astronomer James Bradley, who used it to discover the aberration of light. \ No newline at end of file diff --git a/en/star/hr6734.md b/en/star/hr6734.md new file mode 100644 index 000000000..e49916b48 --- /dev/null +++ b/en/star/hr6734.md @@ -0,0 +1,9 @@ +--- +name: τ Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 17:30:45.005097 +updated_by: editor.cs +updated_date: 2023-11-05 17:30:45.005102 +--- +A binary star, which consists of a beautiful but close pair of yellow stars with magnitudes of 5.2 and 5.9, respectively, and a period of 280 years. Currently, their separation is about 1.7", but it is still decreasing. At a distance of 100", we can find a guide star with a brightness of 9.3 mag. \ No newline at end of file diff --git a/en/star/hr6752.md b/en/star/hr6752.md new file mode 100644 index 000000000..a5608ed9b --- /dev/null +++ b/en/star/hr6752.md @@ -0,0 +1,9 @@ +--- +name: 70 Oph +constellation: Oph +created_by: editor.cs +created_date: 2023-11-05 17:46:02.095582 +updated_by: editor.cs +updated_date: 2023-11-05 17:46:02.095586 +--- +A binary star consisting of two stars with magnitudes of 4.2 and 6 has a mutual orbital period of 87 years. The orbital path has such a spatial position that the apparent angular separation of the two stars significantly changes during the orbital period. The smallest separation (1.5") was reached by both stars in 1989 and 1990. At the turn of the millennium, their separation increased to 3.9", which could be observed even with a telescope with a 5 cm diameter objective. In 2005, the distance increased to 5". The largest separation of 6.8" will be reached by both stars in 2024. \ No newline at end of file diff --git a/en/star/hr6783.md b/en/star/hr6783.md new file mode 100644 index 000000000..937360951 --- /dev/null +++ b/en/star/hr6783.md @@ -0,0 +1,9 @@ +--- +name: ε Tel +constellation: Tel +created_by: editor.cs +created_date: 2023-11-05 15:41:04.088462 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:04.088466 +--- +A binary star composed of a primary component with a brightness of 4.5 magnitude and a faint companion with a magnitude of 13, which is located at a separation of 21". The components are separated by 410 light-years. \ No newline at end of file diff --git a/en/star/hr681.md b/en/star/hr681.md new file mode 100644 index 000000000..9a6fb56bf --- /dev/null +++ b/en/star/hr681.md @@ -0,0 +1,9 @@ +--- +name: Mira Ceti (ο Cet) +constellation: Cet +created_by: editor.cs +created_date: 2023-11-05 16:44:19.109873 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:19.109876 +--- +The most famous long-period variable star, about which the Dutch amateur observer David Fabricius in Germany believed on August 13, 1596 that it was a new star, similar to the recent Tycho's star from 1572. In the then or older atlas, no star of magnitude 3 was drawn in the neck of the Whale. Only during its observation over the next year did he realize that it changes its brightness. As the first one, even before the invention of the telescope during Galileo's time, he discovered the first variable star in the history of astronomy! The star gradually disappeared and reappeared, until in 1603 the German astrocartographer Johann Bayer included it in his atlas as an object of magnitude 4. Later, in 1662, Jan Hevelius named it "Mira stella" - the wonderful star. The tip of the letter "V" formed by the stars from the constellation of Pisces points to it. Mira is located 300 light-years away. \ No newline at end of file diff --git a/en/star/hr6832.md b/en/star/hr6832.md new file mode 100644 index 000000000..e47db9cee --- /dev/null +++ b/en/star/hr6832.md @@ -0,0 +1,9 @@ +--- +name: η Sgr +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 15:16:57.707277 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:57.707281 +--- +Easily observable double star: the magnitudes of the components are 3.2 and 7.8 and they are located at distances of 3.6". The brighter component is red-orange, while the fainter one is white. At a distance of 93", there is a 10th magnitude star, and at a separation of 33", there is a 13th magnitude star. \ No newline at end of file diff --git a/en/star/hr6855.md b/en/star/hr6855.md new file mode 100644 index 000000000..24e4dfeea --- /dev/null +++ b/en/star/hr6855.md @@ -0,0 +1,9 @@ +--- +name: ξ Pav +constellation: Pav +created_by: editor.cs +created_date: 2023-11-05 15:28:38.750459 +updated_by: editor.cs +updated_date: 2023-11-05 15:28:38.750462 +--- +A tight binary star composed of unequally bright stars. It consists of a red giant with a brightness of 4.4 mag and a companion with a brightness of 8 mag. Both components are located 420 light-years away. When observed with a small telescope, it may be difficult to distinguish the fainter star due to the overpowering brightness of the brighter component. \ No newline at end of file diff --git a/en/star/hr6879.md b/en/star/hr6879.md new file mode 100644 index 000000000..44adc959c --- /dev/null +++ b/en/star/hr6879.md @@ -0,0 +1,9 @@ +--- +name: Kaus Australis (ε Sgr) +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 15:58:02.826032 +updated_by: editor.cs +updated_date: 2023-11-05 15:58:02.826037 +--- +The brightest star of the constellation (1.85mag) is located in the southern part of the arc and reaches a maximum height of 7 degrees above the southern horizon at its culmination. It has a white color. It shines as bright as 250 Suns from a distance of 125 light years. It is also an optical double star, with a companion of seventh magnitude located about 3.3 arc minutes to the northwest, which can also be observed with a telescope. \ No newline at end of file diff --git a/en/star/hr6896.md b/en/star/hr6896.md new file mode 100644 index 000000000..ceba9d7a3 --- /dev/null +++ b/en/star/hr6896.md @@ -0,0 +1,9 @@ +--- +name: 21 Sgr +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 16:44:53.626653 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:53.626656 +--- +unequally bright and contrasting double star of orange (4.9mag) and bluish components (7.4mag), which are separated by only 1.8", so they cannot be easily distinguished with a small telescope. \ No newline at end of file diff --git a/en/star/hr6897.md b/en/star/hr6897.md new file mode 100644 index 000000000..fec3a4cca --- /dev/null +++ b/en/star/hr6897.md @@ -0,0 +1,9 @@ +--- +name: α Tel +constellation: Tel +created_by: editor.cs +created_date: 2023-11-05 16:48:04.338141 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:04.338146 +--- +The brightest star of the constellation has a magnitude of 3.76. It is a blue-white star of spectral class B3, located 249 light-years away from us. \ No newline at end of file diff --git a/en/star/hr6918.md b/en/star/hr6918.md new file mode 100644 index 000000000..cf8b35867 --- /dev/null +++ b/en/star/hr6918.md @@ -0,0 +1,9 @@ +--- +name: 59 Ser +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 15:40:16.642265 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:16.642269 +--- +The unevenly bright but attractive double star of yellow 5.3 magnitude and white component of 7.6 magnitude is located in a particularly dark area of the Great Rift. The separation between this pair is 3.8". \ No newline at end of file diff --git a/en/star/hr6923.md b/en/star/hr6923.md new file mode 100644 index 000000000..5eeeb71c7 --- /dev/null +++ b/en/star/hr6923.md @@ -0,0 +1,9 @@ +--- +name: 39 Dra +constellation: Dra +created_by: editor.cs +created_date: 2023-11-05 15:45:54.262906 +updated_by: editor.cs +updated_date: 2023-11-05 15:45:54.262909 +--- +A multiple star that is visible as a wide pair of stars with magnitudes 5 and 8, even with a small telescope or a binocular. Examining the brighter star at high magnification will reveal an additional (and much closer) component, which also has a magnitude of 8. \ No newline at end of file diff --git a/en/star/hr6934.md b/en/star/hr6934.md new file mode 100644 index 000000000..b371ee8a2 --- /dev/null +++ b/en/star/hr6934.md @@ -0,0 +1,9 @@ +--- +name: δ Tel +constellation: Tel +created_by: editor.cs +created_date: 2023-11-05 16:11:06.342007 +updated_by: editor.cs +updated_date: 2023-11-05 16:11:06.342010 +--- +An optical binary star easily distinguishable with the naked eye. It consists of components with brightness of 4.9mag and 5.1mag, located at a distance of 800 and 1,100 light years. \ No newline at end of file diff --git a/en/star/hr6953.md b/en/star/hr6953.md new file mode 100644 index 000000000..2b9c8ff4a --- /dev/null +++ b/en/star/hr6953.md @@ -0,0 +1,9 @@ +--- +name: κ CrA +constellation: CrA +created_by: editor.cs +created_date: 2023-11-05 15:46:19.541034 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:19.541039 +--- +A remarkable binary star in the rich Milky Way, whose both blue-white companions with magnitudes of 5.9 and 6.6 have a separation of 21.4 arcseconds. Therefore, they can be easily distinguished even in a small telescope. \ No newline at end of file diff --git a/en/star/hr7001.md b/en/star/hr7001.md new file mode 100644 index 000000000..f6537d5e1 --- /dev/null +++ b/en/star/hr7001.md @@ -0,0 +1,9 @@ +--- +name: Vega (α Lyr) +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 17:47:32.757554 +updated_by: editor.cs +updated_date: 2023-11-05 17:47:32.757558 +--- +Thanks to this star, the constellation is unmistakable, as the bluish Vega is the fifth brightest star in the sky (0.04 mag). Together with the stars Deneb in Cygnus and Altair in Aquila, Vega forms the Summer Triangle. Its distance from Earth is estimated to be 25 light-years, and it outshines our Sun by a factor of 40, with an absolute magnitude of +0.5. Two faint companions do not form part of the physical system. \ No newline at end of file diff --git a/en/star/hr7020.md b/en/star/hr7020.md new file mode 100644 index 000000000..c968b7eaa --- /dev/null +++ b/en/star/hr7020.md @@ -0,0 +1,9 @@ +--- +name: δ Sct +constellation: Sct +created_by: editor.cs +created_date: 2023-11-05 16:43:11.074979 +updated_by: editor.cs +updated_date: 2023-11-05 16:43:11.074982 +--- +This star is a prototype of a class of variable stars, whose brightness changes very little due to repeated shrinking and expanding of its diameter with a period of several hours. During 4.65 hours, its brightness fluctuates between 4.9mag and 5.2mag. δ Scuti also has a blue companion at a separation of 52.6", which nicely contrasts with the main, bright yellow star. \ No newline at end of file diff --git a/en/star/hr7051.md b/en/star/hr7051.md new file mode 100644 index 000000000..e9dbcebe9 --- /dev/null +++ b/en/star/hr7051.md @@ -0,0 +1,9 @@ +--- +name: ε Lyrae +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 16:35:32.162138 +updated_by: editor.cs +updated_date: 2023-11-05 16:35:32.162142 +--- +"Double double", a multiple system near Vega, in which we can distinguish two components with the naked eye. In a telescope, these components are clearly distinguishable, with magnitudes of 5.1 and 5.4 at a separation of 208". When observed with a telescope of at least 60mm aperture and higher magnification, they split into double stars (companions ε1 with magnitude 6.5 and ε2 with magnitude 5.3). The mutual separation of one pair is 2.6", and the other pair is 2.3", with orbital periods determined to be 1,166 and 585 years. They are located at distances of 162 light-years and 156 light-years. \ No newline at end of file diff --git a/en/star/hr707.md b/en/star/hr707.md new file mode 100644 index 000000000..dd147931d --- /dev/null +++ b/en/star/hr707.md @@ -0,0 +1,9 @@ +--- +name: ι Cas +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 18:11:59.090121 +updated_by: editor.cs +updated_date: 2023-11-05 18:11:59.090125 +--- +one of the most beautiful triple stars in the sky. The main, white star with a brightness of 4.7mag is accompanied by a yellow and blue component. At a distance of 2.3", there is the first companion with a brightness of 7mag. At a separation of 7.2", there is a second component associated with this system, with a brightness of 8.4mag. The components of the main AB pair orbit each other every 840 years. \ No newline at end of file diff --git a/en/star/hr7106.md b/en/star/hr7106.md new file mode 100644 index 000000000..dc1980ded --- /dev/null +++ b/en/star/hr7106.md @@ -0,0 +1,9 @@ +--- +name: Sheliak (β Lyr) +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 17:52:04.224743 +updated_by: editor.cs +updated_date: 2023-11-05 17:52:04.224747 +--- +It is a representative of eclipsing variable stars of the beta Lyrae type. Both stars orbiting each other have the shape of a rotational ellipsoid. The star changes its brightness from 3.4mag to 4.4mag in a period of 12.908 days. Within the period, there is also a secondary minimum, during which the brightness decreases by 0.4mag. Suitable comparison stars are γ (3.25mag) and κ LYR (4.33mag). \ No newline at end of file diff --git a/en/star/hr7107.md b/en/star/hr7107.md new file mode 100644 index 000000000..02b60a66e --- /dev/null +++ b/en/star/hr7107.md @@ -0,0 +1,9 @@ +--- +name: κ Pav +constellation: Pav +created_by: editor.cs +created_date: 2023-11-05 17:57:10.951661 +updated_by: editor.cs +updated_date: 2023-11-05 17:57:10.951665 +--- +Short-period variable Cepheids belonging to the subtype known as W Virginis stars from the old population II. Its brightness ranges from 3.9mag to 4.8mag with a period of 9 days and 2 hours. This yellow-white supergiant is located 540 light-years away. \ No newline at end of file diff --git a/en/star/hr7139.md b/en/star/hr7139.md new file mode 100644 index 000000000..1e1f7fba7 --- /dev/null +++ b/en/star/hr7139.md @@ -0,0 +1,9 @@ +--- +name: δ Lyr +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 17:15:20.503974 +updated_by: editor.cs +updated_date: 2023-11-05 17:15:20.503978 +--- +Easily observable optical double star with a separation of 620", one component of which is distinctly reddish (with slightly variable brightness ranging from 4.3m to 4.4mag) and the other is pale blue (5.5mag). They can be resolved with a hand lens. \ No newline at end of file diff --git a/en/star/hr7141.md b/en/star/hr7141.md new file mode 100644 index 000000000..5a82df6c6 --- /dev/null +++ b/en/star/hr7141.md @@ -0,0 +1,9 @@ +--- +name: Alya (θ Ser) +constellation: Ser +created_by: editor.cs +created_date: 2023-11-05 16:30:48.320590 +updated_by: editor.cs +updated_date: 2023-11-05 16:30:48.320594 +--- +Double star on the eastern edge of the constellation. The pair of blue-white stars with magnitudes 4.6 and 5.1 are separated by 22.3", so a regular telescope is sufficient for their resolution. Both belong to the spectral class A5 and are physically related. They are located at a distance of 86 light-years. \ No newline at end of file diff --git a/en/star/hr7152.md b/en/star/hr7152.md new file mode 100644 index 000000000..8b50fe548 --- /dev/null +++ b/en/star/hr7152.md @@ -0,0 +1,9 @@ +--- +name: ε CrA +constellation: CrA +created_by: editor.cs +created_date: 2023-11-05 15:41:15.634870 +updated_by: editor.cs +updated_date: 2023-11-05 15:41:15.634875 +--- +An eclipsing variable star with a period of 14 hours. Since it is located on the northern edge of the constellation, it can be seen here as well, at least from areas at higher altitudes and without light pollution. \ No newline at end of file diff --git a/en/star/hr7157.md b/en/star/hr7157.md new file mode 100644 index 000000000..469ae79a5 --- /dev/null +++ b/en/star/hr7157.md @@ -0,0 +1,9 @@ +--- +name: R Lyrae +constellation: Lyr +created_by: editor.cs +created_date: 2023-11-05 17:53:55.082658 +updated_by: editor.cs +updated_date: 2023-11-05 17:53:55.082662 +--- +The conspicuously reddish-orange star visible to the naked eye is a semi-regular variable star, whose brightness varies in the range from 3.8mag to 5mag approximately every 46 days. \ No newline at end of file diff --git a/en/star/hr7243.md b/en/star/hr7243.md new file mode 100644 index 000000000..40e7c6f6b --- /dev/null +++ b/en/star/hr7243.md @@ -0,0 +1,9 @@ +--- +name: R Aquilae +constellation: Aql +created_by: editor.cs +created_date: 2023-11-05 15:01:25.896890 +updated_by: editor.cs +updated_date: 2023-11-05 15:01:25.896893 +--- +A variable star of the Mira type, located in the Milky Way, 5.5 degrees south of the star ζ Aquilae. Since the beginning of the 20th century, the period of brightness changes of this red giant has shortened by about 66 days. At the beginning of the 20th century, the period lasted approximately 350 days. Currently, the brightness changes from 5.5mag to 11.5mag in 284 days. \ No newline at end of file diff --git a/en/star/hr7296.md b/en/star/hr7296.md new file mode 100644 index 000000000..87fadac0d --- /dev/null +++ b/en/star/hr7296.md @@ -0,0 +1,9 @@ +--- +name: RY Sgr +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 17:13:29.496865 +updated_by: editor.cs +updated_date: 2023-11-05 17:13:29.496868 +--- +The equivalent of R Coronae Borealis, because it suddenly and unexpectedly changes its brightness from the eighth to the fourteenth magnitude. It does not have any precise period, and after R Coronae Borealis itself, it is the brightest star of this type. Its brightness unexpectedly decreases when carbon soot accumulates in the atmosphere. \ No newline at end of file diff --git a/en/star/hr7326.md b/en/star/hr7326.md new file mode 100644 index 000000000..a2a9af668 --- /dev/null +++ b/en/star/hr7326.md @@ -0,0 +1,9 @@ +--- +name: U Sge +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 15:15:28.307310 +updated_by: editor.cs +updated_date: 2023-11-05 15:15:28.307314 +--- +In a period of 3.38 days, the brightness of this eclipsing variable star of Algol type changes from 6.6 mag to 9.2 mag. It is suitable for observation even with a small telescope, as the changes near the beginning and end of the minimum can be observed within a few minutes. The eclipse, which occurs approximately once every three and a half days, lasts for approximately one hour and forty minutes. The primary component is a blue main sequence star, while the larger but fainter companion is a yellow giant. \ No newline at end of file diff --git a/en/star/hr7337.md b/en/star/hr7337.md new file mode 100644 index 000000000..b02bff0e9 --- /dev/null +++ b/en/star/hr7337.md @@ -0,0 +1,9 @@ +--- +name: Arkab (β Sgr) +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 17:45:07.560439 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:07.560443 +--- +Wide optical double star suitable for observation with a refractor. The primary component has a magnitude of 3.9, and additionally, there is a companion of magnitude 8 located at a distance of 28.4". \ No newline at end of file diff --git a/en/star/hr7417.md b/en/star/hr7417.md new file mode 100644 index 000000000..a176d4d7c --- /dev/null +++ b/en/star/hr7417.md @@ -0,0 +1,9 @@ +--- +name: Albireo (β Cygni) +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 17:49:07.377067 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:07.377072 +--- +It forms the head of the Swan or the bottom of the Cross and is one of the most beautiful contrasting double stars. Because it is not possible to directly observe the weaker star orbiting the brighter one, it cannot be said with certainty that it is a physical double star. The system is approximately 400 light-years away. The primary component is 950 times and the secondary component is 230 times brighter than the Sun. \ No newline at end of file diff --git a/en/star/hr7476.md b/en/star/hr7476.md new file mode 100644 index 000000000..fc6f88ad9 --- /dev/null +++ b/en/star/hr7476.md @@ -0,0 +1,9 @@ +--- +name: 54 Sgr +constellation: Sgr +created_by: editor.cs +created_date: 2023-11-05 16:48:38.373197 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:38.373201 +--- +The beautiful triple star is easily distinguishable in small telescopes. The brightest component is dark yellow (5.4 mag), the second one is pale blue (11.9 mag), and the third one is yellowish (8.9 mag). The separation of the AB pair is 38", and the separation of the AC components is 45.6". \ No newline at end of file diff --git a/en/star/hr7479.md b/en/star/hr7479.md new file mode 100644 index 000000000..9579f023d --- /dev/null +++ b/en/star/hr7479.md @@ -0,0 +1,9 @@ +--- +name: Sham (α Sge) +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 15:42:10.136979 +updated_by: editor.cs +updated_date: 2023-11-05 15:42:10.136983 +--- +The name, introduced about 200 years ago by Giuseppe Piazzi, an Italian astronomer who discovered the first asteroid Ceres, is based on the ancient Arabic name Sahm - arrow. This yellow giant of spectral class G0 has a brightness of 4.4mag and is located 382ly away. It has four faint companions. \ No newline at end of file diff --git a/en/star/hr749.md b/en/star/hr749.md new file mode 100644 index 000000000..b41cb527f --- /dev/null +++ b/en/star/hr749.md @@ -0,0 +1,9 @@ +--- +name: ω For +constellation: For +created_by: editor.cs +created_date: 2023-11-05 17:29:31.699815 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:31.699819 +--- +A double star distinguishable with a 50mm telescope. The primary white component has a brightness of 4.9mag, the blue companion of 7.7mag is located at a distance of 10.8". \ No newline at end of file diff --git a/en/star/hr7528.md b/en/star/hr7528.md new file mode 100644 index 000000000..506943d56 --- /dev/null +++ b/en/star/hr7528.md @@ -0,0 +1,9 @@ +--- +name: δ Cygni +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 17:51:32.837916 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:32.837921 +--- +Binary star, with component magnitudes reaching values of 2.9 and 6.3, their separation is 2.4" and the distance from Earth is 124 light-years. It is a good test for a 10-15 cm telescope. The primary component is reported by observers as white, pale blue, or even blue-green, while the secondary appears pale blue to blue. \ No newline at end of file diff --git a/en/star/hr7544.md b/en/star/hr7544.md new file mode 100644 index 000000000..53323d2fb --- /dev/null +++ b/en/star/hr7544.md @@ -0,0 +1,9 @@ +--- +name: π Aquilae +constellation: Aql +created_by: editor.cs +created_date: 2023-11-05 15:42:05.385814 +updated_by: editor.cs +updated_date: 2023-11-05 15:42:05.385817 +--- +A pair of beautiful yellow stars (6.1mag and 6.9mag) with a separation of 1.4" can already be seen with a 10 cm telescope. Although at 150x magnification they are still in contact with each other. \ No newline at end of file diff --git a/en/star/hr7546.md b/en/star/hr7546.md new file mode 100644 index 000000000..d9258c5a6 --- /dev/null +++ b/en/star/hr7546.md @@ -0,0 +1,9 @@ +--- +name: ζ Sge +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 15:39:46.184575 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:46.184579 +--- +The main star with a brightness of 5.5 mag has a companion with a separation of 8.6". In smaller telescopes, they appear as a closely separated pair of unequal brightness. The main star is a physical binary, indistinguishable with amateur telescopes - it appears as a bright yellow, while the companion is blue. The system is located at a distance of 260 light-years. At a separation of 76", there is a fourth star with a magnitude of 11 mag in the sky. \ No newline at end of file diff --git a/en/star/hr7557.md b/en/star/hr7557.md new file mode 100644 index 000000000..f818e51f9 --- /dev/null +++ b/en/star/hr7557.md @@ -0,0 +1,9 @@ +--- +name: Altair (α Aquilae) +constellation: Aql +created_by: editor.cs +created_date: 2023-11-05 16:31:42.835136 +updated_by: editor.cs +updated_date: 2023-11-05 16:31:42.835139 +--- +one of the closest bright stars visible to the naked eye. It has a magnitude of 0.77 and is approximately 16.5 light-years away from us. It is only 11 times brighter and has a diameter one and a half times larger than our Sun. Altair is also an optical double star, with a companion of magnitude 10 located at a distance of 165 arcseconds, still visible with an 8 cm telescope. \ No newline at end of file diff --git a/en/star/hr7564.md b/en/star/hr7564.md new file mode 100644 index 000000000..60c06714b --- /dev/null +++ b/en/star/hr7564.md @@ -0,0 +1,9 @@ +--- +name: χ Cygni +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 16:49:52.495979 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:52.495982 +--- +At its maximum of 3rd to 5th magnitude, this long-period variable star is located in the southwest part of the constellation visible to the naked eye, while in 6 to 7 months or up to 406 days it reaches a minimum around 13th to 14th magnitude. After the Mira Ceti itself, it is the brightest star of this type. A suitable comparison star is η Cygni (3.89 mag). \ No newline at end of file diff --git a/en/star/hr7570.md b/en/star/hr7570.md new file mode 100644 index 000000000..c5911e23f --- /dev/null +++ b/en/star/hr7570.md @@ -0,0 +1,9 @@ +--- +name: η Aquilae +constellation: Aql +created_by: editor.cs +created_date: 2023-11-05 17:16:46.497610 +updated_by: editor.cs +updated_date: 2023-11-05 17:16:46.497614 +--- +The brightest Cepheid on the sky, located 1,000 light-years away, lies 8 degrees south of Altair. The changes in brightness of this giant star can be easily observed with the naked eye. Its brightness fluctuates regularly between 3.7 mag and 4.4 mag over a period of 7 days and 4 hours. It is advisable to compare the changes in its brightness with the stars θ, δ (3 mag), and λ (4 mag). \ No newline at end of file diff --git a/en/star/hr758.md b/en/star/hr758.md new file mode 100644 index 000000000..5b4717083 --- /dev/null +++ b/en/star/hr758.md @@ -0,0 +1,9 @@ +--- +name: R Trianguli +constellation: Tri +created_by: editor.cs +created_date: 2023-11-05 15:03:30.068335 +updated_by: editor.cs +updated_date: 2023-11-05 15:03:30.068339 +--- +The variable star of Mira Ceti type with a magnitude fluctuation from 5.7 to 12.6 with a period of 267 days. \ No newline at end of file diff --git a/en/star/hr7635.md b/en/star/hr7635.md new file mode 100644 index 000000000..f90fa67aa --- /dev/null +++ b/en/star/hr7635.md @@ -0,0 +1,9 @@ +--- +name: γ Sge +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 16:49:36.525346 +updated_by: editor.cs +updated_date: 2023-11-05 16:49:36.525350 +--- +The brightest star of the constellation has an apparent magnitude of 3.71. It is an orange giant of spectral class K5, shining from a distance of approximately 258 light-years. \ No newline at end of file diff --git a/en/star/hr7705.md b/en/star/hr7705.md new file mode 100644 index 000000000..9e71569cc --- /dev/null +++ b/en/star/hr7705.md @@ -0,0 +1,9 @@ +--- +name: θ Sge +constellation: Sge +created_by: editor.cs +created_date: 2023-11-05 15:39:07.223523 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:07.223528 +--- +The asterism is observed along the southwest boundary of the inconspicuous open star cluster NGC 6873, which is located in the same field of view in a larger telescope. In a 100 mm telescope, the components AB appear pale yellow (6.5 mag), and at a separation of 84", there is also a third, orange star of magnitude 9. \ No newline at end of file diff --git a/en/star/hr7754.md b/en/star/hr7754.md new file mode 100644 index 000000000..575d54440 --- /dev/null +++ b/en/star/hr7754.md @@ -0,0 +1,9 @@ +--- +name: Prima Giedy (α1 Cap) +constellation: Cap +created_by: editor.cs +created_date: 2023-11-05 17:18:16.209637 +updated_by: editor.cs +updated_date: 2023-11-05 17:18:16.209641 +--- +The brightness of 4.2 mag, together with α2 (Secunda Giedo - 3.6 mag), forms an optical double star that can be distinguished with the naked eye under favorable conditions, in the northwest corner of the "triangular" constellation. The components are separated by 378 arcseconds, which corresponds to about 1/5 of the diameter of the full Moon. Prima Giedo is a giant star located 117 light-years away, while the supergiant Secunda Giedo is closer, at a distance of about 102 light-years. However, they form a beautiful pair of two orange-yellow stars in the sky. \ No newline at end of file diff --git a/en/star/hr7790.md b/en/star/hr7790.md new file mode 100644 index 000000000..a8d920287 --- /dev/null +++ b/en/star/hr7790.md @@ -0,0 +1,9 @@ +--- +name: Peacock (α Pavi) +constellation: Pav +created_by: editor.cs +created_date: 2023-11-05 16:42:14.809035 +updated_by: editor.cs +updated_date: 2023-11-05 16:42:14.809039 +--- +The brightest star of the constellation has an apparent magnitude of 1.9. In reality, it consists of two close components separated by 250 light-years. The star serves mainly as a reference point in a relatively poor area of stars. In a telescope, we can reveal two companions with magnitudes of 9 and 10.3. Peacock is a star of spectral class B2 with a diameter 2.5 times larger than the Sun. It shines 1000 times brighter than our Sun from a distance of 183 light-years. \ No newline at end of file diff --git a/en/star/hr7796.md b/en/star/hr7796.md new file mode 100644 index 000000000..dfd8123d8 --- /dev/null +++ b/en/star/hr7796.md @@ -0,0 +1,9 @@ +--- +name: Sadr (γ Cygni) +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 15:47:23.717268 +updated_by: editor.cs +updated_date: 2023-11-05 15:47:23.717272 +--- +The star has a companion with a magnitude of 9.9 at a separation of 142" that can be seen using a telescope with a 6 cm diameter objective. It itself is also a close binary star. Its distance from Earth is estimated to be 1800 light-years, so its luminosity is therefore 33,000 times greater than that of the Sun. \ No newline at end of file diff --git a/en/star/hr7814.md b/en/star/hr7814.md new file mode 100644 index 000000000..a1713bd22 --- /dev/null +++ b/en/star/hr7814.md @@ -0,0 +1,9 @@ +--- +name: π Cap +constellation: Cap +created_by: editor.cs +created_date: 2023-11-05 17:42:50.783225 +updated_by: editor.cs +updated_date: 2023-11-05 17:42:50.783228 +--- +A binary star consisting of two components with magnitudes of 5.3 and 8.9, separated by 3.2". To resolve them, we will need a telescope with a minimum objective diameter of 10 cm and an eyepiece with a shorter focal length. Even with a 200 mm telescope and 200x magnification, they appear as a close pair of faint and blue components. \ No newline at end of file diff --git a/en/star/hr7869.md b/en/star/hr7869.md new file mode 100644 index 000000000..8ca035791 --- /dev/null +++ b/en/star/hr7869.md @@ -0,0 +1,9 @@ +--- +name: α Ind +constellation: Ind +created_by: editor.cs +created_date: 2023-11-05 16:24:48.087374 +updated_by: editor.cs +updated_date: 2023-11-05 16:24:48.087378 +--- +The brightest star of the constellation has an apparent magnitude of 3.21. It is located 100 light years away. \ No newline at end of file diff --git a/en/star/hr7924.md b/en/star/hr7924.md new file mode 100644 index 000000000..3a03fa004 --- /dev/null +++ b/en/star/hr7924.md @@ -0,0 +1,9 @@ +--- +name: Deneb (α Cygni) +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 16:11:40.285750 +updated_by: editor.cs +updated_date: 2023-11-05 16:11:40.285754 +--- +The brightest star of the constellation, which, together with Vega in Lyra to the west and Altair in Aquila to the south, forms the Summer Triangle. This bright blue-white supergiant (1.2 mag) is much farther away than other bright stars in our sky - it is located at a distance of 2600 light-years. In order for Deneb to be so bright from this distance, it must have a greater energy output than 60,000 Suns, making it one of the most luminous stars visible to the naked eye (for example, Vega is 25 light-years away from us and Altair is only 11 light-years away). Its mass is 19 times that of the Sun and its diameter is 203 times larger. The surface temperature reaches 8500K. \ No newline at end of file diff --git a/en/star/hr7948.md b/en/star/hr7948.md new file mode 100644 index 000000000..aa442cf32 --- /dev/null +++ b/en/star/hr7948.md @@ -0,0 +1,9 @@ +--- +name: γ1,2 Del +constellation: Del +created_by: editor.cs +created_date: 2023-11-05 16:44:11.258776 +updated_by: editor.cs +updated_date: 2023-11-05 16:44:11.258780 +--- +A physical binary star, whose components have apparent magnitudes of 4.3 (yellow) and 5.1 (greenish), are separated by 10" in the sky, so they can be resolved even in a 5 cm telescope. The companion may appear bluish in some eyepieces, which is due to the contrast with the yellow primary component. \ No newline at end of file diff --git a/en/star/hr7965.md b/en/star/hr7965.md new file mode 100644 index 000000000..778ffadc2 --- /dev/null +++ b/en/star/hr7965.md @@ -0,0 +1,9 @@ +--- +name: α Mic +constellation: Mic +created_by: editor.cs +created_date: 2023-11-05 17:29:44.183060 +updated_by: editor.cs +updated_date: 2023-11-05 17:29:44.183064 +--- +It is not the brightest star in the constellation. This object belongs to the G6 class, so we can expect its yellow color. Its brightness is 5mag and at a separation of 20.5", we can see gray-white companions of magnitude 10 in the telescope. It is located 380 light-years away. \ No newline at end of file diff --git a/en/star/hr8034.md b/en/star/hr8034.md new file mode 100644 index 000000000..ae3a743e2 --- /dev/null +++ b/en/star/hr8034.md @@ -0,0 +1,9 @@ +--- +name: ε Equ +constellation: Equ +created_by: editor.cs +created_date: 2023-11-05 16:00:15.161568 +updated_by: editor.cs +updated_date: 2023-11-05 16:00:15.161572 +--- +A binary star with a magnitude of 6mag at a separation of 0.8" and a true orbit of approximately 101.4 years. At low magnification, they merge into one bright yellow star, which nicely contrasts with a blue star of magnitude 7mag in the same field of view (10.7"). Even at 200x magnification in a 200mm telescope, the two main components appear as an elongated line. The brighter of these two components is actually a physical binary star with an orbital period of 100 years, but its components are too close together to be separated by a small telescope. \ No newline at end of file diff --git a/en/star/hr8039.md b/en/star/hr8039.md new file mode 100644 index 000000000..b40f44ae0 --- /dev/null +++ b/en/star/hr8039.md @@ -0,0 +1,9 @@ +--- +name: γ Mic +constellation: Mic +created_by: editor.cs +created_date: 2023-11-05 17:18:06.473032 +updated_by: editor.cs +updated_date: 2023-11-05 17:18:06.473036 +--- +The brightest star of the constellation. It has an apparent magnitude of only 4.71. It used to belong to the constellation Southern Fish as the star 1 Piscis Austrini. It is located 220 light-years away from the Sun. It is a yellow star of the G8 spectral class, which has a companion with a brightness of 13.7 mag at a distance of 26". \ No newline at end of file diff --git a/en/star/hr804.md b/en/star/hr804.md new file mode 100644 index 000000000..6fb134c5e --- /dev/null +++ b/en/star/hr804.md @@ -0,0 +1,9 @@ +--- +name: Kaffaljidhma (γ Cet) +constellation: Cet +created_by: editor.cs +created_date: 2023-11-05 16:14:06.045003 +updated_by: editor.cs +updated_date: 2023-11-05 16:14:06.045007 +--- +A beautiful close physical binary star, distinguishable in a 100 mm telescope, with a yellow component of magnitude 3.5 and a white component of magnitude 7.3. It is separated by 2.8". The mutual orbital period of this pair is estimated to be several millennia. In a 200 mm telescope, a red dwarf of magnitude 10 is added, which is also part of the system. It is separated by 14'. The entire system is located approximately 80 light-years away. \ No newline at end of file diff --git a/en/star/hr8085.md b/en/star/hr8085.md new file mode 100644 index 000000000..53458e625 --- /dev/null +++ b/en/star/hr8085.md @@ -0,0 +1,9 @@ +--- +name: 61 Cygni +constellation: Cyg +created_by: editor.cs +created_date: 2023-11-05 16:46:21.626691 +updated_by: editor.cs +updated_date: 2023-11-05 16:46:21.626695 +--- +The inconspicuous binary star, distinguishable even with a smaller telescope, is known for being the first one to have its trigonometric parallax measured in 1838 - the distance of this celestial object was determined by the German astronomer Friedrich Wilhelm Bessel (who mainly worked in astrometry - he accurately measured the positions of over 50,000 stars and based on the analysis of their irregular proper motions, he predicted the presence of their long-invisible companions for both Sirius and Procyon in 1844). \ No newline at end of file diff --git a/en/star/hr8131.md b/en/star/hr8131.md new file mode 100644 index 000000000..aa55c3909 --- /dev/null +++ b/en/star/hr8131.md @@ -0,0 +1,9 @@ +--- +name: Kitalpha (α Equ) +constellation: Equ +created_by: editor.cs +created_date: 2023-11-05 15:47:09.593277 +updated_by: editor.cs +updated_date: 2023-11-05 15:47:09.593281 +--- +It is the brightest star of the constellation, although it only reaches a magnitude of 3.92. The other stars of the constellation are already below 4th magnitude. Kitalpha is a yellow giant of spectral class G0, from which light has been traveling to us for 186 years. \ No newline at end of file diff --git a/en/star/hr8140.md b/en/star/hr8140.md new file mode 100644 index 000000000..a3b9067e9 --- /dev/null +++ b/en/star/hr8140.md @@ -0,0 +1,9 @@ +--- +name: θ Ind +constellation: Ind +created_by: editor.cs +created_date: 2023-11-05 15:43:59.065164 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:59.065167 +--- +relatively easily distinguishable double star for a small telescope. The primary component has a brightness of 4.7mag and its companion with a brightness of 7.1mag is located at a separation of 6 arcseconds. This system is located at a distance of 97 light years. \ No newline at end of file diff --git a/en/star/hr815.md b/en/star/hr815.md new file mode 100644 index 000000000..d6cffc1f1 --- /dev/null +++ b/en/star/hr815.md @@ -0,0 +1,9 @@ +--- +name: RZ Cassiopeiae +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 16:30:33.921026 +updated_by: editor.cs +updated_date: 2023-11-05 16:30:33.921030 +--- +Interesting eclipsing variable star. The period of brightness changes is 1.19 days, but the decrease in brightness from 6.18mag to 7.72mag lasts only two hours, while the brightening then occurs immediately and the star returns to its original magnitude in the next two hours. \ No newline at end of file diff --git a/en/star/hr8151.md b/en/star/hr8151.md new file mode 100644 index 000000000..a4adf7e9f --- /dev/null +++ b/en/star/hr8151.md @@ -0,0 +1,9 @@ +--- +name: θ Mic +constellation: Mic +created_by: editor.cs +created_date: 2023-11-05 16:38:39.746324 +updated_by: editor.cs +updated_date: 2023-11-05 16:38:39.746328 +--- +A triple star system consisting of a close pair of components with magnitudes 6.4 and 7, separated by a distance of 0.5", which is a good test for a 250mm telescope. Higher magnification and stable atmospheric conditions are necessary to see this close pair of yellow stars as at least two disks in contact. 78.4" away from this close pair, there is another star of magnitude 11. \ No newline at end of file diff --git a/en/star/hr8162.md b/en/star/hr8162.md new file mode 100644 index 000000000..2f101da97 --- /dev/null +++ b/en/star/hr8162.md @@ -0,0 +1,9 @@ +--- +name: Alderamin (α Cep) +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 17:14:49.395548 +updated_by: editor.cs +updated_date: 2023-11-05 17:14:49.395550 +--- +The brightest star of the constellation has a magnitude of 2.44. It is a yellow-white star of spectral class A7, located 49 light-years away from us, forming a quadrilateral with the stars β (magnitude 3.21), ζ (magnitude 3.35), and ι (magnitude 3.52). In its center lies the star ξ Cep. Due to the precession of the Earth's axis, Alderamin will become the closest star to the North Celestial Pole around the year 7500 AD. It has a luminosity 17 times greater than that of the Sun. \ No newline at end of file diff --git a/en/star/hr8238.md b/en/star/hr8238.md new file mode 100644 index 000000000..4815d6901 --- /dev/null +++ b/en/star/hr8238.md @@ -0,0 +1,9 @@ +--- +name: Alfirk (β Cep) +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 16:36:17.355201 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:17.355204 +--- +A double star distinguishable by a small telescope with a 6 cm diameter objective, consisting of two components with magnitudes 3.2 (bright white) and 7.9 (blue - appearing emerald green in a large telescope) at a mutual distance of 13.3". The primary star is also a spectroscopic binary, with an orbital period of only 4 and 3/4 hours. In the same period, it exhibits a slight change in brightness between magnitudes 3.3 and 3.4. It is even a prototype of a group of variable stars called beta Cepheids, whose brightness fluctuations are so small that they can hardly be observed with the naked eye. It is located at a distance of 690 light-years. \ No newline at end of file diff --git a/en/star/hr8254.md b/en/star/hr8254.md new file mode 100644 index 000000000..720934967 --- /dev/null +++ b/en/star/hr8254.md @@ -0,0 +1,9 @@ +--- +name: ν Oct +constellation: Oct +created_by: editor.cs +created_date: 2023-11-05 17:11:43.947129 +updated_by: editor.cs +updated_date: 2023-11-05 17:11:43.947134 +--- +The brightest star in the constellation has a magnitude of 3.74. It is an orange giant. \ No newline at end of file diff --git a/en/star/hr8280.md b/en/star/hr8280.md new file mode 100644 index 000000000..e2c9e8c3d --- /dev/null +++ b/en/star/hr8280.md @@ -0,0 +1,9 @@ +--- +name: λ Oct +constellation: Oct +created_by: editor.cs +created_date: 2023-11-05 15:59:48.364460 +updated_by: editor.cs +updated_date: 2023-11-05 15:59:48.364465 +--- +A binary star with brightness components of 5.5mag and 7.7mag, separated by 3 arc seconds, therefore we will need a telescope with an objective diameter of around 100 mm to resolve them. \ No newline at end of file diff --git a/en/star/hr8308.md b/en/star/hr8308.md new file mode 100644 index 000000000..8c4727656 --- /dev/null +++ b/en/star/hr8308.md @@ -0,0 +1,9 @@ +--- +name: Enif (ε Peg) +constellation: Peg +created_by: editor.cs +created_date: 2023-11-05 17:51:06.261082 +updated_by: editor.cs +updated_date: 2023-11-05 17:51:06.261085 +--- +The brightest star of the constellation. In a small telescope, besides this orange giant of the second magnitude, a companion of 9th magnitude appears. In a large telescope, a companion of 11.3 magnitude is also added. Astronomers believed that Enif is a variable star, but this has not yet been definitively confirmed. It is located 690 light-years away. \ No newline at end of file diff --git a/en/star/hr8316.md b/en/star/hr8316.md new file mode 100644 index 000000000..1094588fa --- /dev/null +++ b/en/star/hr8316.md @@ -0,0 +1,9 @@ +--- +name: Erakis (μ Cep) +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 15:39:16.343327 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:16.343331 +--- +The star, due to its striking dark red color, was named "Granátová hvězda" (Garnet Star) by William Herschel - it belongs to the reddest stars in the entire sky, which is easily verifiable even to the unaided human eye. Even in a small telescope, it provides a nice view. Gradually, when observed with a larger telescope, it can take on an orange-red or orange-yellow hue. It has a surface temperature of only 3,500 K, while its diameter is 70 times larger than that of the Sun. This M-type spectrum star is actually much brighter in comparison to another known red supergiant - Betelgeuse in Orion, it is at least as bright as 174,000 Suns and has an absolute magnitude of -8.3. We perceive it as a faint star in the sky only because of its large distance of 2,800 light-years. \ No newline at end of file diff --git a/en/star/hr8322.md b/en/star/hr8322.md new file mode 100644 index 000000000..b35519241 --- /dev/null +++ b/en/star/hr8322.md @@ -0,0 +1,9 @@ +--- +name: Deneb Algedi (δ Cap) +constellation: Cap +created_by: editor.cs +created_date: 2023-11-05 16:45:47.789573 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:47.789581 +--- +The brightest star of the constellation. It is an eclipsing variable star of the Algol type, but its brightness varies only in the range of 2.9mag to 3.1mag, which is difficult to observe with the naked eye. It is located at a distance of 38 light-years. \ No newline at end of file diff --git a/en/star/hr834.md b/en/star/hr834.md new file mode 100644 index 000000000..f9d1578fc --- /dev/null +++ b/en/star/hr834.md @@ -0,0 +1,11 @@ +--- +name: Miram (η Per) +constellation: Per +created_by: editor.cs +created_date: 2023-11-05 17:00:55.244701 +updated_by: editor.cs +updated_date: 2023-11-05 17:00:55.244706 +--- +Astronomical text translation: + +A very easily distinguishable pair with magnitudes of 3.8 and 8.5 at a separation of 28.3". It resembles the well-known double star Albireo, as its components have a golden-blue contrast. 66" almost west of the main component, there is a close double star composed of components with magnitudes of 10mag and 10.5mag, which is likely part of the η Per system. A dozen fainter stars form a small star cluster around this system. \ No newline at end of file diff --git a/en/star/hr8353.md b/en/star/hr8353.md new file mode 100644 index 000000000..1375a6ca4 --- /dev/null +++ b/en/star/hr8353.md @@ -0,0 +1,9 @@ +--- +name: γ Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 16:46:49.013724 +updated_by: editor.cs +updated_date: 2023-11-05 16:46:49.013728 +--- +The blue giant is even brighter than the two previous stars. It is located 230 light-years away from us. Its visual magnitude in the sky is 3.2 mag. \ No newline at end of file diff --git a/en/star/hr8383.md b/en/star/hr8383.md new file mode 100644 index 000000000..25de63b05 --- /dev/null +++ b/en/star/hr8383.md @@ -0,0 +1,9 @@ +--- +name: VV Cephei +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 17:56:05.936475 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:05.936479 +--- +Red supergiant, component of an eclipsing variable star, which changes its apparent brightness from 4.9 mag to 5.7 mag over a period of 20 years. It was once considered the largest known star in the observed part of the universe. It has a diameter 2,400 times larger than the Sun, with an average density only one three-millionth of the density of water. Its distance from Earth is 5,000 light-years. \ No newline at end of file diff --git a/en/star/hr8386.md b/en/star/hr8386.md new file mode 100644 index 000000000..bde46579d --- /dev/null +++ b/en/star/hr8386.md @@ -0,0 +1,9 @@ +--- +name: η PsA +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 15:27:33.531360 +updated_by: editor.cs +updated_date: 2023-11-05 15:27:33.531365 +--- +In a 200 mm telescope, this binary system appears as two blue-white disks almost in contact. The components have magnitudes of 5.8 and 6.8 and are separated by 1.7". \ No newline at end of file diff --git a/en/star/hr8387.md b/en/star/hr8387.md new file mode 100644 index 000000000..22592bcb5 --- /dev/null +++ b/en/star/hr8387.md @@ -0,0 +1,9 @@ +--- +name: ε Ind +constellation: Ind +created_by: editor.cs +created_date: 2023-11-05 15:14:49.751362 +updated_by: editor.cs +updated_date: 2023-11-05 15:14:49.751366 +--- +One of our closest stars, located just 11.3 light-years away. This yellow dwarf of fifth magnitude is somewhat similar to the Sun. Its diameter reaches 4/5 of the solar diameter and its luminosity is 1/8 of the Sun's luminosity. It is the least luminous star visible to the naked eye. It has a fast proper motion and moves 4.7" across the sky in a year. By the year 2640, it will be part of a different constellation - Tucana. \ No newline at end of file diff --git a/en/star/hr8417.md b/en/star/hr8417.md new file mode 100644 index 000000000..8d0aa5bc4 --- /dev/null +++ b/en/star/hr8417.md @@ -0,0 +1,9 @@ +--- +name: Al Kurhah (ξ Cep) +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 17:17:41.932231 +updated_by: editor.cs +updated_date: 2023-11-05 17:17:41.932236 +--- +This physical binary star consists of two components with magnitudes of 4.6 (white) and 6.5 (yellow-brown) at a separation of 8", which can be resolved by a telescope with an objective diameter larger than 6 cm under ideal conditions. Their distance from Earth is determined to be 86 light-years. They are peripheral members of the "Taurus moving group" primarily associated with the open star cluster Hyades. \ No newline at end of file diff --git a/en/star/hr8425.md b/en/star/hr8425.md new file mode 100644 index 000000000..3802927f7 --- /dev/null +++ b/en/star/hr8425.md @@ -0,0 +1,9 @@ +--- +name: Alnair (α Gruis) +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 16:36:31.064390 +updated_by: editor.cs +updated_date: 2023-11-05 16:36:31.064393 +--- +The brightest star in the constellation with a visual magnitude of 1.7. Its name means "bright star". It is a blue-white main sequence star 70 times more luminous than the Sun, located 60 light-years away. Among the trio of the brightest stars in the constellation, it is the closest to us. At an angular distance of 28.4", there is a faint companion with a magnitude of 11.8. \ No newline at end of file diff --git a/en/star/hr8480.md b/en/star/hr8480.md new file mode 100644 index 000000000..7e8dd89db --- /dev/null +++ b/en/star/hr8480.md @@ -0,0 +1,9 @@ +--- +name: 41 Aqr +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 17:53:03.122679 +updated_by: editor.cs +updated_date: 2023-11-05 17:53:03.122683 +--- +A binary star composed of two components with the same brightness of 7.1 mag at a separation of 5". In the field of view of a telescope with an objective diameter of around 20 cm, it appears as a tight, equally bright pair of golden and blue components. \ No newline at end of file diff --git a/en/star/hr8486.md b/en/star/hr8486.md new file mode 100644 index 000000000..fa55efd7f --- /dev/null +++ b/en/star/hr8486.md @@ -0,0 +1,9 @@ +--- +name: μ Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 17:00:42.383739 +updated_by: editor.cs +updated_date: 2023-11-05 17:00:42.383742 +--- +Wide optical double star distinguishable with the naked eye. It consists of yellow giants with magnitudes of 4.8 and 5.1, located at a distance of 260 and 240 light years. \ No newline at end of file diff --git a/en/star/hr8502.md b/en/star/hr8502.md new file mode 100644 index 000000000..0ca7c17db --- /dev/null +++ b/en/star/hr8502.md @@ -0,0 +1,9 @@ +--- +name: α Tuc +constellation: Tuc +created_by: editor.cs +created_date: 2023-11-05 17:49:44.410097 +updated_by: editor.cs +updated_date: 2023-11-05 17:49:44.410100 +--- +The brightest star of the constellation has an apparent magnitude of 2.91 and an orange hue. It is located 62 light-years away from Earth. \ No newline at end of file diff --git a/en/star/hr8540.md b/en/star/hr8540.md new file mode 100644 index 000000000..44d42b741 --- /dev/null +++ b/en/star/hr8540.md @@ -0,0 +1,9 @@ +--- +name: δ Tuc +constellation: Tuc +created_by: editor.cs +created_date: 2023-11-05 15:59:28.484897 +updated_by: editor.cs +updated_date: 2023-11-05 15:59:28.484901 +--- +An easily distinguishable double star. The primary component has a brightness of 4.8 magnitude and is separated by 7 arcseconds from a companion with a brightness of 9 magnitude, which can be separated by at least a 100 mm telescope. \ No newline at end of file diff --git a/en/star/hr8545.md b/en/star/hr8545.md new file mode 100644 index 000000000..bc88ea357 --- /dev/null +++ b/en/star/hr8545.md @@ -0,0 +1,9 @@ +--- +name: 53 Aqr +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 16:29:03.218638 +updated_by: editor.cs +updated_date: 2023-11-05 16:29:03.218642 +--- +Multiple star. In a 200 mm telescope, a close pair (3.1") of two yellow stars (6.4mag, 6.6mag), which are not related at all - they are just an optical double star. Nearby, two fainter stars are also visible, with magnitudes of 12.9mag and 13.9mag. \ No newline at end of file diff --git a/en/star/hr8556.md b/en/star/hr8556.md new file mode 100644 index 000000000..862ecc7cc --- /dev/null +++ b/en/star/hr8556.md @@ -0,0 +1,25 @@ +--- +name: δ Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 15:43:30.073367 +updated_by: editor.cs +updated_date: 2023-11-05 15:43:30.073371 +--- +Astronomický text: + +A naked-eye distinguishable optical double star. The separation between the yellow 4mag and the red giant 4.1mag is 12 arcminutes. Both components are also doubled. In the first one, we can distinguish a companion with a brightness of 12.8mag at a distance of 5.6". + +Překlad českých zkratek světových stran do angličtiny: + +S - South +Z - West +J - East +E - North + +Překlad anglických zkratek světových stran do češtiny: + +N - Sever (North) +W - Západ (West) +S - Jih (South) +E - Východ (East) \ No newline at end of file diff --git a/en/star/hr8559.md b/en/star/hr8559.md new file mode 100644 index 000000000..178f304e4 --- /dev/null +++ b/en/star/hr8559.md @@ -0,0 +1,9 @@ +--- +name: Dzeta Aquarii (ζ Aqr) +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 16:48:07.865677 +updated_by: editor.cs +updated_date: 2023-11-05 16:48:07.865682 +--- +The well-known binary star in the Aquarius constellation. The two almost equally bright components with magnitudes of 4.3 and 4.5 have a period of mutual orbit determined to be 856 years. In 1967, the stars were only 1.7" apart, but since then their separation has slowly increased. In 1985, it was 1.8", but at the beginning of the third millennium, we perceive them as a yellow to white pair, approximately two arc seconds wide, easily distinguishable even with a small telescope with a 5cm objective diameter. In the year 2160, their separation will increase to 6". The system is located 92 light-years away. \ No newline at end of file diff --git a/en/star/hr8571.md b/en/star/hr8571.md new file mode 100644 index 000000000..5e39f0462 --- /dev/null +++ b/en/star/hr8571.md @@ -0,0 +1,9 @@ +--- +name: δ Cephei +constellation: Cep +created_by: editor.cs +created_date: 2023-11-05 17:30:11.587332 +updated_by: editor.cs +updated_date: 2023-11-05 17:30:11.587337 +--- +Together with the stars ε (4.19mag) and ζ Cep (3.35mag), it forms a small triangle. While these two stars are constant, δ Cephei changes its brightness regularly due to pulsation. The entire group of variable stars - delta Cepheids - is named after this star. The variability of δ Cephei was discovered in 1784 by the twenty-year-old John Goodrick, a deaf-mute English amateur astronomer of Dutch origin (he discovered three variable stars, thoroughly studied the brightness changes of the star Algol, and correctly explained them at the age of 19, two years later he died at the age of 21). In its brightest form, the star reaches a magnitude of 3.48, while in its minimum it has a brightness of 4.37mag, so these changes can be easily observed with the naked eye. Its period is 5.37 days. Astronomers use Cepheids to estimate distances in the universe. \ No newline at end of file diff --git a/en/star/hr8576.md b/en/star/hr8576.md new file mode 100644 index 000000000..db0ef7621 --- /dev/null +++ b/en/star/hr8576.md @@ -0,0 +1,9 @@ +--- +name: Fum al Samakah (β PsA) +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 16:46:16.635716 +updated_by: editor.cs +updated_date: 2023-11-05 16:46:16.635719 +--- +Optical double star distinguishable with a good refractor. The primary white component of this pair has a brightness of 4.4mag and the blue companion at a separation of 30.3" reaches a magnitude of 7.9mag. \ No newline at end of file diff --git a/en/star/hr86.md b/en/star/hr86.md new file mode 100644 index 000000000..d6c48b6b9 --- /dev/null +++ b/en/star/hr86.md @@ -0,0 +1,9 @@ +--- +name: 42 Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 18:12:23.666438 +updated_by: editor.cs +updated_date: 2023-11-05 18:12:23.666441 +--- +This binary star can be easily distinguished with a telescope with a 100 mm objective diameter. It consists of an orange primary component with a brightness of 6.2 magnitude and a companion located 28.5" away with a magnitude of 10. \ No newline at end of file diff --git a/en/star/hr8603.md b/en/star/hr8603.md new file mode 100644 index 000000000..1521d25ee --- /dev/null +++ b/en/star/hr8603.md @@ -0,0 +1,9 @@ +--- +name: 8 Lac +constellation: Lac +created_by: editor.cs +created_date: 2023-11-05 16:33:21.385446 +updated_by: editor.cs +updated_date: 2023-11-05 16:33:21.385452 +--- +Struve 2922 has so many companions that it could be classified as a poor open star cluster rather than just a multiple star. Four close companions, all white or pale blue components, lie within 82" of the primary star. Another one lies 336" WSW. There are also stars of magnitude 13-14 in the area. A minimum of a 200mm telescope is required for sufficient enjoyment of the view. \ No newline at end of file diff --git a/en/star/hr8628.md b/en/star/hr8628.md new file mode 100644 index 000000000..7c2063075 --- /dev/null +++ b/en/star/hr8628.md @@ -0,0 +1,9 @@ +--- +name: ε PsA +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 15:44:25.874918 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:25.874922 +--- +The companions have a brightness of 5.5mag and 6.5mag, with a separation of 1.6". We need a telescope with an objective diameter above 100 mm. \ No newline at end of file diff --git a/en/star/hr8636.md b/en/star/hr8636.md new file mode 100644 index 000000000..b39679f40 --- /dev/null +++ b/en/star/hr8636.md @@ -0,0 +1,9 @@ +--- +name: β Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 17:45:11.761761 +updated_by: editor.cs +updated_date: 2023-11-05 17:45:11.761764 +--- +The red giant irregularly varies in brightness from 2mag to 2.3mag. Its luminosity is approximately 800 times that of the Sun. It is located 200 light years away. In the eyepiece, it nicely contrasts with the blue-white star Alnair. \ No newline at end of file diff --git a/en/star/hr8650.md b/en/star/hr8650.md new file mode 100644 index 000000000..843b040da --- /dev/null +++ b/en/star/hr8650.md @@ -0,0 +1,9 @@ +--- +name: Matar (η Peg) +constellation: Peg +created_by: editor.cs +created_date: 2023-11-05 17:43:29.304894 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:29.304898 +--- +The main yellow component has a magnitude of 2.94 and is separated by 90.4" from a blue companion with a magnitude of 9.9. The blue companion is still a close binary, but the AB pair can be easily resolved in a telescope. The system is located 167 light-years away. \ No newline at end of file diff --git a/en/star/hr8695.md b/en/star/hr8695.md new file mode 100644 index 000000000..4ef0f16fe --- /dev/null +++ b/en/star/hr8695.md @@ -0,0 +1,9 @@ +--- +name: γ PsA +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 15:28:45.094415 +updated_by: editor.cs +updated_date: 2023-11-05 15:28:45.094419 +--- +Stars with magnitudes 4.5 and 8.1 have a separation of 4.3". To resolve them, we need a 100 mm telescope, mainly due to the difference in brightness of both components. They are located at a distance of 215 light-years. \ No newline at end of file diff --git a/en/star/hr8728.md b/en/star/hr8728.md new file mode 100644 index 000000000..8b0491106 --- /dev/null +++ b/en/star/hr8728.md @@ -0,0 +1,9 @@ +--- +name: Fomalhaut (α PsA) +constellation: PsA +created_by: editor.cs +created_date: 2023-11-05 16:28:17.722570 +updated_by: editor.cs +updated_date: 2023-11-05 16:28:17.722574 +--- +It lies on the extended line connecting the stars Schema-Markab in the constellation Pegasus. With its brightness of 1.2 mag, the yellow-white Fomalhaut is only 25 light-years away and is among the 20 brightest stars in the sky. Compared to the Sun, it is more than twice the diameter and its luminosity exceeds our star by 16 times. \ No newline at end of file diff --git a/en/star/hr8775.md b/en/star/hr8775.md new file mode 100644 index 000000000..70dffab4b --- /dev/null +++ b/en/star/hr8775.md @@ -0,0 +1,9 @@ +--- +name: Scheat (β Peg) +constellation: Peg +created_by: editor.cs +created_date: 2023-11-05 16:41:14.088317 +updated_by: editor.cs +updated_date: 2023-11-05 16:41:14.088321 +--- +The red giant, whose brightness irregularly varies between 2.4mag and 2.6mag. This semi-regular variable star of spectral class M2 has a period of approximately 35 to 40 days. α and γ are suitable comparison stars. It is located 196 light-years away. \ No newline at end of file diff --git a/en/star/hr8787.md b/en/star/hr8787.md new file mode 100644 index 000000000..2f9316024 --- /dev/null +++ b/en/star/hr8787.md @@ -0,0 +1,9 @@ +--- +name: θ Gru +constellation: Gru +created_by: editor.cs +created_date: 2023-11-05 15:40:21.333066 +updated_by: editor.cs +updated_date: 2023-11-05 15:40:21.333071 +--- +A physical binary star, whose companions can be distinguished even in a small telescope at a separation of 14 arcseconds. They have magnitudes of 4.5 and 7. \ No newline at end of file diff --git a/en/star/hr8841.md b/en/star/hr8841.md new file mode 100644 index 000000000..28feabc15 --- /dev/null +++ b/en/star/hr8841.md @@ -0,0 +1,9 @@ +--- +name: ψ Aqr +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 16:41:56.027283 +updated_by: editor.cs +updated_date: 2023-11-05 16:41:56.027287 +--- +The main star with a brightness of 4.5 mag has a companion of 9.4 mag at a distance of 49". In a 10cm telescope, it appears as a wide, unevenly bright pair consisting of an orange and greenish component, resembling the planet Uranus. Very nice color contrast. \ No newline at end of file diff --git a/en/star/hr8866.md b/en/star/hr8866.md new file mode 100644 index 000000000..4923f3465 --- /dev/null +++ b/en/star/hr8866.md @@ -0,0 +1,9 @@ +--- +name: 94 Aqr +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 16:45:58.219741 +updated_by: editor.cs +updated_date: 2023-11-05 16:45:58.219744 +--- +An easily distinguishable and beautiful double star, composed of two components with magnitudes of 5.3 and 7.3, separated by 12.7", so even a small telescope is sufficient for resolution. One has a nice reddish-yellow hue and the other has a light green shade. \ No newline at end of file diff --git a/en/star/hr887.md b/en/star/hr887.md new file mode 100644 index 000000000..60f07e402 --- /dev/null +++ b/en/star/hr887.md @@ -0,0 +1,9 @@ +--- +name: ε Arietis +constellation: Ari +created_by: editor.cs +created_date: 2023-11-05 15:46:14.925792 +updated_by: editor.cs +updated_date: 2023-11-05 15:46:14.925796 +--- +Binary star, white components with nearly the same brightness (5.2 mag and 5.5 mag) at a separation of 1.5". We can sufficiently separate them with a magnification of 150x using a 200 mm telescope during good seeing. \ No newline at end of file diff --git a/en/star/hr897.md b/en/star/hr897.md new file mode 100644 index 000000000..0dfeb1e15 --- /dev/null +++ b/en/star/hr897.md @@ -0,0 +1,9 @@ +--- +name: Acamar (θ Eri) +constellation: Eri +created_by: editor.cs +created_date: 2023-11-05 16:37:00.432904 +updated_by: editor.cs +updated_date: 2023-11-05 16:37:00.432909 +--- +This star is believed to have weakened from 1st to 3rd magnitude in the historical period, although there is not enough evidence for it. However, it is a very beautiful binary star, with its white companions having a brightness of 3.4 mag and 4.5 mag, and they are 8.2" apart. To resolve this pair, a telescope with a 5 cm diameter objective is sufficient. However, due to its low declination, this system is very difficult to observe in our country. \ No newline at end of file diff --git a/en/star/hr8992.md b/en/star/hr8992.md new file mode 100644 index 000000000..7eed83298 --- /dev/null +++ b/en/star/hr8992.md @@ -0,0 +1,9 @@ +--- +name: R Aqr +constellation: Aqr +created_by: editor.cs +created_date: 2023-11-05 17:32:11.549356 +updated_by: editor.cs +updated_date: 2023-11-05 17:32:11.549359 +--- +Variable star, whose magnitude can sometimes reach a value of up to 5.8mag, although it is usually much fainter. It exhibits rapid, unpredictable fluctuations. \ No newline at end of file diff --git a/en/star/hr90.md b/en/star/hr90.md new file mode 100644 index 000000000..b3523eadc --- /dev/null +++ b/en/star/hr90.md @@ -0,0 +1,9 @@ +--- +name: R Andromedae +constellation: And +created_by: editor.cs +created_date: 2023-11-05 16:43:21.577246 +updated_by: editor.cs +updated_date: 2023-11-05 16:43:21.577251 +--- +The long-period variable star of Mira Ceti type, the brightest in this constellation. It is located near the small triangle of stars θ, σ, and ρ And. At its maximum brightness of 5.8 mag, it is on the edge of visibility to the naked eye, but over 409.33 days its brightness decreases to 14.9 mag (thus changing by 9 magnitudes) and with smaller amateur telescopes it is practically unobservable. The distance is not precisely determined, approximately 790 light-years. \ No newline at end of file diff --git a/en/star/hr9004.md b/en/star/hr9004.md new file mode 100644 index 000000000..ec17a48a1 --- /dev/null +++ b/en/star/hr9004.md @@ -0,0 +1,9 @@ +--- +name: TX Psc +constellation: Psc +created_by: editor.cs +created_date: 2023-11-05 15:01:45.299217 +updated_by: editor.cs +updated_date: 2023-11-05 15:01:45.299220 +--- +A very interesting irregular variable star, also known as 19 Piscium. The range of its magnitude is from 6.9 to 7.7 and it seems to have no hint of periodicity. TX Psc, with a spectral class of N, is one of the reddest stars within reach of a telescope. In the same field of view, there are ι Psc (4.1 mag) and λ Psc (4.5 mag). \ No newline at end of file diff --git a/en/star/hr9045.md b/en/star/hr9045.md new file mode 100644 index 000000000..f5eb73550 --- /dev/null +++ b/en/star/hr9045.md @@ -0,0 +1,9 @@ +--- +name: ρ Cas +constellation: Cas +created_by: editor.cs +created_date: 2023-11-05 14:50:27.665054 +updated_by: editor.cs +updated_date: 2023-11-05 14:50:27.665060 +--- +An irregular variable star, similar to R Coronae Borealis, its brightness varies between 4.1mag and 6.2mag in a cycle that lasts slightly less than one year. Suitable comparison stars are σ (4.9mag) and τ Cas (4.87mag). This exceptionally luminous supergiant is located 3400 light-years away. In the sky, we see it near the star β Cas. \ No newline at end of file diff --git a/en/star/hr911.md b/en/star/hr911.md new file mode 100644 index 000000000..5061a2262 --- /dev/null +++ b/en/star/hr911.md @@ -0,0 +1,9 @@ +--- +name: Menkar (α Cet) +constellation: Cet +created_by: editor.cs +created_date: 2023-11-05 15:16:49.087223 +updated_by: editor.cs +updated_date: 2023-11-05 15:16:49.087228 +--- +The orange field of apparent brightness 2.53mag is located 250 light-years away from us. At a distance of nearly 16', the star 93 Ceti (5.6mag) lies to the north, visible to the naked eye as an optical companion. \ No newline at end of file diff --git a/en/star/hr963.md b/en/star/hr963.md new file mode 100644 index 000000000..1484dee58 --- /dev/null +++ b/en/star/hr963.md @@ -0,0 +1,9 @@ +--- +name: α For +constellation: For +created_by: editor.cs +created_date: 2023-11-05 15:44:50.661614 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:50.661617 +--- +The main yellow star has a brightness of 3.9 mag and is located 40 light-years away from Earth. It is a binary star with an orbital period of 314 years. The yellow companion has a brightness of 7 mag. Around the year 2000, it could be resolved using a smaller telescope with a 6 cm objective diameter when it was at a separation of 5.1". By the year 2020, the separation will increase to 5.8". The system is located 46 light-years away from us. \ No newline at end of file diff --git a/en/star/hr98.md b/en/star/hr98.md new file mode 100644 index 000000000..4b3488073 --- /dev/null +++ b/en/star/hr98.md @@ -0,0 +1,9 @@ +--- +name: β Hyi +constellation: Hyi +created_by: editor.cs +created_date: 2023-11-05 14:50:06.238281 +updated_by: editor.cs +updated_date: 2023-11-05 14:50:06.238285 +--- +A star similar to our Sun of spectral class G shining from a distance of 22 light years. Its diameter is twice that of the Sun, surface temperature reaches 6,300 K, and its mass is 1.4 times that of our Sun. It is the brightest star in the constellation, with an apparent magnitude of 2.8. \ No newline at end of file diff --git a/en/star/hr99.md b/en/star/hr99.md new file mode 100644 index 000000000..a08921c2b --- /dev/null +++ b/en/star/hr99.md @@ -0,0 +1,9 @@ +--- +name: Ankaa (α Phe) +constellation: Phe +created_by: editor.cs +created_date: 2023-11-05 15:39:30.894835 +updated_by: editor.cs +updated_date: 2023-11-05 15:39:30.894840 +--- +The brightest star of the constellation. Its brightness reaches 2.3mag. It is distinctly orange and belongs to the spectral class KO. It is located on the northern edge of the constellation and for observers at 40 degrees north latitude, it culminates at a height of 8 degrees above the southern horizon. It is located at a distance of 77 light years. \ No newline at end of file diff --git a/en/star/x_Vel.md b/en/star/x_Vel.md new file mode 100644 index 000000000..7c1861be0 --- /dev/null +++ b/en/star/x_Vel.md @@ -0,0 +1,9 @@ +--- +name: x Vel +constellation: Vel +created_by: editor.cs +created_date: 2023-11-05 17:56:36.937509 +updated_by: editor.cs +updated_date: 2023-11-05 17:56:36.937514 +--- +A binary star, with components of 4.3 magnitude and 6.6 magnitude, can be resolved as a double star at a separation of 52". \ No newline at end of file diff --git a/en/star/ι_Tri.md b/en/star/ι_Tri.md new file mode 100644 index 000000000..2a1d12da1 --- /dev/null +++ b/en/star/ι_Tri.md @@ -0,0 +1,9 @@ +--- +name: ι Tri +constellation: Tri +created_by: editor.cs +created_date: 2023-11-05 15:59:32.761417 +updated_by: editor.cs +updated_date: 2023-11-05 15:59:32.761420 +--- +A binary star with components of brightness 5.3mag and 6.9mag is separated by 3.9". To resolve the yellow and blue stars, we need an 80mm telescope. \ No newline at end of file diff --git a/en/star/π1_UMi.md b/en/star/π1_UMi.md new file mode 100644 index 000000000..be89fe054 --- /dev/null +++ b/en/star/π1_UMi.md @@ -0,0 +1,9 @@ +--- +name: π1 UMi +constellation: UMi +created_by: editor.cs +created_date: 2023-11-05 15:44:19.163062 +updated_by: editor.cs +updated_date: 2023-11-05 15:44:19.163066 +--- +The binary star, with the primary component being yellow (6.6 mag) and the companion being white (7.3 mag), is located at a mutual distance of 31.1" and actually completes an orbit every 150 years. The stellar field around it is composed of a chain of relatively bright stars, forming a circle and an arc of three fainter stars. \ No newline at end of file diff --git a/en/star/φ_Hyi.md b/en/star/φ_Hyi.md new file mode 100644 index 000000000..51985c2ed --- /dev/null +++ b/en/star/φ_Hyi.md @@ -0,0 +1,9 @@ +--- +name: φ Hyi +constellation: Hyi +created_by: editor.cs +created_date: 2023-11-05 17:43:40.698864 +updated_by: editor.cs +updated_date: 2023-11-05 17:43:40.698869 +--- +An optical double star distinguishable under good conditions with the naked eye. Both components have nearly the same brightness - 5.4 mag and 5.5 mag. These red giants are located at a distance of 740 and 470 light-years. \ No newline at end of file