czsky/en/star/hr7790.md

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Peacock (α Pavi) Pav editor.cs 2023-11-05 16:42:14.809035 editor.cs 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.