Peacock (α Pavonis) is the brightest star in the constellation Pavo. It is about 180 light-years (ly) away and has an apparent magnitude of 1.94 mag. It is only visible south of 32 degrees north latitude.
Peacock (α Pavonis) is a spectroscopic double star with an orbital period of 11.8 days, suggesting a distance of the two components of just 0.21 AU.
Peacock | |
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Constellation | Pavo |
Right ascension | 20h 25m 38.86s |
Declination | -56° 44′ 6.3″ |
Apparent magnitude | 1.94 mag |
Distance | (179 ± 5) ly |
Bayer designation | α Pavonis |
Bright Star Catalogue | HR 7790 |
Hipparcos Catalogue | HIP 100751 |
SAO Catalogue | SAO 246574 |
