Star Gamma Pavonis
Yellow-White star Gamma Pavonis is located 30 light years away from the Sun.
It is a single star of spectral class F9 V, that has 121 % of solar mass.
For now, there are no known exoplanets in this star system.
More about Gamma Pavonis
Nearby star Gamma Pavonis is a main sequence star that fuses hydrogen atoms into helium. It is is approximately 15 % bigger than the Sun and temperature on its surface is around 6160 K (5887 °C), which is about 107 % of Sun's temperature.
Gamma Pavonis can be found in southern celestial hemisphere, and it is possible to see it with naked eye.
Other designations of this star
γ Pav, CD−65° 2751, FK5 805, Gliese 827, HD 203608, HIP 105858, HR 8181, LHS 3674, LTT 8510, SAO 254999, gam Pav, Gaia EDR3 6401464693867773568
External sources
Simbad database (* gam Pav)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
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Right ascension: 21h 26m 26.816s
Declination: -65° 21' 45.504'' (southern hemisphere)
Parallax: 108.01
Sun distance: 30.197 ly | 9.3 pc
Temperature: 6160 K | 1.07 T Sun
Age: 1 billions years | 0.22 Sun
Luminosity: 1.52 L Sun
Apparent magnitude (V): 4.2
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