Star Delta Pavonis
Subgiant Delta Pavonis is located 20 light years away from the Sun.
It is a single star of spectral class G8 IV, that has 99 % of solar mass.
For now, there are no known exoplanets in this star system.
More about Delta Pavonis
Nearby star Delta Pavonis is is approximately 22 % bigger than the Sun and temperature on its surface is around 5600 K (5327 °C), which is about 97 % of Sun's temperature.
Delta Pavonis can be found in southern celestial hemisphere, and it is possible to see it with naked eye.
Other designations of this star
δ Pav, δ Pavonis, CD-66 2367, GCTP 4754, Gliese 780, HD 190248, HIP 99240, HR 7665, LHS 485, LTT 7946, LFT 1520, NSV 12790, SAO 254733, del Pav, Gaia EDR3 6427464123776727168
External sources
Simbad database (* del Pav)
Astronomical database SIMBAD (the Set of Identifications, Measurements and Bibliography for Astronomical Data)
Class of stars Subgiant
A subgiant is a term used to describe a luminous star that is typically running out of hydrogen for nuclear fusion and is thus departing from the main sequence. These stars are classified as Yerkes luminosity class IV.
stars
exoplanets
en
Right ascension: 20h 8m 46.817s
Declination: -66° 11' 13.529'' (southern hemisphere)
Parallax: 163.954
Sun distance: 19.893 ly | 6.1 pc
Temperature: 5600 K | 0.97 T Sun
Age: 9.3 billions years | 2.02 Sun
Luminosity: 1.22 L Sun
Apparent magnitude (V): 3.6
česky
espaňol
deutsch
francais
X (twitter)
facebook