Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pisces |
Right ascension | 23h 17m 09.937s[1] |
Declination | +03° 16′ 56.25″[1] |
Apparent magnitude (V) | 3.699[2] |
Characteristics | |
Evolutionary stage | Horizontal branch[3] |
Spectral type | G8 III[4] |
U−B color index | +0.572 [2] |
B−V color index | +0.924[2] |
Astrometry | |
Radial velocity (Rv) | −13.6[5] km/s |
Proper motion (μ) | RA: 759.268 mas/yr[1] Dec.: 17.568 mas/yr[1] |
Parallax (π) | 24.1958 ± 0.2967 mas[6] |
Distance | 135 ± 2 ly (41.3 ± 0.5 pc) |
Absolute magnitude (MV) | 0.68±0.08[7] |
Details | |
Mass | 0.97±0.12[3] M☉ |
Radius | 11.28±0.10[4] R☉ |
Luminosity | 62.7±3.3[4] L☉ |
Surface gravity (log g) | 2.43 ± 0.06[7] cgs |
Temperature | 4833±62[4] K |
Metallicity [Fe/H] | −0.51[7] dex |
Age | ~12[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Gamma Piscium (γ Piscium) is a star approximately 135 light years away from Earth in the zodiac constellation of Pisces. It is a yellow star with a spectral type of G8 III, meaning it has a surface temperature of 4,833 K and is a giant star. It is slightly cooler than the Sun, yet it is 11[4] solar radii in size and shines with the light of 63 Suns.[4] The star is a member of the red clump, which means it is undergoing core helium fusion.[9] At an apparent magnitude of 3.7,[2] it is the second brightest star in the constellation Pisces, between Eta and Alpha.
Gamma Piscium moves across the sky at three-quarters of an arcsecond per year, which at 135 light years corresponds to 153 kilometers per second.[citation needed] This suggests it is a visitor from another part of the Milky Way Galaxy; in astronomical terms, it will quickly leave the vicinity of the Sun. Its metallicity is only one-fourth that of the Sun, and visitors from outside the thin disk that composes the Milky Way tend to be metal-poor. Gamma Piscium is part of the asterism known as the "circlet of Pisces."[10]
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