Gamma Piscium
Gamma Piscium (Gamma Psc, γ Piscium, γ Psc) is a star approximately 138 light years away from Earth,[1] 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[3] solar radii in size and shines with the light of 63 Suns.[3] At an apparent magnitude of 3.7,[2] it is the second brightest star in the constellation Pisces, between Eta and Alpha. Once a white A2 star, it is 5.5 billion years old.[dubious ]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Pisces |
| Right ascension | 23h 17m 09.93749s[1] |
| Declination | +03° 16′ 56.2380″[1] |
| Apparent magnitude (V) | 3.699[2] |
| Characteristics | |
| Spectral type | G8 III[3] |
| U−B color index | +0.572 [2] |
| B−V color index | +0.924[2] |
| Astrometry | |
| Radial velocity (Rv) | -13.6[4] km/s |
| Proper motion (μ) | RA: 759.82[1] mas/yr Dec.: 17.77[1] mas/yr |
| Parallax (π) | 23.64 ± 0.18 mas[1] |
| Distance | 138 ± 1 ly (42.3 ± 0.3 pc) |
| Absolute magnitude (MV) | 0.68 ± 0.08[5] |
| Details | |
| Mass | 1.11±0.29[3] M☉ |
| Radius | 11.28±0.10[3] R☉ |
| Luminosity | 62.7±3.3[3] L☉ |
| Surface gravity (log g) | 2.43 ± 0.06[5] cgs |
| Temperature | 4833±62[3] K |
| Metallicity [Fe/H] | −0.51[5] dex |
| Age | 4.58±3.10[3] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Gamma Piscium moves across the sky at three-quarters of an arcsecond per year, which at 138 light years corresponds to 153 kilometers per second. 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."[7]
Naming
In Chinese, 霹靂 (Pī Lì), meaning Thunderbolt, refers to an asterism consisting of γ Piscium, β Piscium, θ Piscium, ι Piscium and ω Piscium. Consequently, the Chinese name for γ Piscium itself is 霹靂二 (Pī Lì èr, English: the Second Star of Thunderbolt.)[8]
Planetary system
In 2021, a gas giant planet was detected by radial velocity method.[9]
| Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| Gamma Piscium b | >1.34+0.02 −0.31 MJ | 1.32+0.05 −0.08 | 555.1+6.0 −2.5 | 0.204+0.114 −0.141 | — | — |
In fiction
In Frank Herbert's Dune series, Gamma Waiping (The Chinese name for Pisces) is the home system of Imperial House Corrino.[citation needed]
References
- ^ a b c d e f van Leeuwen, Floor (13 August 2007). "Validation of the new Hipparcos reduction". Astronomy & Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. eISSN 1432-0746. ISSN 0004-6361. Vizier catalog entry
- ^ a b c d Cousins, A. W. J. (1984), "Standardization of Broadband Photometry of Equatorial Standards", South African Astronomical Observatory Circulars, 8: 59, Bibcode:1984SAAOC...8...59C
- ^ a b c d e f g h Baines, Ellyn K.; et al. (2018). "Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer". The Astronomical Journal. 155 (1). 30. arXiv:1712.08109. Bibcode:2018AJ....155...30B. doi:10.3847/1538-3881/aa9d8b. S2CID 119427037.
- ^ Wielen, R.; et al. (1999), "Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg, Astronomisches Rechen-Institut Heidelberg, 35 (35): 1, Bibcode:1999VeARI..35....1W
- ^ a b c da Silva, L.; et al. (November 2006), "Basic physical parameters of a selected sample of evolved stars", Astronomy and Astrophysics, 458 (2): 609–623, arXiv:astro-ph/0608160, Bibcode:2006A&A...458..609D, doi:10.1051/0004-6361:20065105, S2CID 9341088
- ^ "* gam Psc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved September 30, 2007.
- ^ "SPACE.com -- SpaceWatch -- Pisces Rising". Space.com. Retrieved September 30, 2007.[dead link]
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 8 日
- ^ a b Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro (2022), "Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate", Publications of the Astronomical Society of Japan, 74: 92–127, arXiv:2112.07169, doi:10.1093/pasj/psab112