astro.wikisort.org - StarPhi1 Cancri, Latinised from φ1 Cancri, is a solitary,[3] orange-hued star in the constellation Cancer. It is faintly visible to the naked eye with an apparent visual magnitude of +5.57.[2] Based upon an annual parallax shift of 8.74 mas,[1] it is approximately 370 light-years from the Sun.
Orange-hued giant star in the constellation Cancer
Phi1 Cancri
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
Constellation |
Cancer |
Right ascension |
08h 26m 27.70615s[1] |
Declination |
+27° 53′ 36.8867″[1] |
Apparent magnitude (V) |
+5.57[2] |
Characteristics |
Spectral type |
K5 III[3] |
U−B color index |
+1.68[2] |
B−V color index |
+1.40[2] |
Astrometry |
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Radial velocity (Rv) | +25.25±0.19[4] km/s |
Proper motion (μ) | RA: −33.28[1] mas/yr Dec.: −116.17[1] mas/yr |
Parallax (π) | 8.74 ± 0.40 mas[1] |
Distance | 370 ± 20 ly (114 ± 5 pc) |
Absolute magnitude (MV) | +0.29[5] |
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Details |
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Radius | 17[6] R☉ |
Luminosity | 121[7] L☉ |
Temperature | 4,138[7] K |
Metallicity [Fe/H] | −0.134±0.093[8] dex |
Rotational velocity (v sin i) | 1.3[9] km/s |
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Other designations |
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Database references |
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SIMBAD | data |
This is an evolved K-type giant star with a stellar classification of K5 III.[3] The measured angular diameter of this star, after correction for limb darkening, is 1.87±0.02 mas.[11] At the estimated distance of Phi1 Cancri, this yields a physical size of about 17 times the radius of the Sun.[6] It is radiating 121 times the Sun's luminosity from its photosphere at an effective temperature of 4,138 K.[7]
References
- van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
- Ducati, J. R. (2002), "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system", CDS/ADC Collection of Electronic Catalogues, 2237, Bibcode:2002yCat.2237....0D.
- Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
- Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by:

- Cousins, A. W. J.; et al. (1966), "Photoelectric magnitudes and colours of southern stars, II", Royal Observatory Bulletins, 121: 1, Bibcode:1966RGOB..121....1C.
- Taylor, B. J. (February 1999), "Catalogs of temperatures and [Fe/H] averages for evolved G and K stars", Astronomy and Astrophysics Supplement, 134 (3): 523–524, Bibcode:1999A&AS..134..523T, doi:10.1051/aas:1999153.
- De Medeiros, J. R.; et al. (November 2000), "Rotation and lithium in single giant stars", Astronomy and Astrophysics, 363: 239–243, arXiv:astro-ph/0010273, Bibcode:2000A&A...363..239D.
- "phi01 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-06-09.
- Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode:2005A&A...431..773R, doi:10.1051/0004-6361:20042039.
Constellation of Cancer |
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Stars | |
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Galaxies | NGC | |
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Other |
- 3C 191
- 3C 212
- 3C 215
- OJ 287
- QSO B0839+187
- DLA0817g
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 Category |
На других языках
- [en] Phi1 Cancri
[ru] Фи¹ Рака
φ1 Рака (22 Рака, лат. φ1 Cancri) — двойная звезда, которая находится в созвездии Рака. Главная звезда, φ1 Рака А, — оранжевый гигант класса K с видимой звёздной величиной в +5,58. Находится на расстоянии около 398 световых лет от Земли.
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