3 Cancri
Star in the constellation Cancer
3 Cancri is a single[ 7] star in the zodiac constellation of Cancer , located around 810 light years from the Sun. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.60.[ 2] This object is moving further from the Earth with a heliocentric radial velocity of +39.5 km/s,[ 1] and may be a member of the Hyades group.[ 8] It is located near the ecliptic and thus is subject to lunar eclipses .[ 9]
This is an aging giant star with a stellar classification of K3 III[ 4] that is most likely (86% chance) on the horizontal branch .[ 3] The star has 2.9 times the mass of the Sun and has expanded to 40 times the Sun's radius .[ 3] It is radiating 569[ 2] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,300 K.[ 5]
Planetary system
One super-Jupiter exoplanet orbiting 3 Cancri was detected in 2020 on a very mildly eccentric orbit using the radial velocity method .[ 10]
See also
References
^ a b c d e f g Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d e 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 .
^ a b c d e Stock, S.; et al. (August 2018), "Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search", Astronomy & Astrophysics , 616 : 15, arXiv :0709.1145 , Bibcode :2018A&A...616A..33S , doi :10.1051/0004-6361/201833111 , S2CID 119361866 , A33.
^ a b Adams, Walter S.; et al. (1935), "The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars", Astrophysical Journal , 81 : 187, Bibcode :1935ApJ....81..187A , doi :10.1086/143628
^ a b c d e Hekker, S.; Meléndez, J. (2007), "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters", Astronomy and Astrophysics , 475 (3): 1003– 1009, arXiv :0709.1145 , Bibcode :2007A&A...475.1003H , doi :10.1051/0004-6361:20078233 , S2CID 10436552 .
^ "3 Cnc" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-02-22 .
^ 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 .
^ Eggen, O. J. (June 1972), "The red giants in the Hyades group", Publications of the Astronomical Society of the Pacific , 84 : 406, Bibcode :1972PASP...84..406E , doi :10.1086/129303 .
^ White, Nathaniel M.; Feierman, Barry H. (September 1987), "A Catalog of Stellar Angular Diameters Measured by Lunar Occultation", Astronomical Journal , 94 : 751, Bibcode :1987AJ.....94..751W , doi :10.1086/114513 .
^ Pinto, Marcelo Tala; Reffert, Sabine; Quirrenbach, Andreas; Stock, Stephan; Trifonov, Trifon; Mitchell, David S. (2020). "Precise radial velocities of giant stars". Astronomy & Astrophysics . 644 : A1. doi :10.1051/0004-6361/202038285 . hdl :10150/622444 .
^ "The Extrasolar Planet Encyclopaedia — 3 Cnc b" . Extrasolar Planets Encyclopaedia . Retrieved 2021-04-29 .