Star in the constellation Cancer
For other stars with this Bayer designation , see ψ Cancri .
14 Cancri
Observation dataEpoch J2000.0 Equinox J2000.0 (ICRS )
Constellation
Canis Major
Right ascension
08 10 27.18056
Declination
+25° 30′ 26.4061″
Apparent magnitude (V)
+5.73
Characteristics
Spectral type
G7 V
U−B color index
+0.43
B−V color index
+0.81
Astrometry Radial velocity (Rv )−44.48±0.09 km/s Proper motion (μ) RA: −73.35 mas /yr Dec.: −347.60 mas /yr Parallax (π)24.18 ± 0.35 mas Distance 135 ± 2 ly (41.4 ± 0.6 pc ) Absolute magnitude (MV )+2.65
Details Mass 1.49±0.04 M ☉ Radius 3.20±0.11 R ☉ Luminosity 8 L ☉ Surface gravity (log g )3.87±0.08 cgs Temperature 5,311±23 K Metallicity −0.12±0.06 dex Rotational velocity (v sin i )0.98±0.42 km/s Age 2.39±0.14 Gyr
Other designations ψ Cnc , 14 Cnc , BD +25°1865, FK5 2633, GC 11091, HD 67767, HIP 40023, HR 3191, SAO 79995, CCDM 08104+2530
Database references SIMBAD data
14 Cancri is a star in the northern zodiac constellation of Cancer . It can be referred to as ψ Cancri , very occasionally as ψ Cancri , to distinguish it from 13 Cancri which is sometimes called ψ Cancri. It is just barely visible to the naked eye, having an apparent visual magnitude of +5.73. Based upon an annual parallax shift of 24.18 mas as seen from Earth, it is located 135 light years from the Sun . It may be a member of the Wolf 630 moving group of stars.
This object has a stellar classification of G7 V, which would suggest it is a G-type main-sequence star . However, Jofré et al. (2015) consider it to be a more evolved subgiant star due to a surface gravity of log g = 3.87. As such, it has an estimated 1.5 times the mass of the Sun and 3.2 times the Sun's radius . The star is 2.4 billion years old with what appears to be a leisurely rotation rate, judging by a projected rotational velocity of 0.98 km/s. It is radiating eight times the Sun's luminosity from its photosphere at an effective temperature of 5,311 K.
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 .
^ Argue, A. N. (1966), "UBV photometry of 550 F, G and K type stars", Monthly Notices of the Royal Astronomical Society , 133 (4): 475, Bibcode :1966MNRAS.133..475A , doi :10.1093/mnras/133.4.475 .
^ Cowley, A. P.; Bidelman, W. P. (February 1979), "MK spectral types for some F and G stars", Publications of the Astronomical Society of the Pacific , 91 : 83–86, Bibcode :1979PASP...91...83C , doi :10.1086/130446 .
^ Jofré, E.; et al. (2015), "Stellar parameters and chemical abundances of 223 evolved stars with and without planets", Astronomy & Astrophysics , 574 : A50, arXiv :1410.6422 , Bibcode :2015A&A...574A..50J , doi :10.1051/0004-6361/201424474 , S2CID 53666931 .
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 .
"tet Cnc" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-09-08.
Kostjuk, N. D. (2004), "VizieR Online Data Catalog: HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index (Kostjuk, 2002)", VizieR On-line Data Catalog: IV/27A. Originally Published in: Institute of Astronomy of Russian Academy of Sciences (2002) , 4027 , Bibcode :2004yCat.4027....0K .
McDonald, A. R. E.; Hearnshaw, J. B. (August 1983), "The Wolf 630 moving group of stars", Monthly Notices of the Royal Astronomical Society , 204 (3): 841–852, Bibcode :1983MNRAS.204..841M , doi :10.1093/mnras/204.3.841 .
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