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79 Cancri

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G-type star in the constellation Cancer
79 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cancer
Right ascension 09 10 20.85841
Declination +21° 59′ 47.1000″
Apparent magnitude (V) 6.04
Characteristics
Evolutionary stage giant
Spectral type G5 III
B−V color index 0.871
Astrometry
Radial velocity (Rv)−3.24±0.13 km/s
Proper motion (μ) RA: +2.933 mas/yr
Dec.: +5.027 mas/yr
Parallax (π)8.1569 ± 0.0676 mas
Distance400 ± 3 ly
(123 ± 1 pc)
Absolute magnitude (MV)0.78
Details
Mass2.30 M
Radius9.41+0.38
−0.57 R
Luminosity57.6±0.6 L
Surface gravity (log g)2.88 cgs
Temperature5,076±47 K
Metallicity −0.10 dex
Age770 Myr
Other designations
79 Cnc, BD+22°2063, GC 12655, HD 78715, HIP 45033, HR 3640, SAO 80674, WDS 09103+2200
Database references
SIMBADdata

79 Cancri is a star in the constellation Cancer, located 400 light years from the Sun. It is just visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 6.04. This object is gradually moving slower to the Earth with a heliocentric radial velocity of −3.2 km/s.

This is an aging giant star with a stellar classification of G5 III, which indicates that, at the age of 770 million years, it has exhausted the hydrogen at its core and evolved away from the main sequence. The star has 2.30 times the mass of the Sun and has expanded to 9.4 times the Sun's radius. It is radiating 58 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,076 K.

References

  1. ^ 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.
  2. ^ 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.
  3. ^ 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.
  4. ^ Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3), 88, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
  5. ^ Liu, Y. J.; et al. (April 2014), "The Lithium Abundances of a Large Sample of Red Giants", The Astrophysical Journal, 785 (2): 12, arXiv:1404.1687, Bibcode:2014ApJ...785...94L, doi:10.1088/0004-637X/785/2/94, S2CID 119226316, 94.
  6. "78 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-03-11.
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