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83 Cancri

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Star in the constellation Cancer
83 Cancri
Observation data
Epoch J2000      Equinox J2000
Constellation Cancer
Right ascension 09 18 58.82772
Declination +17° 42′ 19.2744″
Apparent magnitude (V) 6.61
Characteristics
Evolutionary stage main sequence
Spectral type F4V + WD
B−V color index 0.487±0.030
Variable type constant
Astrometry
Radial velocity (Rv)−14.8±0.4 km/s
Proper motion (μ) RA: −135.130 mas/yr
Dec.: −105.267 mas/yr
Parallax (π)24.5641 ± 0.0966 mas
Distance132.8 ± 0.5 ly
(40.7 ± 0.2 pc)
Absolute magnitude (MV)3.57
Orbit
Period (P)32±2.5 d
Eccentricity (e)0.6±0.2
Inclination (i)94±6°
Longitude of the node (Ω)148±5°
Periastron epoch (T)1976.0±3.5
Argument of periastron (ω)
(secondary)
351±42°
Details
83 Cnc A
Mass1.13 M
Radius1.53+0.02
−0.05 R
Luminosity3.135±0.015 L
Surface gravity (log g)3.99 cgs
Temperature6,218+96
−53 K
Metallicity −0.26±0.02 dex
Age3.1 Gyr
83 Cnc B
Mass1.3 M
Other designations
83 Cnc, BD+18°2165, FK5 350, HD 80218, HIP 45699, SAO 98488
Database references
SIMBADdata

83 Cancri is an astrometric binary star system in the northern constellation of Cancer, positioned near the constellation border with Leo. It is a challenge to view with the naked eye, having an apparent visual magnitude of 6.61. Despite having a Flamsteed designation, the system was too faint to be included in the Bright Star Catalogue. It is located at a distance of 133 light years from the Sun, based on parallax, but is drifting closer with a radial velocity of −15 km/s. 83 Cancri has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.185 per annum.

The pair have an orbital period of around 32 days and an eccentricity of about 0.6. The visible member of this system, designated component A, is an F-type main-sequence star with a stellar classification of F4V. Its atmosphere is enhanced with s-process elements, particularly strontium and yttrium, which is attributed to mass transfer from the companion while the latter was on the asymptotic giant branch. The primary is 3.1 billion years old with 1.1 times the mass of the Sun and 1.5 times the Sun's radius. It is radiating 3.1 times the luminosity of the Sun from its photosphere at an effective temperature of 6,218 K. The unseen secondary companion is most likely a high mass white dwarf, having around 1.3 times the Sun's mass.

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. ^ Goncharov, G. A.; Kiyaeva, O. V. (April 2002), "Astrometric Orbits from a Direct Combination of Ground-Based Catalogs with the Hipparcos Catalog", Astronomy Letters, 28 (4): 261–271, Bibcode:2002AstL...28..261G, doi:10.1134/1.1467262, S2CID 121692881.
  4. ^ David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146, S2CID 33401607.
  5. "83 Cnc". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 August 2017.
  6. Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal, 147 (4): 14, arXiv:1401.6827, Bibcode:2014AJ....147...87T, doi:10.1088/0004-6256/147/4/87, S2CID 56066740, 87.
  7. 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.
  8. Bidelman, W. P. (December 1990), "Flamsteed stars not contained in the Yale "Catalogue of Bright Stars"", Bulletin d'Information du Centre de Données Stellaires, 38: 13, Bibcode:1990BICDS..38...13B.
  9. Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal, 129 (3): 1483–1522, arXiv:astro-ph/0412070, Bibcode:2005AJ....129.1483L, doi:10.1086/427854, S2CID 2603568.
  10. Reddy, Bacham E.; et al. (March 2003), "The chemical compositions of Galactic disc F and G dwarfs", Monthly Notices of the Royal Astronomical Society, 340 (1): 304–340, arXiv:astro-ph/0211551, Bibcode:2003MNRAS.340..304R, doi:10.1046/j.1365-8711.2003.06305.x, S2CID 14388692.
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