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Sigma2 Cancri

From Wikipedia, the free encyclopedia
White-hued subgiant star in the constellation Cancer
For other stars with this Bayer designation, seeσ Cancri.
Sigma2 Cancri
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCancer[1]
Right ascension08h 56m 56.598s[2]
Declination+32° 54′ 37.54″[2]
Apparent magnitude (V)+5.436[3]
Characteristics
Evolutionary stagemain sequence[4][2]
Spectral typeA7 IV[4]
B−Vcolor index+0.157[3]
Astrometry
Radial velocity (Rv)−26.2±0.7[5] km/s
Proper motion (μ)RA: −53.031mas/yr[2]
Dec.: −66.186mas/yr[2]
Parallax (π)17.0377±0.0716 mas[2]
Distance191.4 ± 0.8 ly
(58.7 ± 0.2 pc)
Absolute magnitude (MV)+1.57[1]
Details
Mass1.79[6] M
Radius2.28+0.02
−0.04
[2] R
Luminosity21.5[4] L
Surface gravity (log g)4.17[6] cgs
Temperature8,309±283[6] K
Rotational velocity (v sin i)133[4] km/s
Age441[6] Myr
Other designations
σ2 Cnc,59 Cancri,BD+33°1785,HD 76398,HIP 43932,HR 3555,SAO 61146[7]
Database references
SIMBADdata

Sigma2 Cancri is a solitary,[8] white-huedstar in theconstellationCancer. Its name is aBayer designation that isLatinized from σ2 Cancri, and abbreviated Sigma2 Cnc σ2 Cnc. This star is faintly visible to thenaked eye, having anapparent visual magnitude of +5.44.[3] Based upon an annualparallax shift of17.04 mas as seen from Earth,[2] this star is located 191light-years (59 pc) from theSun. It is drifting closer to the Sun with aradial velocity of −26 km/s.[5]

With an estimated age of 441[6] million years, this is anA-typesubgiant star with astellar classification of A7 IV.[4] It is spinning rapidly with aprojected rotational velocity of 133 km/s.[4] The star has an estimated 1.8[6] times themass of the Sun with 2.3 times the Sun's radius.[2] It is radiating 21.5[4] times theSun's luminosity from itsphotosphere at aneffective temperature of roughly 8,309 K.[6]

References

[edit]
  1. ^abAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdefghVallenari, A.; et al. (Gaia collaboration) (2023),"Gaia Data Release 3. Summary of the content and survey properties",Astronomy and Astrophysics,674: A1,arXiv:2208.00211,Bibcode:2023A&A...674A...1G,doi:10.1051/0004-6361/202243940,S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcHøg, E.; et al. (March 2000), "The Tycho-2 catalogue of the 2.5 million brightest stars",Astronomy and Astrophysics,355:L27 –L30,Bibcode:2000A&A...355L..27H,doi:10.1888/0333750888/2862.
  4. ^abcdefgZorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  5. ^abde 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.
  6. ^abcdefgDavid, 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.
  7. ^"sig02 Cnc",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-06-12.
  8. ^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.
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