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34 Cancri

From Wikipedia, the free encyclopedia
Star in the constellation Cancer
34 Cancri
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCancer
Right ascension08h 32m 39.87069s[1]
Declination+10° 03′ 57.6306″[1]
Apparent magnitude (V)6.48[2]
Characteristics
Spectral typeA1 V[3][4]
B−Vcolor index−0.007±0.007[2]
Astrometry
Radial velocity (Rv)−11.0±7.4[5] km/s
Proper motion (μ)RA: +4.517[1]mas/yr
Dec.: −6.139[1]mas/yr
Parallax (π)5.7408±0.0912 mas[1]
Distance568 ± 9 ly
(174 ± 3 pc)
Absolute magnitude (MV)0.40[2]
Details
Mass2.67±0.09[6] M
Radius2.7[7] R
Luminosity69.84[2] L
Temperature9,661±111[6] K
Rotational velocity (v sin i)18[6] km/s
Age336[2] Myr
Other designations
34 Cnc,BD+10°1818,GC 11689,HD 72359,HIP 41904,HR 3372,SAO 97902[4]
Database references
SIMBADdata

34 Cancri is astar in thezodiacconstellation ofCancer, located about 568 light years away from the Sun.[1] It is a challenge to view with the naked even under good viewing conditions, having anapparent visual magnitude of 6.48.[2] At the distance of this star, its visual magnitude is diminished by anextinction of 0.14 due tointerstellar dust.[8]

This is anA-type main-sequence star with astellar classification of A1 V.[3] It is achemically peculiar star, possibly of the magnetic-type (CP2), showing an abnormal abundance of strontium.[9] The star is an estimated 336[2] million years old with only a moderateprojected rotational velocity of 18 km/s.[6] It has an estimated 2.7[6] times themass of the Sun and about 2.7[7] times the Sun's radius. The star is radiating 70[2] times theSun's luminosity from itsphotosphere at aneffective temperature of 9,661 K.[6]

References

[edit]
  1. ^abcdefBrown, 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 atVizieR.
  2. ^abcdefghAnderson, 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. ^abCowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications",Astronomical Journal,74:375–406,Bibcode:1969AJ.....74..375C,doi:10.1086/110819.
  4. ^ab"34 Cnc".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-02-28.
  5. ^de 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. ^abcdefZorec, J.; et al. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy and Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  7. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (Third ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  8. ^Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars",Astronomy Letters,38 (11):694–706,arXiv:1606.09028,Bibcode:2012AstL...38..694G,doi:10.1134/S1063773712110035,S2CID 119108982.
  9. ^Wraight, K. T.; et al. (February 2012), "A photometric study of chemically peculiar stars with the STEREO satellites - I. Magnetic chemically peculiar stars",Monthly Notices of the Royal Astronomical Society,420 (1):757–772,arXiv:1110.6283,Bibcode:2012MNRAS.420..757W,doi:10.1111/j.1365-2966.2011.20090.x,S2CID 14811051.
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