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Theta Cancri

From Wikipedia, the free encyclopedia
Star in the constellation Cancer
Theta Cancri
Location of θ Cancri (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCancer
Right ascension08h 31m 35.73082s[1]
Declination+18° 05′ 39.9166″[1]
Apparent magnitude (V)+5.323[2]
Characteristics
Spectral typeK5 III[3]
U−Bcolor index+1.949[2]
B−Vcolor index+1.565[2]
Astrometry
Radial velocity (Rv)+44.47±0.19[4] km/s
Proper motion (μ)RA: −60.438[1]mas/yr
Dec.: −57.331[1]mas/yr
Parallax (π)7.3204±0.1826 mas[1]
Distance450 ± 10 ly
(137 ± 3 pc)
Absolute magnitude (MV)−0.19[5]
Details
Radius40.02+2.22
−2.35
[1] R
Luminosity353.1±10.1[1] L
Temperature3,955+121
−105
[1] K
Other designations
θ Cnc,31 Cancri,BD+18° 1963,FK5 2667,HD 72094,HIP 41822,HR 3357,SAO 97881[6]
Database references
SIMBADdata

Theta Cancri,Latinised from θ Cancri, is amultiple star[7][3] system in thezodiacconstellation ofCancer. It is visible to the naked eye as a dim point of light with anapparent visual magnitude of +5.32.[2] The system is located at a distance of approximately 450 light-years away from the Sun, based onparallax,[1] and is drifting further away with aradial velocity of +44 km/s.[4] Since it is near theecliptic, it can beocculted by theMoon[8] and, very rarely, byplanets.

The primary, designated component A, isK-typegiant star with astellar classification of K5 III,[3] having exhausted the supply of hydrogen at itscore, then cooled and expanded. At present it has 40[1] times the girth of the Sun. It is radiating 353[1] times theluminosity of the Sun at aneffective temperature of3,955 K.[1]

InChinese astronomy,Ghost (Chinese:鬼宿;pinyin:Guǐ Xiù) refers to anasterism consisting of Theta Cancri,Eta Cancri,Gamma Cancri andDelta Cancri.[9] Theta Cancri is the first star of Ghost (Chinese:鬼宿一;pinyin:Guǐ Xiù yī), as it is also the determinative star for that asterism.[10]

References

[edit]
  1. ^abcdefghijklBrown, 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. ^abcdGutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards",Publications of the Department of Astronomy University of Chile,1, Publicaciones Universidad de Chile, Department de Astronomy:1–17,Bibcode:1966PDAUC...1....1G.
  3. ^abcEggleton, 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.
  4. ^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.
  5. ^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.
  6. ^"tet Cnc -- Star",SIMBAD Astronomical Database, Centre de Données astronomiques de Strasbourg, retrieved2017-06-19.
  7. ^Hartkopf, W. I.; McAlister, H. A. (January 1984), "Binary stars unresolved by speckle interferometry. III",Publications of the Astronomical Society of the Pacific,96:105–116,Bibcode:1984PASP...96..105H,doi:10.1086/131309.
  8. ^White, Nathaniel M.; Feierman, Barry H. (September 1987), "A Catalog of Stellar Angular Diameters Measured by Lunar Occultation",Astronomical Journal,94: 751,Bibcode:1987AJ.....94..751W,doi:10.1086/114513.
  9. ^陳久金 (2005).Zhōngguó Xīngzuò Shénhuà中國星座神話 [Chinese Constellation Mythology]. 台灣古籍出版有限公司. p. 394.ISBN 978-986-7332-25-7.
  10. ^陳久金 (2005).Zhōngguó Xīngzuò Shénhuà中國星座神話 [Chinese Constellation Mythology]. 台灣古籍出版有限公司. p. 193.ISBN 978-986-7332-25-7.
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