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Theta Cancri

From Wikipedia, the free encyclopedia
Star system in the constellation Cancer
Theta Cancri
Location of θ Cancri (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCancer[1]
Right ascension08h 31m 35.730s[2]
Declination+18° 05′ 39.91″[2]
Apparent magnitude (V)+5.323[3]
Characteristics
Evolutionary stagered giant branch[2]
Spectral typeK5 III[4]
U−Bcolor index+1.949[3]
B−Vcolor index+1.565[3]
Astrometry
Radial velocity (Rv)+44.47±0.19[5] km/s
Proper motion (μ)RA: −59.639mas/yr[2]
Dec.: −56.615mas/yr[2]
Parallax (π)7.5577±0.1008 mas[2]
Distance432 ± 6 ly
(132 ± 2 pc)
Absolute magnitude (MV)−0.19[1]
Details
Mass1.3[6] M
Radius67[2] R
Luminosity949[2] L
Surface gravity (log g)1.82[6] cgs
Temperature3,998[6] K
Metallicity[Fe/H]−0.19[6] dex
Other designations
θ Cnc,31 Cancri,BD+18°1963,FK5 2667,HD 72094,HIP 41822,HR 3357,SAO 97881[7]
Database references
SIMBADdata

Theta Cancri, is amultiple star[8][4] system in thezodiacconstellation ofCancer. Its name is aBayer designation that isLatinised from θ Cancri, and abbreviated Theta Cnc or θ Cnc. This star is visible to thenaked eye as a dim point of light with anapparent visual magnitude of +5.32.[3] The system is located at a distance of approximately 432light-years (132 pc) from the Sun, based onparallax,[2] and is drifting further away with aradial velocity of +44 km/s.[5] Since it is near theecliptic, it can beocculted by theMoon[9] and, very rarely, byplanets.

The primary, designated component A, isK-typegiant star with astellar classification of K5 III,[4] having exhausted the supply of hydrogen at itscore, then cooled and expanded. At present it has 67 times the girth of the Sun. It is radiating 949[2] times theluminosity of the Sun at aneffective temperature of3,998 K.[6]

InChinese astronomy,Ghost (Chinese:鬼宿;pinyin:Guǐ Xiù) refers to anasterism consisting of Theta Cancri,Eta Cancri,Gamma Cancri andDelta Cancri.[10] 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.[11]

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. ^abcdefghiVallenari, 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. ^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.
  4. ^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.
  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. ^abcdeKhalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G.; Valentini, M.; Torralba Elipe, G.; Steinmetz, M.; Pantaleoni-González, M.; Malhotra, S.; Jiménez-Arranz, Ó.; Enke, H.; Casamiquela, L.; Ardèvol, J. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost".Astronomy and Astrophysics.691: A98.arXiv:2407.06963.Bibcode:2024A&A...691A..98K.doi:10.1051/0004-6361/202451427.
  7. ^"tet Cnc",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-06-19.
  8. ^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.
  9. ^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.
  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. 394,ISBN 978-986-7332-25-7.
  11. ^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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