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Rho Ceti

From Wikipedia, the free encyclopedia
A-type main sequence star in the constellation Cetus
Rho Ceti
Location of ρ Ceti (circled in red)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCetus
Right ascension02h 25m 57.00560s[1]
Declination−12° 17′ 25.7104″[1]
Apparent magnitude (V)4.885[2]
Characteristics
Spectral typeA0 V[3]
U−Bcolor index+0.001[2]
B−Vcolor index−0.037[2]
Astrometry
Radial velocity (Rv)+18.9±2.0[4] km/s
Proper motion (μ)RA: −11.28[1]mas/yr
Dec.: −9.48[1]mas/yr
Parallax (π)7.15±0.26 mas[1]
Distance460 ± 20 ly
(140 ± 5 pc)
Absolute magnitude (MV)−0.85[5]
Details
Radius3.1[6] R
Luminosity178[7] L
Temperature8,905[7] K
Rotational velocity (v sin i)219[8] km/s
Other designations
ρ Cet,72 Cet,BD−12°451,FK5 1066,HD 15130,HIP 11345,HR 708,SAO 148385.[9]
Database references
SIMBADdata

Rho Ceti,Latinized from ρ Ceti, is theBayer designation for astar in theequatorialconstellation ofCetus. It is faintly visible to the naked eye with anapparent visual magnitude of 4.885.[2] The distance to this star, based upon an annualparallax shift of 7.15 mas,[1] is around 460 light years.

This is anA-type main sequence star with astellar classification of A0 V.[3] It is spinning rapidly with aprojected rotational velocity of 219[8] km/s, giving the star anoblate shape with anequatorial bulge that is 10% larger than the polar radius.[10] The star has an estimated size 3.1[6] times theradius of the Sun and is radiating 178 times thesolar luminosity from itsouter atmosphere at aneffective temperature of 8,905 K.[7]

Name

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This star, along withπ Cet,ε Cet andσ Cet, was Al Sufi'sAl Sadr al Ḳaiṭos, the Whale's Breast[11]

According to the catalogue of stars in theTechnical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Stars,Al Sadr al Ḳaiṭos were the title for four stars :this star (ρ Cet) asAl Sadr al Ḳaiṭos I,σ Cet asAl Sadr al Ḳaiṭos II,ε Cet asAl Sadr al Ḳaiṭos III andπ Cet asAl Sadr al Ḳaiṭos IV[12]

InChinese,芻蒿 (Chú Hāo), meaningHay, refers to an asterism consisting of ρ Ceti,77 Ceti,67 Ceti,71 Ceti,HD 14691[13] andε Cet. Consequently, theChinese name for ρ Ceti itself is芻蒿一 (Chú Hāo yī, English:the First Star of Celestial Meadows.[14]

References

[edit]
  1. ^abcdefvan Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdGutierrez-Moreno, Adelina; et al. (1966), "A System of photometric standards",Publ. Dept. Astron. Univ. Chile,1, Publicaciones Universidad de Chile, Department de Astronomy:1–17,Bibcode:1966PDAUC...1....1G.
  3. ^abHouk, Nancy; Smith-Moore, M. (1978), "Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars",Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume 4,4, Ann Arbor: Dept. of Astronomy, University of Michigan,Bibcode:1988mcts.book.....H.
  4. ^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.
  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. ^abPasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (2) (3rd ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  7. ^abcMcDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–57,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  8. ^abRoyer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions",Astronomy and Astrophysics,463 (2):671–682,arXiv:astro-ph/0610785,Bibcode:2007A&A...463..671R,doi:10.1051/0004-6361:20065224,S2CID 18475298.
  9. ^"rho Cet".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-02-09.
  10. ^Belle, G. T. (2012). "Interferometric observations of rapidly rotating stars".The Astronomy and Astrophysics Review.20 (1): 51.arXiv:1204.2572.Bibcode:2012A&ARv..20...51V.doi:10.1007/s00159-012-0051-2.S2CID 119273474.
  11. ^Allen, R. H. (1963).Star Names: Their Lore and Meaning (Reprint ed.). New York: Dover Publications Inc. p. 162.ISBN 0-486-21079-0. Retrieved2010-12-12.{{cite book}}:ISBN / Date incompatibility (help)
  12. ^Jack W. Rhoads -Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propulsion Laboratory, California Institute of Technology; November 15, 1971
  13. ^(in Chinese)夢之大地 @ 國立成功大學 WebBBS DreamLand @ National Cheng Kung University WebBBS System
  14. ^(in Chinese)AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 12 日Archived 2011-05-22 at theWayback Machine

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