Astronomy:Rho Ceti

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Short description: A-type main sequence star in the constellation Cetus
Rho Ceti
Location of ρ Ceti (circled in red)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cetus[1]
Right ascension  02h 25m 57.006s[2]
Declination −12° 17′ 25.708″[2]
Apparent magnitude (V) 4.885[3]
Characteristics
Evolutionary stage subgiant[4]
Spectral type A0 V[5]
U−B color index +0.001[3]
B−V color index −0.037[3]
Astrometry
Radial velocity (Rv)+18.9±2.0[6] km/s
Proper motion (μ) RA: −11.596[2] mas/yr
Dec.: −9.786[2] mas/yr
Parallax (π)5.8054 ± 0.1358[2] mas
Distance560 ± 10 ly
(172 ± 4 pc)
Absolute magnitude (MV)−0.85[1]
Details
Mass2.3[7] M
Radius6.3[8] R
Luminosity328[9] L
Surface gravity (log g)3.56[10] cgs
Temperature9,505[10] K
Rotational velocity (v sin i)219[11] km/s
Age72[7] Myr
Other designations
ρ Cet, 72 Cet, BD−12°451, FK5 1066, HD 15130, HIP 11345, HR 708, SAO 148385[12]
Database references
SIMBADdata

Rho Ceti is a star in the equatorial constellation of Cetus. Its name is a Bayer designation that is Latinized from ρ Ceti, and abbreviated Rho Cet or ρ Cet. This star is faintly visible to the naked eye with an apparent visual magnitude of 4.885.[3] The distance to this star, based upon an annual parallax shift of 5.81 mas,[2] is around 560 light years. It is drifting further away with a line of sight velocity component of +19 km/s.[6]

This star has a stellar classification of A0 V,[5] which is presenting as an A-type main sequence star. However, it may be in the subgiant stage of its evolution.[4] It is spinning rapidly with a projected rotational velocity of 219[11] km/s, giving the star an oblate shape with an equatorial bulge that is 10% larger than the polar radius.[13] The star has an estimated size 6.3 times the radius of the Sun[8] and is radiating 328 times the solar luminosity[9] from its outer atmosphere at an effective temperature of 9,505 K.[10]

Name

This star, along with π Cet, ε Cet and σ Cet, was Al Sufi's Al Sadr al Ḳaiṭos, the Whale's Breast.[14]

According to the catalogue of stars in the Technical 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) as Al Sadr al Ḳaiṭos I, σ Cet as Al Sadr al Ḳaiṭos II, ε Cet as Al Sadr al Ḳaiṭos III and π Cet as Al Sadr al Ḳaiṭos IV.[15]

In Chinese, 芻蒿 (Chú Hāo), meaning Hay, refers to an asterism consisting of ρ Ceti, 77 Ceti, 67 Ceti, 71 Ceti, HD 14691[16] and ε Cet. Consequently, the Chinese name for ρ Ceti itself is 芻蒿一 (Chú Hāo yī, English: the First Star of Celestial Meadows.[17]

References

  1. 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode2012AstL...38..331A  XHIP record for this object at VizieR.
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940.  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 3.2 3.3 Gutierrez-Moreno, Adelina et al. (1966), "A System of photometric standards", Publ. Dept. Astron. Univ. Chile (Publicaciones Universidad de Chile, Department de Astronomy) 1: 1–17, Bibcode1966PDAUC...1....1G. 
  4. 4.0 4.1 Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy and Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode2012A&A...537A.120Z. 
  5. 5.0 5.1 Houk, Nancy; Smith-Moore, M. (1978), Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars, 4, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode1988mcts.book.....H. 
  6. 6.0 6.1 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, doi:10.1051/0004-6361/201219219, A61, Bibcode2012A&A...546A..61D. 
  7. 7.0 7.1 Gullikson, Kevin et al. (2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars", The Astronomical Journal 152 (2): 40, doi:10.3847/0004-6256/152/2/40, Bibcode2016AJ....152...40G. 
  8. 8.0 8.1 Stassun, Keivan G. et al. (2019), "The Revised TESS Input Catalog and Candidate Target List", The Astronomical Journal 158 (4): 138, doi:10.3847/1538-3881/ab3467, Bibcode2019AJ....158..138S. 
  9. 9.0 9.1 Fetherolf, Tara et al. (2023), "Variability Catalog of Stars Observed during the TESS Prime Mission", The Astrophysical Journal Supplement Series 268 (1): 4, doi:10.3847/1538-4365/acdee5, Bibcode2023ApJS..268....4F. 
  10. 10.0 10.1 10.2 Cardiel, Nicolás et al. (2021), "Synthetic RGB photometry of bright stars: Definition of the standard photometric system and UCM library of spectrophotometric spectra", Monthly Notices of the Royal Astronomical Society 504 (3): 3730, doi:10.1093/mnras/stab997, Bibcode2021MNRAS.504.3730C. 
  11. 11.0 11.1 Royer, F. et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics 463 (2): 671–682, doi:10.1051/0004-6361:20065224, Bibcode2007A&A...463..671R. 
  12. "rho Cet". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=rho+Cet. 
  13. Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review 20 (1): 51, doi:10.1007/s00159-012-0051-2, Bibcode2012A&ARv..20...51V. 
  14. Star Names: Their Lore and Meaning (Reprint ed.), New York: Dover Publications Inc., 1963, p. 162, ISBN ((0-486-21079-0)), https://archive.org/details/starnamestheirlo00alle/page/162, retrieved 2010-12-12. 
  15. Rhoads, Jack W. (November 15, 1971), Technical Memorandum 33-507-A Reduced Star Catalog Containing 537 Named Stars, Jet Propulsion Laboratory, California Institute of Technology, https://ntrs.nasa.gov/citations/19720005197. 
  16. Script error: The function "in_lang" does not exist. 夢之大地 @ 國立成功大學 WebBBS DreamLand @ National Cheng Kung University WebBBS System
  17. Script error: The function "in_lang" does not exist. AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 12 日