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85 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Aries
85 Ceti

Location 85 Ceti (HD 16861) within the Aries constellation (pink)
Observation data
Epoch J2000      Equinox J2000
ConstellationAries
Right ascension02h 42m 28.93647s[1]
Declination+10° 44′ 30.2137″[1]
Apparent magnitude (V)6.30[2]
Characteristics
Spectral typeA2 V[3]
U−Bcolor index+0.06[2]
B−Vcolor index+0.06[2]
R−Icolor index0.02
Astrometry
Radial velocity (Rv)+6.1[4] km/s
Proper motion (μ)RA: –22.88[1]mas/yr
Dec.: –22.95[1]mas/yr
Parallax (π)7.87±1.05 mas[1]
Distanceapprox. 410 ly
(approx. 130 pc)
Details
Mass2.38 ± 0.15[5] M
Luminosity48[5] L
Temperature8,810[5] K
Rotational velocity (v sin i)18[6] km/s
Other designations
BD+10° 360,HD 16861,HIP 12647,HR 797,NSV 899,SAO 93067.[7]
Database references
SIMBADdata

85 Ceti is an olderFlamsteed designation[8] for astar that is now within the borders of the northernconstellation ofAries,[9] the ram. In the present day it is known by star catalogue designations such asHD 16861 andHR 797.[7] It has anapparent visual magnitude of 6.30[2] and is approximately 410light-years (130parsecs) distant from the Earth. This is anA-type main sequence star with astellar classification of A2 V.[3] It has 2.4 times the mass of the Sun and shines with 48 times the Sun's luminosity. This energy is being radiated into outer space from the star'souter atmosphere at aneffective temperature of 8,810 K.[5] This heat gives it the white-hued glow of anA-type star.[10]

References

[edit]
  1. ^abcdevan Leeuwen, F. (November 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. ^abcdJohnson, H. L.; et al. (1966). "UBVRIJKL photometry of the bright stars".Communications of the Lunar and Planetary Laboratory.4 (99): 99.Bibcode:1966CoLPL...4...99J.
  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. ^Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities",Washington, Carnegie Institute of Washington D.C.,Bibcode:1953GCRV..C......0W.
  5. ^abcdZorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  6. ^Royer, F.; Zorec, J.; Gómez, A. E. (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.
  7. ^ab"HD 16861".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-07-18.
  8. ^Smart, W. M. (June 1939), "The Ursa Major cluster, (Second paper)",Monthly Notices of the Royal Astronomical Society,99 (9):710–722,Bibcode:1939MNRAS..99..710S,doi:10.1093/mnras/99.9.710. Page 712 of this reference links 85 Cet to B.S. 797; B.S., an abbreviation of theBright Star Catalogue, was an earlier version of the Harvard Revised Photometry Catalogue, or HR. Hence, 85 Ceti is the same as HR 797.
  9. ^Hoffleit, D. (July 1979), "Discordances in Star Designations",Bulletin d'Information du Centre de Données Stellaires,17 (17): 38,Bibcode:1979BICDS..17...38H.
  10. ^"The Colour of Stars",Australia Telescope, Outreach and Education,Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on March 18, 2012, retrieved2012-01-16.

External links

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