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1 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Cetus
1 Ceti
Observation data
EpochJ2000      EquinoxJ2000
ConstellationCetus
Right ascension23h 58m 21.22532s[1]
Declination–15° 50′ 50.9421″[1]
Apparent magnitude (V)+6.276[2]
Characteristics
Spectral typeK1III CNII[3]
U−Bcolor index+1.03[4]
B−Vcolor index+1.08[4]
Astrometry
Radial velocity (Rv)4.3±2[5] km/s
Proper motion (μ)RA: +82.668[1]mas/yr
Dec.: –7.878[1]mas/yr
Parallax (π)6.0976±0.0711 mas[1]
Distance535 ± 6 ly
(164 ± 2 pc)
Absolute magnitude (MV)–0.10[6]
Details
Radius28[7] R
Luminosity143.53[6] L
Other designations
1 Cet,BD−16°6394,FK5 3925,GC 33242,HD 224481,HIP 118178,HR 9065,SAO 165972[8]
Database references
SIMBADdata

1 Ceti is astar in theconstellation ofCetus. With anapparent magnitude of about 6.2,[2] the star is barely visible to the naked eye (seeBortle scale).Parallax estimates put it at a distance of about 535light-years (164parsecs) away from theEarth. It is moving further from the Sun with a heliocentricradial velocity of 4 km/s.[5]

This star has aspectral type of K1III,[3] implying aK-type giant. These types of stars are generally reddish-colored stars with spectral types fromK toM, with radii that are 10 to 100 times larger than theSun.[9] The "CNII" in its spectral type indicates strongcyanogen signature in its outer atmosphere.[10][11] The star is radiating 144[6] times theSun's luminosity from its enlargedphotosphere.

References

[edit]
  1. ^abcdeBrown, 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.
  2. ^abHøg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27 –L30.Bibcode:2000A&A...355L..27H.
  3. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  4. ^abJohnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4: 99.Bibcode:1966CoLPL...4...99J.
  5. ^abWilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities".Carnegie Institute Washington D.C. Publication.Bibcode:1953GCRV..C......0W.
  6. ^abcAnderson, 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.
  7. ^Pasinetti Fracassini, L. E.; et al. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)".Astronomy & Astrophysics.367 (2) (Third ed.):521–24.arXiv:astro-ph/0012289.Bibcode:2001A&A...367..521P.doi:10.1051/0004-6361:20000451.S2CID 425754.
  8. ^"1 Cet".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedDecember 21, 2018.
  9. ^Darling, David."Red giant".The Internet Encyclopedia of Science. Retrieved21 March 2017.
  10. ^Keenan, Philip C. (1987)."Spectral types and their uses".Publications of the Astronomical Society of the Pacific.99: 713.Bibcode:1987PASP...99..713K.doi:10.1086/132036.
  11. ^Janes, K. A.; McClure, Robert D. (May 1971). "Strong-Cyanogen Stars: Photometry and Kinematics".Astrophysical Journal.165: 561.Bibcode:1971ApJ...165..561J.doi:10.1086/150921.
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