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69 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Cetus
69 Ceti
Observation data
EpochJ2000      EquinoxJ2000
ConstellationCetus
Right ascension02h 21m 56.62838s[1]
Declination+00° 23′ 44.4288″[1]
Apparent magnitude (V)5.287[2]
Characteristics
Evolutionary stageAGB[3]
Spectral typeM1/2III[4]
U−Bcolor index+1.85[5]
B−Vcolor index+1.65[5]
Astrometry
Radial velocity (Rv)+26.99±0.32[1] km/s
Proper motion (μ)RA: −12.393[1]mas/yr
Dec.: −8.059[1]mas/yr
Parallax (π)3.7821±0.2323 mas[1]
Distance860 ± 50 ly
(260 ± 20 pc)
Absolute magnitude (MV)−2.73[6]
Details
Radius100+10
−18
[1] R
Luminosity1,813±126[1] L
Temperature3,765+392
−177
[1] K
Other designations
69 Cet,BD−00°355,HD 14652,HIP 11021,HR 689,SAO 110495[7]
Database references
SIMBADdata

69 Ceti is a single[8]star located around 860[1] light years away in theequatorialconstellation ofCetus. It is visible to the naked eye with anapparent visual magnitude of 5.3.[2] This is an agingred giant star with astellar classification of M1/2III.[4] It is radiating 1,813 times theSun's luminosity from an enlargedphotosphere, 100 times theSun's radius, at aneffective temperature of 3,765 K.[1]

References

[edit]
  1. ^abcdefghijkBrown, 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. Gaia DR2 record for this source atVizieR.
  2. ^abHøg, E.; et al. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355: L27.Bibcode:2000A&A...355L..27H.doi:10.1888/0333750888/2862.
  3. ^Eggen, Olin J. (1992). "Asymptotic Giant Branch Stars Near the Sun".The Astronomical Journal.104: 275.Bibcode:1992AJ....104..275E.doi:10.1086/116239.
  4. ^abHouk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars".Michigan Spectral Survey.5.Bibcode:1999MSS...C05....0H.
  5. ^abJohnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4: 99.Bibcode:1966CoLPL...4...99J.
  6. ^Ryon, Jenna; Shetrone, Matthew D.; Smith, Graeme H. (2009). "Comparing the CaiiH and K Emission Lines in Red Giant Stars".Publications of the Astronomical Society of the Pacific.121 (882): 842.arXiv:0907.3346.Bibcode:2009PASP..121..842R.doi:10.1086/605456.S2CID 17821279.
  7. ^"69 Cet".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedDecember 28, 2018.
  8. ^Eggleton, 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.
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