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Phi3 Ceti

From Wikipedia, the free encyclopedia
Star in the constellation Cetus
For other stars with thisBayer designation, seeφ Ceti.
Phi3 Ceti
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationCetus
Right ascension00h 56m 01.48867s[1]
Declination−11° 15′ 59.4988″[1]
Apparent magnitude (V)5.31[2]
Characteristics
Spectral typeK5 III[3]
B−Vcolor index+1.52[2]
Astrometry
Radial velocity (Rv)−25.48±0.38[1] km/s
Proper motion (μ)RA: −26.909[1]mas/yr
Dec.: −7.174[1]mas/yr
Parallax (π)6.1068±0.2570 mas[1]
Distance530 ± 20 ly
(164 ± 7 pc)
Absolute magnitude (MV)−0.78[4]
Details
Mass1.4[5] M
Radius44.33+0.76
−2.94
[1] R
Luminosity441±21[1] L
Surface gravity (log g)1.67[6] cgs
Temperature3,974+139
−34
[1] K
Metallicity [Fe/H]−0.31[6] dex
Rotational velocity (v sin i)1.0[5] km/s
Other designations
φ3 Ceti,22 Cet,BD−12° 162,HD 5437,HIP 4371,HR 267,SAO 147519[7]
Database references
SIMBADdata

Phi3 Ceti is a solitary,[8] orange-huedstar in the equatorialconstellation ofCetus. It is faintly visible to the naked eye with anapparent visual magnitude of 5.31.[2] Based upon an annualparallax shift of6.11 mas as seen from Earth,[1] it is located approximately 530 light years from theSun, give or take 20 light years. The star is drifting closer with aradial velocity of −25.5 km/s.[1]

This is anevolvedK-typegiant star with astellar classification of K5 III.[3] It has about 1.4[5] times the mass and 44[1] times the radius of the Sun. The star radiates 441 times thesolar luminosity from itsphotosphere at aneffective temperature of 3,974 K.[1]

References

[edit]
  1. ^abcdefghijklmBrown, 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. ^abcJohnson, 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. ^abHouk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5, Ann Arbor, Michigan: Department of Astronomy, University of Michigan,Bibcode:1999MSS...C05....0H.
  4. ^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.
  5. ^abcMelo, C. H. F.; et al. (August 2005), "On the nature of lithium-rich giant stars. Constraints from beryllium abundances",Astronomy and Astrophysics,439 (1):227–235,arXiv:astro-ph/0504133,Bibcode:2005A&A...439..227M,doi:10.1051/0004-6361:20041805,S2CID 10580797.
  6. ^abSoubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters",Astronomy and Astrophysics,515: A111,arXiv:1004.1069,Bibcode:2010A&A...515A.111S,doi:10.1051/0004-6361/201014247,S2CID 118362423.
  7. ^"phi03 Cet".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-04-22.
  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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