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62 Arietis

From Wikipedia, the free encyclopedia
Star in the constellation Aries
62 Arietis
Observation data
Epoch J2000      Equinox J2000
ConstellationAries
Right ascension03h 22m 11.89351s[1]
Declination+27° 36′ 27.1911″[1]
Apparent magnitude (V)5.52[2]
Characteristics
Evolutionary stagehorizontal branch
Spectral typeG5 III[3]
B−Vcolor index1.100±0.015[4]
Astrometry
Radial velocity (Rv)7.0±0.3[4] km/s
Proper motion (μ)RA: +5.874[1]mas/yr
Dec.: −14.102[1]mas/yr
Parallax (π)4.7394±0.1128 mas[1]
Distance690 ± 20 ly
(211 ± 5 pc)
Absolute magnitude (MV)−1.57[4]
Details[5]
Mass3.74+0.38
−0.21
 M
Radius35.27+2.81
−3.81
 R
Luminosity533.48 L
Surface gravity (log g)1.92+0.07
−0.08
 cgs
Temperature4,665+30
−31
 K
Metallicity [Fe/H]−0.17[6] dex
Rotational velocity (v sin i)9.43[6] km/s
Age219+38
−53
 Myr
Other designations
62 Ari,BD+27°500,HD 20825,HIP 15696,HR 1012,SAO 75892[7]
Database references
SIMBADdata

62 Arietis is a single[3]star in the northernconstellation ofAries, a few degrees to the north ofTau Arietis.62 Arietis is theFlamsteed designation. It is visible to the naked eye as a dim, yellow-hued star with anapparent visual magnitude of 5.52.[2] Based upon an annualparallax shift of4.7±0.1 mas,[1] it is approximately 690light-years (210parsecs) distant from the Earth.

This object is an aginggiant star with astellar classification of G5 III,[3] most likely (96% chance) on thehorizontal branch.[5] Having exhausted the supply of hydrogen at itscore, the star has expanded to 35 times theSun's radius. It is around 219 million years old with 3.7 times themass of the Sun. The star is radiating 533 times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,665 K.[5]

Chinese name

[edit]

InChinese astronomy, 62 Arietis is called 天阿,Pinyin: Tiānhé, meaningCelestial River, because this star is marking itself and stand alone inCelestial River asterism,Hairy Head mansion (see :Chinese constellation).[8] 天阿 (Tiānhé) is westernized intoTeen Ho, but according to another opinion about this asterism,Teen Ho is asterism consisting four stars in Aries.[9]

Another "Tiānhé" (Celestial River) inTail mansion, is asterism consisting the stars inOphiuchus[10]

References

[edit]
  1. ^abcdefBrown, 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. ^abRybka, E. (1969), "The corrected magnitudes and colours of 278 stars near S.A. 1-139 in the UBV system",Acta Astronomica,19: 229,Bibcode:1969AcA....19..229R.
  3. ^abcEggleton, 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.
  4. ^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.
  5. ^abcStock, S.; et al. (August 2018), "Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search",Astronomy & Astrophysics,616: 15,arXiv:1805.04094,Bibcode:2018A&A...616A..33S,doi:10.1051/0004-6361/201833111,S2CID 119361866, A33.
  6. ^abHekker, S.; Meléndez, J. (2007), "Precise radial velocities of giant stars. III. Spectroscopic stellar parameters",Astronomy and Astrophysics,475 (3): 1003,arXiv:0709.1145,Bibcode:2007A&A...475.1003H,doi:10.1051/0004-6361:20078233,S2CID 10436552.
  7. ^"62 Ari".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-06-03.
  8. ^zh:白羊座
  9. ^Richard Hinckley Allen: Star Names — Their Lore and Meaning: Aries
  10. ^zh:蛇夫座

External links

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