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Zeta2 Antliae

From Wikipedia, the free encyclopedia
Star in the constellation Antlia
For other stars with this designation, seeZeta Antliae.
Zeta2 Antliae
Location of ζ2 Antliae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAntlia
Right ascension09h 31m 32.155s[1]
Declination−31° 52′ 18.52″[1]
Apparent magnitude (V)5.91[2]
Characteristics
Spectral typeA9 IV[3]
U−Bcolor index+0.16[2]
B−Vcolor index+0.23[2]
Astrometry
Radial velocity (Rv)+19.8±1.6[4] km/s
Proper motion (μ)RA: −46.727mas/yr[1]
Dec.: −9.036mas/yr[1]
Parallax (π)8.8101±0.0593 mas[1]
Distance370 ± 2 ly
(113.5 ± 0.8 pc)
Absolute magnitude (MV)+0.44[5]
Details
Mass1.71[6] M
Radius4.22[6] R
Luminosity49.5[6] L
Surface gravity (log g)3.42[6] cgs
Temperature7,455[6] K
Other designations
ζ2 Antliae, Zet2 Ant, ζ2 Ant,CD−31 7369,HD 82513,HIP 46734,HR 3789,SAO 200459,PPM 286565[7]
Database references
SIMBADdata

Zeta2 Antliae is a star in the southernconstellation ofAntlia, the air pump. ItsBayer designation isLatinized from ζ2 Antliae, and abbreviated Zet2 Ant or ζ2 Ant, respectively. With anapparent visual magnitude of 5.91,[2] it is a relatively faint star that requiresdark suburban skies for viewing with thenaked eye.Parallax measurements show it to be located at a distance of approximately 370light-years (110parsecs) from Earth.[1] The star is receding with a heliocentricradial velocity of +20 km/s.[4]

Thespectrum of this star matches astellar classification of A9 IV,[3] where theluminosity class of IV indicates that this is asubgiant star that isevolving away from themain sequence as the supply of hydrogen at its core is becoming exhausted. This is catalogued as anAm star, which means it is achemically peculiar star that shows strong indications of certain tracemetals in its spectrum.[5] However, the chemical peculiarity is now considered doubtful.[8] The star has 1.7 times the mass and 4.2 times the radius of the Sun. It is radiating 49.5 times the luminosity of the Sun from itsphotosphere at aneffective temperature of 7,455 K.[6]

References

[edit]
  1. ^abcdeBrown, A. G. A.; et al. (Gaia collaboration) (2021)."Gaia Early Data Release 3: Summary of the contents and survey properties".Astronomy & Astrophysics.649: A1.arXiv:2012.01533.Bibcode:2021A&A...649A...1G.doi:10.1051/0004-6361/202039657.S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source atVizieR.
  2. ^abcdMendoza, E. E.; Gomez, V. T.; Gonzalez, S. (June 1978), "UBVRI photometry of 225 Am stars",The Astronomical Journal,83:606–614,Bibcode:1978AJ.....83..606M,doi:10.1086/112242.
  3. ^abHouk, Nancy (1979),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan,Bibcode:1982mcts.book.....H.
  4. ^abGontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  5. ^abHauck, B.; Curchod, A. (December 1980), "Properties of AM stars in the Geneva photometric system",Astronomy and Astrophysics,92 (3):289–295,Bibcode:1980A&A....92..289H.
  6. ^abcdefStassun K.G.; et al. (October 2019), "The revised TESS Input Catalog and Candidate Target List",The Astronomical Journal,158 (4): 138,arXiv:1905.10694,Bibcode:2019AJ....158..138S,doi:10.3847/1538-3881/ab3467,S2CID 166227927.
  7. ^"zet02 Ant".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-06-27.
  8. ^Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars",Astronomy and Astrophysics,498 (3):961–966,Bibcode:2009A&A...498..961R,doi:10.1051/0004-6361/200810788.

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