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Eta2 Doradus

From Wikipedia, the free encyclopedia
Star in the constellation Dorado
For other stars with this Bayer designation, seeη Doradus.
Eta2 Doradus
Observation data
EpochJ2000.0      EquinoxJ2000.0
ConstellationDorado[1]
Right ascension06h 11m 14.98s[2]
Declination−65° 35′ 21.9″[2]
Apparent magnitude (V)5.01[1]
Characteristics
Evolutionary stageAGB[3]
Spectral typeM2.5III[1]
B−Vcolor index1.599[1]
Astrometry
Radial velocity (Rv)+34.5±0.8[1] km/s
Proper motion (μ)RA: −23.823[2]mas/yr
Dec.: +118.639[2]mas/yr
Parallax (π)5.6046±0.1562 mas[2]
Distance580 ± 20 ly
(178 ± 5 pc)
Absolute magnitude (MV)−1.45[1]
Details
Mass1.4[4] M
Radius81.89[2] R
Luminosity1,165[2] L
Surface gravity (log g)1.61[4] cgs
Temperature3,726+313
−154
[2] K
Metallicity[Fe/H]−0.13[4] dex
Other designations
η2 Dor,CPD−65°561,FK5 2473,GC 7946,HD 43455,HIP 29353,HR 2245,SAO 249469,PPM 355229,TYC 8901-1098-1[5]
Database references
SIMBADdata

Eta2 Doradus,Latinized fromη2 Doradus, is astar in the southernconstellation ofDorado. It is visible to the naked eye as a dim, reddish star with anapparent visual magnitude of 5.01[1] It is about 580 light years from the Sun as shown byparallax, and its net movement is one of receding, having aradial velocity of +34.5 km/s.[1] It iscircumpolar south of latitude 24° 24′ S.[6]

This object is anM-typegiant star, with itsstellar classification being M2.5III.[1][7] It has left themain sequence after exhausting its core hydrogen and expanded to around 80 R. The star is radiating about 1,200 times theSun's luminosity from itsphotosphere, at aneffective temperature of3,726 K.[2]

References

[edit]
  1. ^abcdefghiAnderson, 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. XHIP record for this object atVizieR.
  2. ^abcdefghiBrown, 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.
  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. ^abcKhalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G.; Valentini, M.; Torralba Elipe, G.; Steinmetz, M.; Pantaleoni-González, M.; Malhotra, S.; Jiménez-Arranz, Ó.; Enke, H.; Casamiquela, L.; Ardèvol, J. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost".Astronomy and Astrophysics.691: A98.arXiv:2407.06963.Bibcode:2024A&A...691A..98K.doi:10.1051/0004-6361/202451427.
  5. ^"HD 43455".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 25, 2008.
  6. ^"Circumpolar Calculations | Celestial Observation | Space FM".
  7. ^Houk, Nancy (1978),Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan,Bibcode:1975mcts.book.....H.


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