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HD 73389

From Wikipedia, the free encyclopedia
Binary star system in the constellation Carina
This article is about e2 Carinae. For e1 Carinae, seeHD 73390. For E Carinae, seeV345 Carinae.
Not to be confused withε Carinae.
HD 73389
Observation data
Epoch J2000      Equinox J2000
ConstellationCarina
Right ascension08h 35m 19.70886s[1]
Declination−58° 00′ 33.2714″[1]
Apparent magnitude (V)+4.84[2](5.08 + 8.02)[3]
Characteristics
Spectral typeK0III[4]
B−Vcolor index0.981±0.041[2]
Astrometry
Radial velocity (Rv)+25.62±0.13[1] km/s
Proper motion (μ)RA: +52.848±0.555[1]mas/yr
Dec.: +28.117±0.491[1]mas/yr
Parallax (π)14.5139±0.2692 mas[1]
Distance225 ± 4 ly
(69 ± 1 pc)
Absolute magnitude (MV)0.68[2]
Details
A
Radius11.13+1.11
−0.39
[1] R
Luminosity64.4±1.4[1] L
Temperature4,903+87
−229
[1] K
Other designations
e2 Car,CPD−57°1591,GC 11797,HD 73389,HIP 42134,HR 3414,SAO 236106,CCDM J08353-5801[5]
Database references
SIMBADdata

HD 73389 is abinary star[3] system in theconstellationCarina. It has theBayer designatione2 Carinae;HD 73389 is the identifier from theHenry Draper Catalogue. This system is visible to the naked eye as a point of light with a combinedapparent visual magnitude of +4.84.[2] Based onparallax measurements, it is located at a distance of approximately 225 light years from theSun. The system is drifting further away with aradial velocity of +25.6 km/s.[1]

The visual magnitude 5.08 primary, component A, is an agingK-typegiant star with astellar classification of K0III.[4] With the supply of hydrogen at itscore exhausted, it has cooled and expanded to 11 times theSun's radius.[1] It is radiating 64 times theluminosity of the Sun from its enlargedphotosphere at aneffective temperature of 4,903 K.[1] The secondary companion, component B, has avisual magnitude of 8.02 and is located at anangular separation of0.30 along aposition angle of 207° from the primary, as of 2015.[6]

References

[edit]
  1. ^abcdefghijklBrown, 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. ^abcdAnderson, 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.
  3. ^abEggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2): 869,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  4. ^abHouk, 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.
  5. ^"HD 73389".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-07-11.
  6. ^Mason, B. D.; et al. (2014),"The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920, retrieved2015-07-22
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