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HD 16028

From Wikipedia, the free encyclopedia
Orange giant star in the constellation Andromeda
HD 16028
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension02h 35m 38.7415s[1]
Declination+37° 18′ 44.1425″[1]
Apparent magnitude (V)5.71[2]
Characteristics
Spectral typeK3III[3]
B−Vcolor index1.41[2]
Astrometry
Radial velocity (Rv)−5.48±0.20[1] km/s
Proper motion (μ)RA: −1.454±0.217[1]mas/yr
Dec.: −13.822±0.177[1]mas/yr
Parallax (π)4.4409±0.1180 mas[1]
Distance730 ± 20 ly
(225 ± 6 pc)
Details[4]
Luminosity299.05 L
Temperature4,371 K
Other designations
BD+36° 519,SAO 55684,HIP 12072,HR 748.
Database references
SIMBADdata

HD 16028 is astar in the constellationAndromeda. Its apparent magnitude is 5.71.[2] Located approximately 225 parsecs (730 ly) distant,[1] it is anorange giant of spectral type K3III,[3] a star that has used up its corehydrogen and has expanded.

Double star catalogues list two stars as optical companions. One has a magnitude of 10.9 and is separated by 16.9arcseconds. It has been suggested it is related to the primary,[3] butparallax measured byGaia yields a much greater distance for this star in comparison to HD 16028.[5] The other is even fainter and is separated 45 arcseconds from the primary.[6]

References

[edit]
  1. ^abcdefgBrown, 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. ^abcHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000), "The Tycho-2 catalogue of the 2.5 million brightest stars",Astronomy & Astrophysics,355:L27 –L30,Bibcode:2000A&A...355L..27H.
  3. ^abcEggleton, 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. ^McDonald, I.; Zijlstra, A. A.; et al. (2012), "Fundamental parameters and infrared excesses of Hipparcos stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–357,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  5. ^Brown, 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.
  6. ^"UCAC4 637-009202".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedJanuary 3, 2019.
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