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Kappa Normae

From Wikipedia, the free encyclopedia
Star in the constellation Norma
Kappa Normae
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationNorma
Right ascension16h 13m 28.72874s[1]
Declination−54° 37′ 49.6860″[1]
Apparent magnitude (V)4.94[2]
Characteristics
Spectral typeG8 III[3]
U−Bcolor index+0.81[2]
B−Vcolor index+1.04[2]
Astrometry
Radial velocity (Rv)−13.5±0.8[4] km/s
Proper motion (μ)RA: −3.845[1]mas/yr
Dec.: −22.366[1]mas/yr
Parallax (π)7.4386±0.2471 mas[1]
Distance440 ± 10 ly
(134 ± 4 pc)
Absolute magnitude (MV)−0.64[5]
Details
Radius21.8+0.6
−1.5
[1] R
Luminosity225.7±8.5[1] L
Temperature4,787+173
−69
[1] K
Other designations
κ Nor,CD−54° 6604,FK5 600,HD 145397,HIP 79509,HR 6024,SAO 243454,WDS J16135-5438A[6]
Database references
SIMBADdata

Kappa Normae,Latinized fromκ Normae, is a solitary,[7] yellow huedstar in the southernconstellation ofNorma. Itsapparent magnitude is 4.94,[2] which is bright enough to be faintly visible to the naked eye. Based upon an annualparallax shift of7.44 mas as seen from Earth,[8] the system is located about 440 light years from theSun. It is drifting closer with aradial velocity of 13.5 km/s.[4]

This is anevolvedgiant star with astellar classification of G8III[3] that has swollen and cooled off themain sequence. At present it has 22[1] times theradius of the Sun. It shines with aluminosity approximately 226 times that of the Sun and has aneffective temperature of 4,787 K.[1]

References

[edit]
  1. ^abcdefghijBrown, 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. ^abcdLodén, L. O.; Nordström, B. (1969), "Photometric standard sequences in Norma iII = 320° − 340°",Arkiv för Astronomi,5:231–239,Bibcode:1969ArA.....5..231L.
  3. ^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.
  4. ^abde Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics,546: 14,arXiv:1208.3048,Bibcode:2012A&A...546A..61D,doi:10.1051/0004-6361/201219219,S2CID 59451347, A61.
  5. ^Anderson, 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.
  6. ^"kap Nor".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2017-08-11.{{cite web}}: CS1 maint: postscript (link)
  7. ^Eggleton, 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.
  8. ^van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
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