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49 Cassiopeiae

From Wikipedia, the free encyclopedia
Binary star system in the constellation Cassiopeia
49 Cassiopeiae
Location of 49 Cassiopeiae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationCassiopeia[1]
49 Cas A
Right ascension02h 05m 31.55013s[2]
Declination+76° 06′ 54.2164″[2]
Apparent magnitude (V)5.32[3]
49 Cas B
Right ascension02h 05m 30.09074s[4]
Declination+76° 06′ 51.9730″[4]
Apparent magnitude (V)12.30[3]
Characteristics
49 Cas A
Evolutionary stagehorizontal branch[5]
Spectral typeG8III[6]
B−Vcolor index0.954±0.003[7]
Astrometry
49 Cas A
Radial velocity (Rv)−0.20±0.30[7] km/s
Proper motion (μ)RA: −11.813[2]mas/yr
Dec.: −20.561[2]mas/yr
Parallax (π)7.6673±0.0700 mas[2]
Distance425 ± 4 ly
(130 ± 1 pc)
Absolute magnitude (MV)−0.44[8]
49 Cas B
Proper motion (μ)RA: −13.572[4]mas/yr
Dec.: −19.339[4]mas/yr
Parallax (π)7.9161±0.0228 mas[4]
Distance412 ± 1 ly
(126.3 ± 0.4 pc)
Details
49 Cas A
Mass2.6[9] M
Radius16.6[2] R
Luminosity140[2] L
Surface gravity (log g)2.66[9] cgs
Temperature5,087[10] K
Metallicity[Fe/H]−0.04[10] dex
Rotational velocity (v sin i)1.2[11] km/s
Age647[10] Myr
49 Cas B
Mass0.81[4] M
Radius0.76[4] R
Luminosity0.28[4] L
Surface gravity (log g)4.59[4] cgs
Temperature4,886[4] K
Age1.6[4] Gyr
Other designations
Rangifer,49 Cas,BD+75°86,GC 2475,HD 12339,HIP 9763,HR 592,SAO 4565,CCDM J02056+7607,GSC 04495-01881[12]
Database references
SIMBADdata

49 Cassiopeiae, also namedRangifer,[13] is abinary star[14] system in the northerncircumpolar constellation ofCassiopeia. It is visible to the naked eye as a faint, yellow-hued point of light with anapparent visual magnitude of 5.22.[7] The system is located about 412 light years away from the Sun, based onparallax. The pair had anangular separation of5.40 along aposition angle of 244°, as of 2008, with the brighter component being of magnitude 5.32 and its faint companion having magnitude 12.30.[3]

The primary, designated component A,[3] is an aginggiant star with astellar classification of G8III.[6] It is 302 million years old with 3.3 times themass of the Sun.[8] With the supply of hydrogen at itscore exhausted, the star has now expanded to 17 times theSun's radius. It is ared clump giant on thehorizontal branch, which indicates it is generating energy through the fusion of helium at its core.[5] The star is radiating 140 times theluminosity of the Sun from its swollenphotosphere at aneffective temperature of5,087 K. Its faint secondary companion, component B, is of an unknown spectral type. It has a temperature similar to the primary, but a luminosity much lower than the Sun's.

This star was part of the now-obsolete constellationRangifer, the reindeer, which was also called Tarandus. Both words meanreindeer in Latin, and they form the reindeer's scientific name,Rangifer tarandus. TheIAU Working Group on Star Names approved the name Rangifer for this star on 25 December 2025, and it is now so entered in the IAU Catalog of Star Names.2 Ursae Minoris was namedTarandus.[13]

References

[edit]
  1. ^Anderson, E.; Francis, Ch. (May 2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5):331–346,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,eISSN 1562-6873,ISSN 1063-7737,S2CID 119257644.
  2. ^abcdefgVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdMason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog",The Astronomical Journal,122 (6):3466–3471,Bibcode:2001AJ....122.3466M,doi:10.1086/323920
  4. ^abcdefghijkVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  5. ^abAlves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity",The Astrophysical Journal,539 (2):732–741,arXiv:astro-ph/0003329,Bibcode:2000ApJ...539..732A,doi:10.1086/309278,S2CID 16673121.
  6. ^abAbt, Helmut A. (2008), "Visual Multiples. IX. MK Spectral Types",The Astrophysical Journal Supplement Series,176 (1):216–217,Bibcode:2008ApJS..176..216A,doi:10.1086/525529.
  7. ^abcAnderson, 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.
  8. ^abTakeda, Yoichi; et al. (August 2008), "Stellar Parameters and Elemental Abundances of Late-G Giants",Publications of the Astronomical Society of Japan,60 (4):781–802,arXiv:0805.2434,Bibcode:2008PASJ...60..781T,doi:10.1093/pasj/60.4.781,S2CID 16258166.
  9. ^abQueiroz, A. B. A.; Anders, F.; Chiappini, C.; Khalatyan, A.; Santiago, B. X.; Steinmetz, M.; Valentini, M.; Miglio, A.; Bossini, D.; Barbuy, B.; Minchev, I.; Minniti, D.; García Hernández, D. A.; Schultheis, M.; Beaton, R. L.; Beers, T. C.; Bizyaev, D.; Brownstein, J. R.; Cunha, K.; Fernández-Trincado, J. G.; Frinchaboy, P. M.; Lane, R. R.; Majewski, S. R.; Nataf, D.; Nitschelm, C.; Pan, K.; Roman-Lopes, A.; Sobeck, J. S.; Stringfellow, G.; Zamora, O. (2020), "From the bulge to the outer disc: StarHorse stellar parameters, distances, and extinctions for stars in APOGEE DR16 and other spectroscopic surveys",Astronomy and Astrophysics,638: A76,arXiv:1912.09778,Bibcode:2020A&A...638A..76Q,doi:10.1051/0004-6361/201937364,S2CID 209439697.
  10. ^abcTing, Yuan-Sen; Rix, Hans-Walter (2019), "The Vertical Motion History of Disk Stars throughout the Galaxy",The Astrophysical Journal,878 (1): 21,arXiv:1808.03278,Bibcode:2019ApJ...878...21T,doi:10.3847/1538-4357/ab1ea5,S2CID 119211560.
  11. ^Glebocki, R.; Gnacinski, P. (2005), "VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005)",VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G,3244,Bibcode:2005yCat.3244....0G.
  12. ^"49 Cas".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-07-22.
  13. ^ab"IAU Catalog of Star Names". Retrieved28 December 2025.
  14. ^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.
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