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50 Cassiopeiae

From Wikipedia, the free encyclopedia
Star in the constellation Cassiopeia
50 Cassiopeiae

50 Cassiopeiae in optical light
Observation data
Epoch J2000      Equinox J2000
ConstellationCassiopeia
Right ascension02h 03m 26.10206s[1]
Declination+72° 25′ 16.6376″[1]
Apparent magnitude (V)+3.95[2]
Characteristics
Evolutionary stagemain sequence[3]
Spectral typeA2 V[3]
B−Vcolor index−0.002±0.007[2]
Astrometry
Radial velocity (Rv)−18.2±0.9[4] km/s
Proper motion (μ)RA: −43.57[5]mas/yr
Dec.: +22.30[5]mas/yr
Parallax (π)20.76±0.14 mas[5]
Distance157 ± 1 ly
(48.2 ± 0.3 pc)
Absolute magnitude (MV)0.54[2]
Details
Mass2.56±0.03[3] M
Radius2.5[6] R
Luminosity63.8+3.5
−6.4
[3] L
Temperature9,376+240
−235
[3] K
Metallicity [Fe/H]+0.18±0.28[7] dex
Rotational velocity (v sin i)91[3] km/s
Other designations
50 Cas,BD+71°117,FK5 70,GC 2445,HD 12216,HIP 9598,HR 580,SAO 4560,NGC 771[8]
Database references
SIMBADdata

50 Cassiopeiae is a whitestar in the northernconstellation ofCassiopeia. In the past, it had been misidentified as a suspectednebula, and given the numberNGC 771.[9] The star is visible to the naked eye, having anapparent visual magnitude of +3.95.[2] Based upon an annualparallax shift of20.76 mas, it is located 157 light years away. It is moving closer, having a heliocentricradial velocity of −18 km/s,[4] and will approach to within 82 ly in 1.879 million years.[2]

Alight curve for 50 Cassiopeiae, plotted fromTESS data[10]

It is anA-type main-sequence star with astellar classification of A2 V.[3] It is a suspected variable star with a very small amplitude.[11] 50 Cas has an estimated 2.56 times themass of the Sun,[3] and about 2.5 times theSun's radius.[6] It is radiating 64 times theSun's luminosity from itsphotosphere at aneffective temperature of around 9,376 K.[3]

The star was the brightest star in the occasionally used 1775 to 19th century constellationCustos Messium, typically drawn as a depiction of Charles Messier standing on top of the giraffe (Camelopardus), betweenCepheus and Cassiopeia.[12]

References

[edit]
  1. ^abBrown, 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.
  2. ^abcdeAnderson, E.; Francis, C (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. ^abcdefghiZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  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. ^abcVan 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.
  6. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics",Astronomy and Astrophysics,367 (2):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  7. ^Gáspár, András; et al. (August 2016), "The Correlation between Metallicity and Debris Disk Mass",The Astrophysical Journal,826 (2): 14,arXiv:1604.07403,Bibcode:2016ApJ...826..171G,doi:10.3847/0004-637X/826/2/171,S2CID 119241004, 171.
  8. ^"50 Cas".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-06-25.
  9. ^Wolfgang Steinicke (19 August 2010).Observing and Cataloguing Nebulae and Star Clusters: From Herschel to Dreyer's New General Catalogue. Cambridge University Press.ISBN 978-1-139-49010-8.
  10. ^MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved8 December 2021.
  11. ^Koen, Chris; Eyer, Laurent (2002)."New periodic variables from the Hipparcos epoch photometry".Monthly Notices of the Royal Astronomical Society.331 (1):45–59.arXiv:astro-ph/0112194.Bibcode:2002MNRAS.331...45K.doi:10.1046/j.1365-8711.2002.05150.x.S2CID 10505995.
  12. ^Ian Ridpath's Star Tales - Custos Messium

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