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50 Cassiopeiae

50 Cassiopeiae is a white star in the northern constellation of Cassiopeia. In the past, it had been misidentified as a suspected nebula, and given the number NGC 771.[9] The star is visible to the naked eye, having an apparent visual magnitude of +3.95.[2] Based upon an annual parallax shift of 20.76 mas, it is located 157 light years away. It is moving closer, having a heliocentric radial velocity of −18 km/s,[4] and will approach to within 82 ly in 1.879 million years.[2]

50 Cassiopeiae

50 Cassiopeiae in optical light
Observation data
Epoch J2000      Equinox J2000
Constellation Cassiopeia
Right ascension 02h 03m 26.10206s[1]
Declination +72° 25′ 16.6376″[1]
Apparent magnitude (V) +3.95[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A2 V[3]
B−V color 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
A light curve for 50 Cassiopeiae, plotted from TESS data[10]

It is an A-type main-sequence star with a stellar 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 the mass of the Sun,[3] and about 2.5 times the Sun's radius.[6] It is radiating 64 times the Sun's luminosity from its photosphere at an effective temperature of around 9,376 K.[3]

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

References Edit

  1. ^ a b 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.
  2. ^ a b c d e Anderson, 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. ^ a b c d e f g h i Zorec, 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. ^ a b de 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. ^ a b c 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.
  6. ^ a b Pasinetti 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. Retrieved 2018-06-25.
  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, retrieved 8 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

External links Edit

  • "DOCdb page for 50 Cas". Retrieved 2016-12-09.

cassiopeiae, white, star, northern, constellation, cassiopeia, past, been, misidentified, suspected, nebula, given, number, star, visible, naked, having, apparent, visual, magnitude, based, upon, annual, parallax, shift, located, light, years, away, moving, cl. 50 Cassiopeiae is a white star in the northern constellation of Cassiopeia In the past it had been misidentified as a suspected nebula and given the number NGC 771 9 The star is visible to the naked eye having an apparent visual magnitude of 3 95 2 Based upon an annual parallax shift of 20 76 mas it is located 157 light years away It is moving closer having a heliocentric radial velocity of 18 km s 4 and will approach to within 82 ly in 1 879 million years 2 50 Cassiopeiae50 Cassiopeiae in optical lightObservation dataEpoch J2000 Equinox J2000Constellation CassiopeiaRight ascension 02h 03m 26 10206s 1 Declination 72 25 16 6376 1 Apparent magnitude V 3 95 2 CharacteristicsEvolutionary stage main sequence 3 Spectral type A2 V 3 B V color index 0 002 0 007 2 AstrometryRadial velocity Rv 18 2 0 9 4 km sProper motion m RA 43 57 5 mas yr Dec 22 30 5 mas yrParallax p 20 76 0 14 mas 5 Distance157 1 ly 48 2 0 3 pc Absolute magnitude MV 0 54 2 DetailsMass2 56 0 03 3 M Radius2 5 6 R Luminosity63 8 3 5 6 4 3 L Temperature9 376 240 235 3 KMetallicity Fe H 0 18 0 28 7 dexRotational velocity v sin i 91 3 km sOther designations50 Cas BD 71 117 FK5 70 GC 2445 HD 12216 HIP 9598 HR 580 SAO 4560 NGC 771 8 Database referencesSIMBADdata A light curve for 50 Cassiopeiae plotted from TESS data 10 It is an A type main sequence star with a stellar 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 the mass of the Sun 3 and about 2 5 times the Sun s radius 6 It is radiating 64 times the Sun s luminosity from its photosphere at an effective temperature of around 9 376 K 3 The star was the brightest star in the occasionally used 1775 to 19th century constellation Custos Messium typically drawn as a depiction of Charles Messier standing on top of the giraffe Camelopardus between Cepheus and Cassiopeia 12 References Edit a b Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 a b c d e Anderson 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 a b c d e f g h i Zorec J Royer F 2012 Rotational velocities of A type stars IV Evolution of rotational velocities Astronomy amp Astrophysics 537 A120 arXiv 1201 2052 Bibcode 2012A amp A 537A 120Z doi 10 1051 0004 6361 201117691 S2CID 55586789 a b de Bruijne J H J Eilers A C October 2012 Radial velocities for the HIPPARCOS Gaia Hundred Thousand Proper Motion project Astronomy amp Astrophysics 546 14 arXiv 1208 3048 Bibcode 2012A amp A 546A 61D doi 10 1051 0004 6361 201219219 S2CID 59451347 A61 a b c Van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 a b Pasinetti 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 amp A 367 521P doi 10 1051 0004 6361 20000451 S2CID 425754 Gaspar Andras 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 50 Cas SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2018 06 25 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 MAST Barbara A Mikulski Archive for Space Telescopes Space Telescope Science Institute retrieved 8 December 2021 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 Ian Ridpath s Star Tales Custos MessiumExternal links Edit DOCdb page for 50 Cas Retrieved 2016 12 09 Retrieved from https en wikipedia org w index php title 50 Cassiopeiae amp oldid 1114697078, wikipedia, wiki, book, books, library,

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