Jump to content

62 Andromedae

From Wikipedia, the free encyclopedia
(Redirected from C Andromedae)
62 Andromedae
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 02h 19m 16.79693s[1]
Declination +47° 22′ 47.9132″[1]
Apparent magnitude (V) 5.31[2]
Characteristics
Spectral type A0V[3]
B−V color index 0.00425[4]
Astrometry
Radial velocity (Rv)−29.6±2.8[5] km/s
Proper motion (μ) RA: –60.03[6] mas/yr
Dec.: –5.61[6] mas/yr
Parallax (π)11.9531 ± 0.1640 mas[1]
Distance273 ± 4 ly
(84 ± 1 pc)
Absolute magnitude (MV)0.93[7]
Details
Mass2.42±0.02[8] M☉
Radius1.8[2] R☉
Luminosity45.2+2.1
−1.9[8] L☉
Temperature9,572+133
−131[8] K
Rotational velocity (v sin i)86[9] km/s
Other designations
c Andromedae[10], 62 And, BD+46°552, FK5 1063, HD 14212, HIP 10819, HR 670, SAO 37948, PPM 44986[11]
Database references
SIMBADdata

62 Andromedae, abbreviated 62 And, is a single[12] star in the northern constellation Andromeda. 62 Andromedae is the Flamsteed designation; it also bears the Bayer designation of c Andromedae.[10] It is bright enough to be seen by the naked eye, with an apparent magnitude of 5.31. Based upon parallax measurements made during the Gaia mission, it is at a distance of roughly 273 light-years (84 parsecs) from Earth.[1] The star is moving closer to the Earth with a heliocentric radial velocity of −30 km/s,[5] and is predicted to come to within 144.6 light-years in 1,6 million years.[7]

This is an A-type main-sequence star with a stellar classification of A0 V.[13] Abt and Morrel (1995) gave it a class of A1 III,[14][7] matching a more evolved giant star. The star has 2.42[8] times the mass of the Sun, about 1.8[2] times the Sun's radius, and is spinning with a projected rotational velocity of 86 km/s.[8] It is radiating 45[8] times the Sun's luminosity from its photosphere at an effective temperature of 9,572 K.[8]

References

[edit]
  1. ^ a b c d 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 Pasinetti Fracassini, L. E.; Pastori, L.; Covino, S.; Pozzi, A. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy & Astrophysics, 367 (2): 521–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451.
  3. ^ van Belle, Gerard T.; von Braun, Kaspar (2009), "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars", The Astrophysical Journal, 694 (2): 1085–1098, arXiv:0901.1206, Bibcode:2009ApJ...694.1085V, doi:10.1088/0004-637X/694/2/1085, S2CID 18370219.
  4. ^ Høg, 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.
  5. ^ 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.
  6. ^ a b 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.Vizier catalog entry
  7. ^ a b c 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.
  8. ^ a b c d e f g 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, A120.
  9. ^ Royer, F.; et al. (2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy & Astrophysics, 393 (3): 897–911, arXiv:1201.2052, Bibcode:2002A&A...393..897R, doi:10.1051/0004-6361:20020943, S2CID 14070763.
  10. ^ a b Tirion, Wil; Rappaport, Barry (1987), Remaklus, Will (ed.), Uranometria 2000.0 - Volume II - The Southern Hemisphere to +6°, Richmond, Virginia, USA, ISBN 0-943396-15-8.
  11. ^ "62 And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved October 4, 2018.
  12. ^ 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.
  13. ^ van Belle, Gerard T.; von Braun, Kaspar (2009), "Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars", The Astrophysical Journal (abstract), 694 (2): 1085–1098, arXiv:0901.1206, Bibcode:2009ApJ...694.1085V, doi:10.1088/0004-637X/694/2/1085, S2CID 18370219
  14. ^ Abt, Helmut A.; Morrell, Nidia I. (July 1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars", Astrophysical Journal Supplement, 99: 135, Bibcode:1995ApJS...99..135A, doi:10.1086/192182.
Retrieved from "https://en.wikipedia.org/w/index.php?title=62_Andromedae&oldid=1241452385"