Star in the constellation Vulpecula
33 Vulpeculae Observation data Epoch J2000 Equinox J2000 |
Constellation | Vulpecula |
Right ascension | 20h 58m 16.34942s[1] |
Declination | +22° 19′ 33.2638″[1] |
Apparent magnitude (V) | 5.31[2] |
Characteristics |
Spectral type | K3.5 III[2] |
B−V color index | 1.419±0.005[3] |
Astrometry |
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Radial velocity (Rv) | −25.23±0.24[3] km/s |
Proper motion (μ) | RA: −2.327[1] mas/yr Dec.: −4.511[1] mas/yr |
Parallax (π) | 6.5257 ± 0.1689 mas[1] |
Distance | 500 ± 10 ly (153 ± 4 pc) |
Absolute magnitude (MV) | −0.41[3] |
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Details |
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Radius | 35.34+1.13 −2.22[1] R☉ |
Luminosity | 333.7±9.9[1] L☉ |
Surface gravity (log g) | 1.91[4] cgs |
Temperature | 4,070[4] K |
Metallicity [Fe/H] | −0.12[4] dex |
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Other designations |
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Database references |
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SIMBAD | data |
33 Vulpeculae is a single[6] star located around 500 light-years away from the Sun in the northern constellation of Vulpecula. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.31.[2] The object is drifting closer to the Earth with a heliocentric radial velocity of −25 km/s.[3]
This is an evolved giant star with a stellar classification of K3.5 III,[2] having exhausted the supply of hydrogen at it its core and expanded to 35[1] times the Sun's radius. It serves as a spectral standard for stars of its particular class.[7] This star is radiating 334[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,070 K.[4]
References
- ^ a b c d e f g h i 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. Gaia DR2 record for this source at VizieR.
- ^ a b c d Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373.
- ^ a b c d 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.
- ^ a b c d Soubiran, C.; et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv:1004.1069, Bibcode:2010A&A...515A.111S, doi:10.1051/0004-6361/201014247, S2CID 118362423.
- ^ "33 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-21.
- ^ 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.
- ^ Keenan, P. C.; Yorka, S. B. (1988), "1988 Revised MK Spectral Standards for Stars GO and Later", Bulletin d'Information du Centre de Données Stellaires, 35: 37, Bibcode:1988BICDS..35...37K.
External links
- 33 Vulpeculae on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
Constellation of Vulpecula
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Stars | Bayer | |
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Flamsteed | |
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Variable | |
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HR | - 7207
- 7250
- 7263
- 7286
- 7364
- 7384
- 7391
- 7421
- 7452
- 7472
- 7490
- 7540
- 7556
- 7573
- 7601
- 7656
- 7716
- 7760
- 7811
- 7849
- 7862
- 7895
- 7903
- 8082
- 8158
- 8190
- 8194
- 8197
- 8198
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HD | |
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Other | |
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Galaxies | |
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![](//upload.wikimedia.org/wikipedia/en/thumb/9/96/Symbol_category_class.svg/16px-Symbol_category_class.svg.png) Category |