From Wikipedia, the free encyclopedia
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
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]
Distance500 ± 10  ly
(153 ± 4  pc)
Absolute magnitude (MV)−0.41 [3]
Details
Radius35.34+1.13
−2.22
[1]  R
Luminosity333.7±9.9 [1]  L
Surface gravity (log g)1.91 [4]  cgs
Temperature4,070 [4]  K
Metallicity [Fe/H]−0.12 [4]  dex
Other designations
33 Vul, BD+21° 4424, FK5 1549, HD 199697, HIP 103511, HR 8032, SAO 89332 [5]
Database references
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

  1. ^ 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.
  2. ^ 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.
  3. ^ 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.
  4. ^ 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.
  5. ^ "33 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-21.
  6. ^ 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.
  7. ^ 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.
From Wikipedia, the free encyclopedia
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
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]
Distance500 ± 10  ly
(153 ± 4  pc)
Absolute magnitude (MV)−0.41 [3]
Details
Radius35.34+1.13
−2.22
[1]  R
Luminosity333.7±9.9 [1]  L
Surface gravity (log g)1.91 [4]  cgs
Temperature4,070 [4]  K
Metallicity [Fe/H]−0.12 [4]  dex
Other designations
33 Vul, BD+21° 4424, FK5 1549, HD 199697, HIP 103511, HR 8032, SAO 89332 [5]
Database references
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

  1. ^ 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.
  2. ^ 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.
  3. ^ 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.
  4. ^ 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.
  5. ^ "33 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-04-21.
  6. ^ 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.
  7. ^ 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.

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