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19 Vulpeculae

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Star in the constellation Vulpecula
19 Vulpeculae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vulpecula
Right ascension 20 11 47.9738
Declination 26° 48′ 32.3736″
Apparent magnitude (V) 5.40
Characteristics
Spectral type K2 IIIa
B−V color index 1.40
Astrometry
Radial velocity (Rv)−19.33±0.11 km/s
Proper motion (μ) RA: 1.619±0.119 mas/yr
Dec.: −10.600±0.122 mas/yr
Parallax (π)1.9328 ± 0.0779 mas
Distance1,690 ± 70 ly
(520 ± 20 pc)
Absolute magnitude (MV)−2.60
Details
Mass4.94±0.53 M
Radius100.3+1.7
−3.0 R
Luminosity2,889±145 L
Surface gravity (log g)1.40 cgs
Temperature4,200 K
Metallicity −0.01 dex
Rotational velocity (v sin i)< 3.4 km/s
Other designations
19 Vul, BD+26° 3825, HD 192004, HIP 99518, HR 7718, SAO 88330
Database references
SIMBADdata

19 Vulpeculae is star located approximately 1,690 light years from Earth in the northern constellation of Vulpecula. It is a probable member of the open cluster NGC 6882. This object is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.40. It is moving closer to the Earth with a heliocentric radial velocity of −19 km/s.

This is an aging giant star with a stellar classification of K2 IIIa, having already consumed the hydrogen at its core and evolved away from the main sequence. It has nearly five times the mass of the Sun but has expanded to around 100 times the Sun's radius. The star is radiating 2,889 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,200 K.

References

  1. ^ 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. ^ Fernie, J. D. (1983). "New UBVRI photometry for 900 supergiants". Astrophysical Journal Supplement Series. 52: 7. Bibcode:1983ApJS...52....7F. doi:10.1086/190856.
  3. ^ 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.
  4. ^ Mermilliod, J. C.; et al. (2008). "Red giants in open clusters. XIV. Mean radial velocities for 1309 stars and 166 open clusters". Astronomy & Astrophysics. 485 (1): 303–314. Bibcode:2008A&A...485..303M. CiteSeerX 10.1.1.30.7545. doi:10.1051/0004-6361:200809664.
  5. 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.
  6. ^ Hohle, M.M.; et al. (2010). "Masses and luminosities of O- and B-type stars and red supergiants". Astronomische Nachrichten. 331 (4): 349. arXiv:1003.2335. Bibcode:2010AN....331..349H. doi:10.1002/asna.200911355. S2CID 111387483.
  7. ^ Luck, R. Earle (March 1994). "Open Cluster Chemical Composition. I. Later Type Stars in Eight Clusters". Astrophysical Journal Supplement. 91: 309. Bibcode:1994ApJS...91..309L. doi:10.1086/191940.
  8. De Medeiros, J. R.; et al. (November 2000). "Rotation and lithium in single giant stars". Astronomy and Astrophysics. 363: 239–243. arXiv:astro-ph/0010273. Bibcode:2000A&A...363..239D.
  9. ^ "19 Vulpeculae". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-11-18.

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