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32 Vulpeculae

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Star in the constellation Vulpecula
32 Vulpeculae
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vulpecula
Right ascension 20 54 33.63782
Declination +28° 03′ 27.4632″
Apparent magnitude (V) 5.03 (4.99–5.06)
Characteristics
Evolutionary stage giant
Spectral type K4 III
B−V color index 1.480
Variable type suspected
Astrometry
Radial velocity (Rv)+5.7±0.6 km/s
Proper motion (μ) RA: −2.525±0.209 mas/yr
Dec.: −2.277±0.197 mas/yr
Parallax (π)5.3885 ± 0.1260 mas
Distance610 ± 10 ly
(186 ± 4 pc)
Absolute magnitude (MV)−1.76
Details
Radius54.29+1.69
−3.42 R
Luminosity708.4±19.5 L
Surface gravity (log g)1.74 cgs
Temperature4,041+134
−61 K
Metallicity −0.16 dex
Rotational velocity (v sin i)8.1 km/s
Other designations
32 Vul, NSV 13398, BD+27° 3911, FK5 786, GC 29178, HD 199169, HIP 103200, HR 8008, SAO 89272
Database references
SIMBADdata

32 Vulpeculae is a single star located around 610 light years away from the Sun in the northern constellation Vulpecula, a few degrees south of the border with Cygnus. It is visible to the naked eye as a faint, orange-hued star with a typical apparent visual magnitude of 5.03. This object is drifting further away from the Earth with a heliocentric radial velocity of +6 km/s.

This is an aging red giant star with a stellar classification of K4 III, having exhausted the supply of hydrogen at its core then expanded to 54 times the Sun's radius. It is a suspected variable of unknown type, with a visual magnitude that has been measured ranging from 4.99 down to 5.06. The star is radiating 708 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,041 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. ^ 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.
  3. ^ Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
  4. ^ Ryon, Jenna; et al. (August 2009), "Comparing the Ca ii H and K Emission Lines in Red Giant Stars", Publications of the Astronomical Society of the Pacific, 121 (882): 842, arXiv:0907.3346, Bibcode:2009PASP..121..842R, doi:10.1086/605456, S2CID 17821279.
  5. ^ Roman, Nancy G. (July 1952), "The Spectra of the Bright Stars of Types F5-K5", Astrophysical Journal, 116: 122, Bibcode:1952ApJ...116..122R, doi:10.1086/145598.
  6. ^ McWilliam, Andrew (December 1990), "High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances", Astrophysical Journal Supplement Series, 74: 1075–1128, Bibcode:1990ApJS...74.1075M, doi:10.1086/191527.
  7. ^ "32 Vul". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-11-17.
  8. Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
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