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62 Aquilae

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(Redirected from 62 Aql) Star in the constellation Aquila
62 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20 04 23.15129
Declination −00° 42′ 33.5147″
Apparent magnitude (V) 5.67
Characteristics
Spectral type K4 III
B−V color index 1.301±0.005
Astrometry
Radial velocity (Rv)+0.2±2.9 km/s
Proper motion (μ) RA: −3.923 mas/yr
Dec.: –117.824 mas/yr
Parallax (π)7.7081 ± 0.1300 mas
Distance423 ± 7 ly
(130 ± 2 pc)
Absolute magnitude (MV)0.14
Details
Mass0.89±0.25 M
Radius22.89+0.94
−0.41 R
Luminosity153±3 L
Surface gravity (log g)1.69±0.11 cgs
Temperature4,246±92 K
Metallicity −0.54±0.05 dex
Age11.2+1.1
−1.0 Gyr
Other designations
62 Aql, BD−01° 3887, GC 27832, HD 190299, HIP 98844, HR 7667, SAO 144045
Database references
SIMBADdata

62 Aquilae is a single star located about 427 light years away from the Sun in the equatorial constellation of Aquila. 62 Aquilae is its Flamsteed designation. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.67.

This is an aging giant star with a stellar classification of K4 III, having exhausted the supply of hydrogen at its core and expanded to 23 times the girth of the Sun. It is 11.2 billion years old with 0.89 times the Sun's mass. The star is radiating 153 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,246 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. ^ Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, 5, Bibcode:1999MSS...C05....0H.
  4. Gontcharov, G. A. (2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system", Astronomy Letters, 32 (11): 759–771, arXiv:1606.08053, Bibcode:2006AstL...32..759G, doi:10.1134/S1063773706110065, S2CID 119231169.
  5. ^ Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances", The Astrophysical Journal, 817 (1): 40, arXiv:1511.04088, Bibcode:2016ApJ...817...40F, doi:10.3847/0004-637X/817/1/40, S2CID 118675933.
  6. "62 Aql". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved November 1, 2018.
  7. 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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