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64 Aquilae

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(Redirected from 64 Aql) Star in the constellation Aquila
64 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20 08 01.82224
Declination −00° 40′ 41.4663″
Apparent magnitude (V) 5.97
Characteristics
Spectral type K1 III/IV
B−V color index +1.023±0.003
Astrometry
Radial velocity (Rv)−3.64±0.39 km/s
Proper motion (μ) RA: −115.520 mas/yr
Dec.: –67.593 mas/yr
Parallax (π)21.4233 ± 0.0627 mas
Distance152.2 ± 0.4 ly
(46.7 ± 0.1 pc)
Absolute magnitude (MV)2.61
Details
Mass1.17±0.06 M
Radius4.49±0.13 R
Luminosity11.17 L
Surface gravity (log g)3.31±0.07 cgs
Temperature4,786±20 K
Metallicity −0.03±0.03 dex
Rotational velocity (v sin i)1.51 km/s
Age6.20±1.18 Gyr
Other designations
64 Aql, BD−01° 3899, GC 27930, HD 191067, HIP 99171, HR 7690, SAO 144095
Database references
SIMBADdata

64 Aquilae, abbreviated 64 Aql, is a star in the equatorial constellation of Aquila. 64 Aquilae is its Flamsteed designation. It is a faint star that requires good viewing conditions to see, having an apparent visual magnitude of 5.97. The distance to 64 Aql, as determined from its annual parallax shift of 21.42 mas, is 152.2 light years. At that distance, the visual magnitude of the star is diminished by an extinction of 0.029 due to interstellar dust. It is moving closer to the Earth with a heliocentric radial velocity of −3.6 km/s.

This is an evolved giant star currently on the red giant branch with a stellar classification of K1 III/IV. The luminosity class of 'III/IV' indicates the spectrum shows a blend of features matching a subgiant and giant star. It is around 6.2 billion years old with 1.17 times the mass of the Sun and has expanded to 4.5 times the Sun's radius. The star is radiating 11 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,786 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.
  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. ^ Maldonado, J.; et al. (June 2013), "The metallicity signature of evolved stars with planets", Astronomy & Astrophysics, 554: 18, arXiv:1303.3418, Bibcode:2013A&A...554A..84M, doi:10.1051/0004-6361/201321082, S2CID 119289111, A84.
  5. ^ Jones, M. I.; et al. (December 2011), "Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets. I. Sample definition and physical properties", Astronomy & Astrophysics, 536: 7, arXiv:1110.6459, Bibcode:2011A&A...536A..71J, doi:10.1051/0004-6361/201117887, S2CID 55769003, A71.
  6. "64 Aql". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved November 1, 2018.
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