Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

64 Aquilae

From Wikipedia, the free encyclopedia
Star in the constellation Aquila
64 Aquilae
Observation data
Epoch J2000      Equinox J2000
ConstellationAquila
Right ascension20h 08m 01.82224s[1]
Declination−00° 40′ 41.4663″[1]
Apparent magnitude (V)5.97[2]
Characteristics
Spectral typeK1 III/IV[3]
B−Vcolor index+1.023±0.003[2]
Astrometry
Radial velocity (Rv)−3.64±0.39[4] km/s
Proper motion (μ)RA: −115.520[1]mas/yr
Dec.: –67.593[1]mas/yr
Parallax (π)21.4233±0.0627 mas[1]
Distance152.2 ± 0.4 ly
(46.7 ± 0.1 pc)
Absolute magnitude (MV)2.61[2]
Details[4]
Mass1.17±0.06 M
Radius4.49±0.13 R
Luminosity11.17[2] L
Surface gravity (log g)3.31±0.07 cgs
Temperature4,786±20 K
Metallicity [Fe/H]−0.03±0.03 dex
Rotational velocity (v sin i)1.51[5] km/s
Age6.20±1.18 Gyr
Other designations
64 Aql,BD−01°3899,GC 27930,HD 191067,HIP 99171,HR 7690,SAO 144095[6]
Database references
SIMBADdata

64 Aquilae, abbreviated64 Aql, is astar in the equatorialconstellation ofAquila.64 Aquilae is itsFlamsteed designation. It is a faint star that requires good viewing conditions to see, having anapparent visual magnitude of 5.97.[2] The distance to 64 Aql, as determined from its annualparallax shift of 21.42 mas,[1] is 152.2 light years. At that distance, the visual magnitude of the star is diminished by anextinction of 0.029 due tointerstellar dust.[5] It is moving closer to the Earth with a heliocentricradial velocity of −3.6 km/s.[4]

This is anevolvedgiant star currently on thered giant branch[5] with astellar classification of K1 III/IV.[3] Theluminosity class of 'III/IV' indicates thespectrum shows a blend of features matching asubgiant and giant star. It is around 6.2 billion years old with 1.17 times themass of the Sun and has expanded to 4.5 times theSun's radius.[4] The star is radiating 11[2] times theSun's luminosity from its enlargedphotosphere at aneffective temperature of 4,786 K.[4]

References

[edit]
  1. ^abcdefBrown, 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. ^abcdefAnderson, 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. ^abHouk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5,Bibcode:1999MSS...C05....0H.
  4. ^abcdeMaldonado, 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. ^abcJones, 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. RetrievedNovember 1, 2018.
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
NGC
Other
Galaxies
NGC
Other
Retrieved from "https://en.wikipedia.org/w/index.php?title=64_Aquilae&oldid=1284769222"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp