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69 Aquilae

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(Redirected from 69 Aql) Star in the constellation Aquila
69 Aquilae
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 20 29 38.99995
Declination −02° 53′ 07.9176″
Apparent magnitude (V) 4.91
Characteristics
Evolutionary stage giant
Spectral type K1/2 III
B−V color index 1.162
Astrometry
Radial velocity (Rv)−22.51±0.16 km/s
Proper motion (μ) RA: +70.355 mas/yr
Dec.: –21.523 mas/yr
Parallax (π)16.2388 ± 0.2271 mas
Distance201 ± 3 ly
(61.6 ± 0.9 pc)
Absolute magnitude (MV)0.97
Details
Mass1.54 M
Radius11 R
Luminosity45.7 L
Surface gravity (log g)2.5 cgs
Temperature4,529±5 K
Metallicity 0.03 dex
Rotational velocity (v sin i)4.0 km/s
Age3.44 Gyr
Other designations
69 Aql, BD−03° 4918, HD 195135, HIP 101101, HR 7831, SAO 144495
Database references
SIMBADdata

69 Aquilae, abbreviated 69 Aql, is a star in the equatorial constellation of Aquila. 69 Aquilae is its Flamsteed designation. It is visible to the naked eye with an apparent visual magnitude of 4.91. Based upon an annual parallax shift of 16.2 mas, it is located 201 light years away. The star is moving closer to the Earth with a heliocentric radial velocity of −22.5 km/s.

The stellar classification of 69 Aquilae is K1/2 III, which means this is an evolved giant star. It belongs to a sub-category called the red clump, indicating that it is on the horizontal branch and is generating energy through helium fusion at its core. The star is about 3.4 billion years old with 1.54 times the mass of the Sun and has expanded to 11 times the Sun's radius. It is radiating 45.7 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,529 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. ^ Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209, S2CID 121883397.
  4. ^ Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, 5, Bibcode:1999MSS...C05....0H.
  5. ^ Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", Astronomical Journal, 150 (3): 23, arXiv:1507.01466, Bibcode:2015AJ....150...88L, doi:10.1088/0004-6256/150/3/88, S2CID 118505114.
  6. "69 Aql". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved November 1, 2018.
  7. Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal, 539 (2): 732–741, arXiv:astro-ph/0003329, Bibcode:2000ApJ...539..732A, doi:10.1086/309278, S2CID 16673121.
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