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Star in the constellation Aquila
70 Aquilae
Observation dataEpoch J2000 Equinox J2000
Constellation
Aquila
Right ascension
20 36 43.63394
Declination
−02° 32′ 59.8341″
Apparent magnitude (V)
4.903
Characteristics
Spectral type
K4+ III Ba1, K3 III, or K5 II
B−V color index
1.606±0.041
Astrometry Radial velocity (Rv )−9.4±0.4 km/s Proper motion (μ) RA: +10.124 mas /yr Dec.: –15.604 mas /yr Parallax (π)3.4533 ± 0.3160 mas Distance 940 ± 90 ly (290 ± 30 pc ) Absolute magnitude (MV )−3.05
Details Mass 6.2±0.6 M ☉ Radius 102 R ☉ Luminosity (bolometric) 4,072 L ☉ Surface gravity (log g )1.9 cgs Temperature 3,900 K Metallicity −0.294±0.093 dex Rotational velocity (v sin i )1.9 km/s Age 63.1±17.8 Myr
Other designations 70 Aql , BD −03° 496, FK5 3648, HD 196321, HIP 101692, HR 7873, SAO 144624
Database references SIMBAD data
70 Aquilae , abbreviated 70 Aql , is a single orange-hued star in the equatorial constellation of Aquila . 70 Aquilae is its Flamsteed designation . It is visible to the naked eye with an apparent visual magnitude of 4.90. The distance to 70 Aquilae, as determined from its annual parallax shift of 3.5 mas , is around 940 light years . The star is moving closer to the Earth with a heliocentric radial velocity of −9 km/s.
Classification
Perkins et al. (1989) found a stellar classification of K4+ III Ba1 for this star, suggesting it is a K-type giant with abundance anomaly of barium . Houk and Swift (1999) matched an ordinary giant with a class of K3 III. Many sources still use the 1991 Bright Star Catalogue classification of K5 II, which instead suggests a bright giant star .
Size and temperature
The interferometry -measured angular diameter of this star, after correcting for limb darkening , is 3.27±0.04 mas, which, at its estimated distance, equates to a physical radius of roughly 102 times the radius of the Sun . 70 Aquilae is about 63 million years old with 6 times the mass of the Sun . It is radiating 4,072 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,900 K.
References
^ 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 .
^ Hohle, M. M.; et al. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten , 331 (4): 349, arXiv :1003.2335 , Bibcode :2010AN....331..349H , doi :10.1002/asna.200911355 , S2CID 111387483 .
^ Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series , 71 : 245, Bibcode :1989ApJS...71..245K , doi :10.1086/191373 .
^ Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey , 5 , Bibcode :1999MSS...C05....0H .
^ Hoffleit, D.; Warren, Jr., W. H. (1991), "The Bright Star Catalogue", New Haven (5th Revised ed.), Astronomical Data Center, NSSDC/ADC, Bibcode :1964cbs..book.....H
^ 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 .
^ Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 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 .
^ Tetzlaff, N.; et al. (2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society , 410 (1): 190–200, arXiv :1007.4883 , Bibcode :2011MNRAS.410..190T , doi :10.1111/j.1365-2966.2010.17434.x , S2CID 118629873 .
^ Lang, Kenneth R. (2006), Astrophysical formulae , Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser , ISBN 3-540-29692-1 . The radius (R* ) is given by:
2
⋅
R
∗
=
(
289.6
⋅
3.27
⋅
10
−
3
)
AU
0.0046491
AU
/
R
⨀
≈
204
⋅
R
⨀
{\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(289.6\cdot 3.27\cdot 10^{-3})\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 204\cdot R_{\bigodot }\end{aligned}}}
^ Domiciano de Souza, A.; et al. (November 2005), "Gravitational-darkening of Altair from interferometry", Astronomy and Astrophysics , 442 (2): 567–578, Bibcode :2005A&A...442..567D , doi :10.1051/0004-6361:20042476 .
Taylor, B. J. (February 1999), "Catalogs of temperatures and averages for evolved G and K stars", Astronomy and Astrophysics Supplement , 134 (3): 523–524, Bibcode :1999A&AS..134..523T , doi :10.1051/aas:1999153 .
"69 Aql" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved November 1, 2018.
^ 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 .
^ Gomez, A. E.; et al. (1997), "Absolute magnitudes and kinematics of barium stars", Astronomy and Astrophysics , 319 : 881, Bibcode :1997A&A...319..881G .
Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics , 431 (2): 773–777, Bibcode :2005A&A...431..773R , doi :10.1051/0004-6361:20042039 .
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