Astronomy:Upsilon Aquilae

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Short description: Star in the constellation Aquila
Upsilon Aquilae
Location of υ Aquilae (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Aquila[1]
Right ascension  19h 45m 39.947s[2]
Declination +07° 36′ 47.37″[2]
Apparent magnitude (V) +5.889[3]
Characteristics
Evolutionary stage main sequence[2][4]
Spectral type A3 IV[5]
U−B color index +0.09[6]
B−V color index +0.18[6]
Astrometry
Radial velocity (Rv)−29.9±2.0[7] km/s
Proper motion (μ) RA: +53.593[2] mas/yr
Dec.: −0.223[2] mas/yr
Parallax (π)18.884 ± 0.0408[2] mas
Distance172.7 ± 0.4 ly
(53.0 ± 0.1 pc)
Absolute magnitude (MV)+2.24[1]
Details
Mass1.68[8] M☉
Luminosity10.5[1] L☉
Surface gravity (log g)4.21[3] cgs
Temperature7,906[3] K
Metallicity [Fe/H]−0.05[3] dex
Rotational velocity (v sin i)22.5[8] km/s
Age361±308[8] Myr
Other designations
υ Aql, 49 Aquilae, BD+07°4210, GC 27342, HD 186689, HIP 97229, HR 7519, SAO 125032, PPM 168596[9]
Database references
SIMBADdata

Upsilon Aquilae is a star in the equatorial constellation of Aquila. Its name is a Bayer designation that is Latinized from υ Aquilae, and abbreviated Upsilon Aql or υ Aql. With an apparent visual magnitude of +5.91[6] it is a faint star but, according to the Bortle Dark-Sky Scale, it is visible to the naked eye from suburban skies. It has an annual parallax shift of 18.9 mas,[10] indicating a distance of 173 light-years (53 parsecs). The star is drifting closer with a radial velocity of −30 km/s.[7]

This is a subgiant star with a stellar classification of A3 IV.[5] The outer atmosphere is radiating energy into space with 10.5[1] times the Sun's luminosity from its photosphere at an effective temperature of 7,906 K,[3] which gives it the white-hot glow of an A-type star. It is 361 million years old with 1.68 times the mass of the Sun and has a relatively high rate of spin with a projected rotational velocity of 22.5 km/s. An infrared excess has been reported, although no circumstellar disk has been resolved.[8]

References

  1. ↑ 1.0 1.1 1.2 1.3 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 3.2 3.3 3.4 Soubiran, C. et al. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics 515: A111, doi:10.1051/0004-6361/201014247, Bibcode: 2010A&A...515A.111S. 
  4. ↑ Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics 537: A120. doi:10.1051/0004-6361/201117691. Bibcode: 2012A&A...537A.120Z. 
  5. ↑ 5.0 5.1 Cowley, A. et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal 74: 375–406, doi:10.1086/110819, Bibcode: 1969AJ.....74..375C. 
  6. ↑ 6.0 6.1 6.2 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J. 
  7. ↑ 7.0 7.1 Wilson, Ralph Elmer (1953), "General catalogue of stellar radial velocities", Washington (Carnegie Institution of Washington): 0, Bibcode: 1953GCRV..C......0W. 
  8. ↑ 8.0 8.1 8.2 8.3 Grandjean, A. et al. (June 2021), "A SOPHIE RV search for giant planets around young nearby stars (YNS). A combination with the HARPS YNS survey", Astronomy & Astrophysics 650: id. A39, doi:10.1051/0004-6361/202039672, Bibcode: 2021A&A...650A..39G. 
  9. ↑ "* ups Aql". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%2A+ups+Aql. 
  10. ↑ Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.