Astronomy:Upsilon Aquilae

From HandWiki
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. Bibcode2012AstL...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, Bibcode2010A&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. Bibcode2012A&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, Bibcode1969AJ.....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, Bibcode1966CoLPL...4...99J. 
  7. 7.0 7.1 Wilson, Ralph Elmer (1953), "General catalogue of stellar radial velocities", Washington (Carnegie Institution of Washington): 0, Bibcode1953GCRV..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, Bibcode2021A&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. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.