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Omega2 Aquilae

From Wikipedia, the free encyclopedia
Star in the constellation Aquila
For other star systems with thisBayer designation, seeω Aquilae.
ω2 Aquilae
Location of ω2 Aquilae (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationAquila[1]
Right ascension19h 19m 53.067s[2]
Declination+11° 32′ 05.87″[2]
Apparent magnitude (V)6.03[1]
Characteristics
Evolutionary stagemain sequence[3]
Spectral typeA2 V[4] or F0V[5]
U−Bcolor index+0.087±0.007[1]
B−Vcolor index+0.08[6]
Astrometry
Radial velocity (Rv)−26.0±4.3[7][1] km/s
Proper motion (μ)RA: 44.335mas/yr[2]
Dec.: 22.475mas/yr[2]
Parallax (π)11.6957±0.0366 mas[2]
Distance278.9 ± 0.9 ly
(85.5 ± 0.3 pc)
Absolute magnitude (MV)1.48[1]
Details
Mass2.10±0.33[3] M
Radius2.25±0.07[3] R
Luminosity23.4±1.0[3] L
Surface gravity (log g)4.06±0.07[3] cgs
Temperature8,472±125[3] K
Rotational velocity (v sin i)152[8] km/s
Age224[8] Myr
Other designations
ω2 Aql,29 Aquilae,BD+11°3802,GC 26660,HD 181383,HIP 95002,HR 7332,SAO 104728,PPM 136128[9]
Database references
SIMBADdata

Omega2 Aquilae is astar in theequatorialconstellation ofAquila, the eagle.[9] Its name is aBayer designation that isLatinized fromω2 Aquilae, and abbreviated Omega2 Aql or ω2 Aql. This star has anapparent visual magnitude of 6.0,[1] which is close to the lower limit of detectability with thenaked eye. According to theBortle Dark-Sky Scale, this star can be viewed from dark rural skies. As the Earth orbits about the Sun, this star undergoes aparallax shift of11.7 mas.[10] This is equivalent to a physical distance of 279light-years (86parsecs) from Earth. The star is drifting closer to the Sun with aradial velocity of −26 km/s.[1]

Analysis of thespectrum of this white-hued star shows it to match astellar classification of A2 V,[4] indicating it is anA-type main sequence star. (A 2001 study found a discrepant class of F0V.[5]) It has about 2.25 the size and 2.1 times the mass of the Sun. The star is radiating 23.4 times theluminosity of the Sun from itsphotosphere at aneffective temperature of 9,245 K,[3] giving it the white hue of anA-type star.[11] Omega2 Aquilae is 224 million years old and is spinning rapidly with aprojected rotational velocity of 152 km/s.[8]

References

[edit]
  1. ^abcdefgAnderson, 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.
  2. ^abcdVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  3. ^abcdefgStassun, Keivan G.; et al. (2019), "The Revised TESS Input Catalog and Candidate Target List",The Astronomical Journal,158 (4): 138,arXiv:1905.10694,Bibcode:2019AJ....158..138S,doi:10.3847/1538-3881/ab3467.
  4. ^abCowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications",Astronomical Journal,74:375–406,Bibcode:1969AJ.....74..375C,doi:10.1086/110819.
  5. ^abPaunzen, E.; et al. (July 2001), "A spectroscopic survey for lambda Bootis stars. II. The observational data",Astronomy and Astrophysics,373:625–632,Bibcode:2001A&A...373..625P,doi:10.1051/0004-6361:20010630.
  6. ^Osawa, K.; Hata, S. (1962), "Three-color photometry of B8-A2 stars (II).",Annals of the Tokyo Astronomical Observatory,7: 209,Bibcode:1962AnTok...7..209O.
  7. ^Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.),Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto:International Astronomical Union, p. 57,Bibcode:1967IAUS...30...57E.
  8. ^abcDavid, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets",The Astrophysical Journal,804 (2): 146,arXiv:1501.03154,Bibcode:2015ApJ...804..146D,doi:10.1088/0004-637X/804/2/146,S2CID 33401607.
  9. ^ab"ome02 Aql".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-07-21.
  10. ^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. Gaia DR2 record for this source atVizieR.
  11. ^"The Colour of Stars",Australia Telescope, Outreach and Education,Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived fromthe original on March 18, 2012, retrieved2012-01-16.

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