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97 Aquarii

From Wikipedia, the free encyclopedia
Binary star in the constellation Aquarius
97 Aquarii
Observation data
Epoch J2000      Equinox J2000
ConstellationAquarius
Right ascension23h 22m 39.17113s[1]
Declination–15° 02′ 21.6245″[1]
Apparent magnitude (V)5.20[2] (5.59/6.72)[3]
Characteristics
Spectral typeA2 V + A7 V[4]
U−Bcolor index+0.10[2]
B−Vcolor index+0.20[2]
Astrometry
Radial velocity (Rv)–12[5] km/s
Proper motion (μ)RA: +117.00[1]mas/yr
Dec.: +16.48[1]mas/yr
Parallax (π)15.30±0.79 mas[1]
Distance210 ± 10 ly
(65 ± 3 pc)
Orbit[6]
Period (P)64.62yr
Semi-major axis (a)0.408″
Eccentricity (e)0.140
Inclination (i)77.6°
Longitude of the node (Ω)276.3°
Periastronepoch (T)1941.29
Argument of periastron (ω)
(secondary)
354.6°
Details
Rotational velocity (v sin i)175[7] km/s
Other designations
BD–15° 6406,HD 220278,HIP 115404,HR 8890,SAO 165658.[8]
Database references
SIMBADdata

97 Aquarii (abbreviated97 Aqr) is abinary star system in theequatorialconstellation ofAquarius.97 Aquarii is theFlamsteed designation. The combinedapparent visual magnitude of the system is 5.20;[2] the brighter star is magnitude 5.59 while the companion is magnitude 6.72.[3] Based upon an annualparallax shift of 15.30 milliarcseconds,[1] this system is at a distance of around 210light-years (64parsecs) from Earth.

The two stars in this system orbit each other over aperiod of 64.62 years at aneccentricity of 0.14.[3] Both areA-type main sequence stars; the primary has astellar classification of A2 V while its companion is A7 V.[4] Their composite spectrum shows the properties of aLambda Boötis star, which means it displayspeculiar abundances of certain elements.[9]

References

[edit]
  1. ^abcdefvan Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction",Astronomy and Astrophysics,474 (2):653–664,arXiv:0708.1752,Bibcode:2007A&A...474..653V,doi:10.1051/0004-6361:20078357,S2CID 18759600.
  2. ^abcdNicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System",Astronomy and Astrophysics Supplement Series,34:1–49,Bibcode:1978A&AS...34....1N.
  3. ^abcEggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  4. ^abChristy, James W.; Walker, R. L. Jr. (October 1969), "MK Classification of 142 Visual Binaries",Publications of the Astronomical Society of the Pacific,81 (482): 643,Bibcode:1969PASP...81..643C,doi:10.1086/128831
  5. ^Wilson, Ralph Elmer (1953). "General Catalogue of Stellar Radial Velocities".Carnegie Institute Washington D.C. Publication. Washington:Carnegie Institution of Washington.Bibcode:1953GCRV..C......0W.
  6. ^Anonymous (1999), "New orbits",International Astronomical Union Commission 26 (Double Stars),139 (Information Circular No. 139):1–2,Bibcode:1999IAUDS.139....1.
  7. ^Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions",Astronomy and Astrophysics,463 (2):671–682,arXiv:astro-ph/0610785,Bibcode:2007A&A...463..671R,doi:10.1051/0004-6361:20065224,S2CID 18475298.
  8. ^"* 97 Aqr".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2012-07-17.
  9. ^Gerbaldi, M.; Faraggiana, R.; Lai, O. (December 2003), "The heterogeneous class of lambda Bootis stars",Astronomy and Astrophysics,412 (2):447–464,Bibcode:2003A&A...412..447G,doi:10.1051/0004-6361:20031472.

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