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Nu Arietis

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Star in the constellation Aries
Nu Arietis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aries
Right ascension 02 38 48.99425
Declination +21° 57′ 41.0616″
Apparent magnitude (V) 5.43
Characteristics
Spectral type A7 V
U−B color index +0.13
B−V color index +0.16
Astrometry
Radial velocity (Rv)+8.0±4.2 km/s
Proper motion (μ) RA: −7.47 mas/yr
Dec.: −15.90 mas/yr
Parallax (π)9.68 ± 0.76 mas
Distance340 ± 30 ly
(103 ± 8 pc)
Absolute magnitude (MV)+0.40
Details
ν Ari A
Mass2.43±0.06 M
Radius1.8 R
Luminosity63.5 L
Surface gravity (log g)3.5±0.25 cgs
Temperature8,000±500 K
Rotational velocity (v sin i)133 km/s
Age621+269
−268 Myr
ν Ari B
Mass1.0±0.03 M
Temperature5,551±107 K
Metallicity 0.0 dex
Rotational velocity (v sin i)10 km/s
Other designations
ν Ari, 32 Arietis, BD+21° 362, FK5 89, HD 16432, HIP 12332, HR 773, SAO 75495
Database references
SIMBADdata

Nu Arietis, Latinized from ν Arietis, is the Bayer designation for a white-hued star in the northern constellation of Aries. It is faintly visible to the naked eye with an apparent visual magnitude of +5.43. Based upon an annual parallax shift of 9.68 mas as seen from Earth, it is located roughly 340 light years from the Sun. It is moving away from the Sun with a radial velocity of 8 km/s.

This is an A-type main sequence star with a stellar classification of A7 V. Nu Arietis has an estimated 2.4 times the mass of the Sun and about 1.8 times the Sun's radius. The star is radiating 63.5 times the Sun's luminosity from its photosphere at an effective temperature of around 8,000 K. It is roughly 621 million years old and is spinning with a projected rotational velocity of 133 km/s. A close companion was discovered in 2016 using the direct spectral detection method.

References

  1. ^ van Leeuwen, F. (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. ^ Oja, T. (April 1983), "UVB photometry of FK4 and FK4 Supplement stars", Astronomy and Astrophysics Supplement Series, 52: 131–134, Bibcode:1983A&AS...52..131O.
  3. ^ Cowley, 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.
  4. ^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics, 546: 14, arXiv:1208.3048, Bibcode:2012A&A...546A..61D, doi:10.1051/0004-6361/201219219, S2CID 59451347, A61.
  5. 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.
  6. ^ Huang, Wenjin; et al. (October 2010), "A Stellar Rotation Census of B Stars: From ZAMS to TAMS", The Astrophysical Journal, 722 (1): 605–619, arXiv:1008.1761, Bibcode:2010ApJ...722..605H, doi:10.1088/0004-637X/722/1/605, S2CID 118532653.
  7. ^ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics, 367 (Third ed.): 5211–524, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
  8. ^ Gullikson, Kevin; et al. (August 2016), "The Close Companion Mass-ratio Distribution of Intermediate-mass Stars", The Astronomical Journal, 152 (2): 13, arXiv:1604.06456, Bibcode:2016AJ....152...40G, doi:10.3847/0004-6256/152/2/40, S2CID 119179065, 40.
  9. "nu. Ari". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-09-28.{{cite web}}: CS1 maint: postscript (link)

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