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Nu2 Lyrae

From Wikipedia, the free encyclopedia
Star in the constellation Lyra
For other stars with thisBayer designation, seeν Lyrae
ν2 Lyrae
Location of ν2 Lyrae (circled)
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationLyra
Right ascension18h 49m 52.91732s[1]
Declination+32° 33′ 03.8170″[1]
Apparent magnitude (V)5.23[2]
Characteristics
Spectral typeA3 V[3]
U−Bcolor index+0.12[2]
B−Vcolor index+0.10[2]
Astrometry
Radial velocity (Rv)+6.59±0.29[1] km/s
Proper motion (μ)RA: −10.685[1]mas/yr
Dec.: −11.771[1]mas/yr
Parallax (π)13.9238±0.0703 mas[1]
Distance234 ± 1 ly
(71.8 ± 0.4 pc)
Absolute magnitude (MV)+0.97[4]
Details
Mass1.91[5] M
Radius1.5[6] R
Luminosity32[7] L
Surface gravity (log g)3.89±0.14[5] cgs
Temperature8,912±303[5] K
Rotational velocity (v sin i)128[3] km/s
Age214[5] Myr
Other designations
ν2 Lyr,9 Lyr,BD+32°3228,HD 174602,HIP 92405,HR 7102,SAO 67446.[8]
Database references
SIMBADdata

Nu2 Lyrae,Latinized from ν2 Lyrae, or sometimes simplyNu Lyrae, is a solitary[9] star in the northernconstellation ofLyra. Based upon an annualparallax shift of 13.92 mas as seen from Earth, it is located around 234 light years from theSun.[1] With anapparent visual magnitude of 5.23,[2] it is bright enough to be faintly visible to the naked eye.

This is a white-huedA-type main sequence star with astellar classification of A3 V.[3] At an estimated age of 214 million years,[5] it is spinning with aprojected rotational velocity of 128 km/s.[3] This is giving the star anoblate shape with anequatorial bulge that is 5% larger than the polar radius.[10] Nu2 Lyrae has an estimated 1.9 times themass of the Sun[5] and about 1.5 times theSun's radius.[6] It is radiating 32 times thesolar luminosity[7] from itsphotosphere at aneffective temperature of around 8,912 K.[5]

References

[edit]
  1. ^abcdefgVallenari, 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.
  2. ^abcdMermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data,SIMBAD,Bibcode:1986EgUBV........0M.
  3. ^abcdRoyer, F.; et al. (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.
  4. ^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.
  5. ^abcdefgDavid, 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.
  6. ^abPasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)",Astronomy and Astrophysics,367 (3rd ed.):521–524,arXiv:astro-ph/0012289,Bibcode:2001A&A...367..521P,doi:10.1051/0004-6361:20000451,S2CID 425754.
  7. ^abMcDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars",Monthly Notices of the Royal Astronomical Society,427 (1):343–57,arXiv:1208.2037,Bibcode:2012MNRAS.427..343M,doi:10.1111/j.1365-2966.2012.21873.x,S2CID 118665352.
  8. ^"* nu. Lyr",SIMBAD,Centre de données astronomiques de Strasbourg, retrieved2017-03-15.
  9. ^Eggleton, 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.
  10. ^van Belle, Gerard T. (March 2012), "Interferometric observations of rapidly rotating stars",The Astronomy and Astrophysics Review,20 (1): 51,arXiv:1204.2572,Bibcode:2012A&ARv..20...51V,doi:10.1007/s00159-012-0051-2,S2CID 119273474.
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