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31 Leonis

Coordinates:Sky map10h 07m 54s, +09° 59′ 51″
From Wikipedia, the free encyclopedia
Binary star system in the constellation Leo
31 Leonis
Location of 31 Leonis (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
ConstellationLeo
Right ascension10h 07m 54.2701s[1]
Declination+09° 59′ 51.025″[1]
Apparent magnitude (V)4.39[2]
Characteristics
Spectral typeK3.5 IIIb Fe-1:[3]
B−Vcolor index1.447[4]
Astrometry
Radial velocity (Rv)+39.84±0.20[5] km/s
Proper motion (μ)RA: −82.021mas/yr[1]
Dec.: −64.844mas/yr[1]
Parallax (π)11.0209±0.1661 mas[1]
Distance296 ± 4 ly
(91 ± 1 pc)[1]
Absolute magnitude (MV)−0.39[2]
Details
Radius33.9+0.7
−0.71
[6] R
Luminosity283±9[6] L
Surface gravity (log g)1.42[6] cgs
Temperature4066±28[6] K
Metallicity[Fe/H]−0.02[7] dex
Rotational velocity (v sin i)5.1[4] km/s
Other designations
Yunü,31 Leo,BD+10°2112,HD 87837,HIP 49637,HR 3980,SAO 98964[8]
Database references
SIMBADdata

31 Leonis, also namedYunü,[9] is abinary star[10] system in the equatorialconstellation ofLeo. The system is visible to the naked eye in unresolved form, having a combinedapparent visual magnitude of 4.39.[2] An estimated distance of around 300 light years is obtained from the annualparallax shift of 11.02 mas as seen from Earth's orbit.[1] At the current distance,interstellar extinction between Earth and 31 Leo diminished the apparent brightness by 0.12 magnitudes.[6] It is moving away from the Sun with aradial velocity of +39.8 km/s.[5]

The primary member of 31 Leonis, component A, is anevolvedK-typered giant[11] with astellar classification ofK3.5 IIIb Fe-1:,[3] where the suffix notation indicates an underabundance of iron in thespectrum. It has expanded to 34 times theSolar radius and is radiating around 283 times theSun's luminosity from itsphotosphere at aneffective temperature of 4,066 K.[6] The magnitude 13.6 secondary, component B, lies at anangular separation of 7.9 arcseconds, as of 2008.[10]

This star has the traditional Chinese name Yunü (御女); it is in the middle of the southernmost stars of the Xuanyuan (轩辕) constellation (ο Leonis andρ Leonis). TheIAU Working Group on Star Names approved the name Yunü for this star on 18 July 2024 and it is now so entered in the IAU Catalog of Star Names.[9]

References

[edit]
  1. ^abcdefVallenari, 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. ^abcAnderson, 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.
  3. ^abKeenan, Philip C; McNeil, Raymond C (1989), "The Perkins catalog of revised MK types for the cooler stars",Astrophysical Journal Supplement Series,71: 245,Bibcode:1989ApJS...71..245K,doi:10.1086/191373,S2CID 123149047.
  4. ^abMassarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity",The Astronomical Journal,135 (1):209–231,Bibcode:2008AJ....135..209M,doi:10.1088/0004-6256/135/1/209,S2CID 121883397.
  5. ^abde 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.
  6. ^abcdefBaines, Ellyn K.; Clark III, James H.; Schmitt, Henrique R.; Stone, Jordan M.; von Braun, Kaspar (2023-12-01), "33 New Stellar Angular Diameters from the NPOI, and Nearly 180 NPOI Diameters as an Ensemble",The Astronomical Journal,166 (6): 268,arXiv:2505.23514,Bibcode:2023AJ....166..268B,doi:10.3847/1538-3881/ad08be,ISSN 0004-6256.
  7. ^Piau, L.; et al. (February 2011), "Surface convection and red-giant radius measurements",Astronomy and Astrophysics,526: A100,arXiv:1010.3649,Bibcode:2011A&A...526A.100P,doi:10.1051/0004-6361/201014442,S2CID 118533297.
  8. ^"31 Leo".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2018-02-18.
  9. ^ab"IAU Catalog of Star Names". Retrieved22 February 2025.
  10. ^abEggleton, 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.
  11. ^Wood, Brian E.; et al. (October 2016), "Hubble Space Telescope Constraints on the Winds and Astrospheres of Red Giant Stars",The Astrophysical Journal,829 (2): 13,arXiv:1607.07732,Bibcode:2016ApJ...829...74W,doi:10.3847/0004-637X/829/2/74,S2CID 119258785, 74.
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