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7 Leonis Minoris

From Wikipedia, the free encyclopedia
G-type giant in the constellation Leo Minor
7 Leonis Minoris
Location of 7 LMi on the map (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationLeo Minor
Right ascension09h 30m 43.22705s[1]
Declination+33° 39′ 20.5700″[1]
Apparent magnitude (V)5.86±0.01[2]
Characteristics
Evolutionary stagehorizontal branch[3]
Spectral typeG9 III[4]
B−Vcolor index+1.05[5]
Astrometry
Radial velocity (Rv)1.7±0.9[6] km/s
Proper motion (μ)RA: −23.939mas/yr[1]
Dec.: −48.160mas/yr[1]
Parallax (π)7.0542±0.1338 mas[1]
Distance462 ± 9 ly
(142 ± 3 pc)
Absolute magnitude (MV)−0.03[7]
Details
Mass2.74+0.24
−0.25
[3] M
Radius13.41±0.68[8] R
Luminosity96.0+3.3
−3.6
[1] L
Surface gravity (log g)2.49+0.07
−0.06
[3] cgs
Temperature4,923±122[9] K
Metallicity[Fe/H]−0.03±0.10[10] dex
Rotational velocity (v sin i)0.24[11] km/s
Age575+201
−139
[3] Myr
Other designations
7 LMi,AG+33°953,BD+34°1999,FK5 2755,GC 13112,HD 82087,HIP 46652,HR 3764,SAO 61529,CCDM J09307+3339A,WDS J09307+3339A,TIC 8855140[12]
Database references
SIMBADdata

7 Leonis Minoris (7 LMi) is astar located in the northernconstellationLeo Minor. It is also designated asHD 82087 andHR 3764. 7 LMi is faintly visible to thenaked eye as a yellow-hued point of light with anapparent magnitude of 5.86.[2]Gaia DR3parallax measurements imply a distance of 462light-years[1] and it is currently receding with a heliocentricradial velocity of1.7 km/s.[6] At its current distance, 7 LMi's brightness is diminished by 0.12magnitudes due tointerstellar extinction[13] and it has anabsolute magnitude of −0.03.[7]

There have been disagreements on the object'sstellar classification. 7 LMi is either aG-typegiant star with a class of either G8 or G9 III,[4] or it is aK-type giant with a class of K0 III.[14] It is most likely on thehorizontal branch (95% fit),[3] generating energy viahelium fusion at itscore. It has 2.74 times themass of the Sun but at the age of 575million years,[3] it has expanded to 13.41 times theradius of the Sun.[8] It radiates 96 times theluminosity of the Sun[1] from its enlargedphotosphere at aneffective temperature of4,923 K.[9] 7 LMi has a near solarmetallicity at [Fe/H] = −0.03[10] and it spins very slowly with aprojected rotational velocity of0.24 km/s.[11]

7 LMi has two visual companions. AG +33°954 is a background star located much farther away than 7 LMi[15] and it is a closespectroscopic binary itself.[16]

7 Leonis Minoris' companions[17]
CompanionStellar classificationPA (deg)Separation (arcsec)Apparent magnitude
AG +33°954 (B)G8 IV-V[4]12561.39.7
CG5 V[4]21795.911.6

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. ^abHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy and Astrophysics.355:L27–L30.Bibcode:2000A&A...355L..27H.ISSN 0004-6361.S2CID 17128864.
  3. ^abcdefStock, Stephan; Reffert, Sabine; Quirrenbach, Andreas (August 2018)."Precise radial velocities of giant stars: X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search".Astronomy & Astrophysics.616: A33.arXiv:1805.04094.Bibcode:2018A&A...616A..33S.doi:10.1051/0004-6361/201833111.ISSN 0004-6361.S2CID 247657118.
  4. ^abcdAbt, H. A. (May 1986). "The ages and dimensions of Trapezium systems".The Astrophysical Journal.304. American Astronomical Society: 688.Bibcode:1986ApJ...304..688A.doi:10.1086/164207.ISSN 0004-637X.S2CID 121295060.
  5. ^Haggkvist, L.; Oja, T. (1970). "Results of BV photometry 1969-70 (Uppsala refractor)".Private Communication.Bibcode:1970Priv.........0H.S2CID 231475662.
  6. ^abGontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35,495 Hipparcos stars in a common system".Astronomy Letters.32 (11):759–771.arXiv:1606.08053.Bibcode:2006AstL...32..759G.doi:10.1134/S1063773706110065.eISSN 1562-6873.ISSN 1063-7737.S2CID 119231169.
  7. ^abAnderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation".Astronomy Letters.38 (5):331–346.arXiv:1108.4971.Bibcode:2012AstL...38..331A.doi:10.1134/S1063773712050015.eISSN 1562-6873.ISSN 1063-7737.S2CID 119257644.
  8. ^abKervella, P.; Thévenin, F.; Di Folco, E.; Ségransan, D. (October 2004)."The angular sizes of dwarf stars and subgiants: Surface brightness relations calibrated by interferometry".Astronomy & Astrophysics.426 (1):297–307.arXiv:astro-ph/0404180.Bibcode:2004A&A...426..297K.doi:10.1051/0004-6361:20035930.eISSN 1432-0746.ISSN 0004-6361.
  9. ^abStassun, Keivan G.; et al. (9 September 2019)."The RevisedTESS 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.eISSN 1538-3881.hdl:1721.1/124721.S2CID 166227927.
  10. ^abReffert, Sabine; Bergmann, Christoph; Quirrenbach, Andreas; Trifonov, Trifon; Künstler, Andreas (December 15, 2014)."Precise Radial Velocities of Giant Stars VII. Occurrence Rate of Giant Extrasolar Planets as a Function of Mass and Metallicity".Astronomy & Astrophysics.574. EDP Sciences: A116.arXiv:1412.4634.Bibcode:2015A&A...574A.116R.doi:10.1051/0004-6361/201322360.ISSN 0004-6361.S2CID 59334290.
  11. ^abHekker, S.; Meléndez, J. (December 2007)."Precise radial velocities of giant stars: III. Spectroscopic stellar parameters".Astronomy & Astrophysics.475 (3):1003–1009.arXiv:0709.1145.Bibcode:2007A&A...475.1003H.doi:10.1051/0004-6361:20078233.ISSN 0004-6361.S2CID 10436552.
  12. ^"* 7 LMi".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedAugust 8, 2023.
  13. ^Gontcharov, George A.; Mosenkov, Aleksandr V. (28 September 2017)."Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars".Monthly Notices of the Royal Astronomical Society.472 (4):3805–3820.arXiv:1709.01160.Bibcode:2017MNRAS.472.3805G.doi:10.1093/mnras/stx2219.eISSN 1365-2966.ISSN 0035-8711.S2CID 118879856.
  14. ^Pertersson, J. H. (1927). "Distribution of stars in Carrington zone".Meddelanden Fran Astronomiska Observatorium Uppsala.29: 1.Bibcode:1927MeUpp..29....1P.
  15. ^Vallenari, 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.
  16. ^Gaia Collaboration (2022). "VizieR Online Data Catalog: Gaia DR3 Part 3. Non-single stars (Gaia Collaboration, 2022)".Vizier Online Data Catalog.Bibcode:2022yCat.1357....0G.
  17. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001)."The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog".The Astronomical Journal.122 (6):3466–3471.Bibcode:2001AJ....122.3466M.doi:10.1086/323920.ISSN 0004-6256.S2CID 119533755.
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