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28 Leonis Minoris

From Wikipedia, the free encyclopedia
Star in the constellation Leo Minor
28 Leonis Minoris
Observation data
EpochJ2000.0      EquinoxJ2000.0 (ICRS)
ConstellationLeo Minor
Right ascension10h 24m 08.60391s[1]
Declination+33° 43′ 06.7069″[1]
Apparent magnitude (V)5.50±0.01[2]
Characteristics
Evolutionary stagered giant branch[1]
Spectral typeK1 III[3]
B−Vcolor index+1.18[4]
Astrometry
Radial velocity (Rv)−24.3±0.2[5] km/s
Proper motion (μ)RA: −14.460mas/yr
Dec.: −2.770mas/yr
Parallax (π)6.7945±0.091 mas[1]
Distance480 ± 6 ly
(147 ± 2 pc)
Absolute magnitude (MV)−0.05[6]
Details
Mass1.19[7] M
Radius22.6[1] R
Luminosity207[1] L
Surface gravity (log g)1.80[7] cgs
Temperature4,580±122[8] K
Metallicity[Fe/H]−0.04[1] dex
Age202[1] Myr
Other designations
28 LMi,AG+33°1015,BD+34°2123,GC 14280,HD 90040,HIP 50935,HR 4081,SAO 62019[9]
Database references
SIMBADdata

28 Leonis Minoris (28 LMi) is a solitary,[10] orange huedstar located in the northernconstellationLeo Minor, the lesser lion. It has anapparent magnitude of 5.5,[2] allowing it to be faintly visible to thenaked eye. Based onparallax measurements from theGaia satellite, it is estimated to be 480light years distant.[1] 28 LMi is approaching theSolar System with a heliocentricradial velocity of−24 km/s.[5] At its current distance, the star brightness is diminished by 0.14magnitudes due to interstellar dust.[11]

This is apopulation II[12]giant star with astellar classification of K1 III.[3] It has a comparablemass to theSun[7] but has expanded to 22.6 times itsgirth.[1] It radiates 207 times theluminosity of the Sun[1] from itsphotosphere at aneffective temperature of4,580 K.[8] It has aniron abundance 90% of the Sun's, making it slightly metal deficient.[1]

References

[edit]
  1. ^abcdefghijklVallenari, 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.
  3. ^abAdams, Walter S.; Joy, Alfred H.; Humason, Milton L.; Brayton, Ada Margaret (April 1935)."The Spectroscopic Absolute Magnitudes and Parallaxes of 4179 Stars".The Astrophysical Journal.81: 187.Bibcode:1935ApJ....81..187A.doi:10.1086/143628.eISSN 1538-4357.ISSN 0004-637X.
  4. ^Haggkvist, L.; Oja, T. (1970). "Results of BV photometry 1969-70 (Uppsala refractor)".Private Communication.Bibcode:1970Priv.........0H.
  5. ^abFamaey, B.; Jorissen, A.; Luri, X.; Mayor, M.; Udry, S.; Dejonghe, H.; Turon, C. (January 2005)."Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters".Astronomy and Astrophysics.430: 165.arXiv:astro-ph/0409579.Bibcode:2005A&A...430..165F.doi:10.1051/0004-6361:20041272.S2CID 17804304.
  6. ^Anderson, 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.
  7. ^abcAnders, F.; et al. (August 2019)."Photo-astrometric distances, extinctions, and astrophysical parameters forGaia DR2 stars brighter thanG = 18".Astronomy & Astrophysics.628: A94.arXiv:1904.11302.Bibcode:2019A&A...628A..94A.doi:10.1051/0004-6361/201935765.eISSN 1432-0746.ISSN 0004-6361.
  8. ^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.
  9. ^"28 LMi".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedNovember 18, 2022.
  10. ^Eggleton, P. P.; Tokovinin, A. A. (11 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.eISSN 1365-2966.ISSN 0035-8711.
  11. ^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.
  12. ^Bartkevicius, A.; Lazauskaite, R. (1 January 1997)."Classification of Population II Stars in the Vilnius Photometric System. II. Results".Open Astronomy.6 (4): 499.Bibcode:1997BaltA...6..499B.doi:10.1515/astro-1997-0402.eISSN 2543-6376.
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