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20 Little Lion

20 Little Lion ( 20 LMi ) is a binary star in the constellation of Little Lion at a distance of about 48 light-years from the Sun. The main component is a yellow dwarf of spectral class G3 Va, similar to the Sun.

20 Little Lion
Star
Yellow dwarf.jpg
20 Small Lion in the representation of the artist.
Observational data
( Age J2000.0 )
Right ascension
Declination
Distance48.6 ± 0.6 St. years (14.9 ± 0.2 pc )
Visible magnitude ( V )+5.4
ConstellationSmall lion
Astrometry
Radial velocity ( R v )+56 km / s
Own movement (μ)RA: −529.18 mas per year
Dec: −428.91 mas per year
Parallax (π)67.14 ± 0.83 mas
Absolute magnitude (V)+4.53
Characteristics
Spectral classG3 Va / M6.5
Color Index ( B - V )0.65
Color Index ( U - B )0.27
physical characteristics
Weight1.1 M ☉
Radius1.18 R ☉
Temperature5600-5700 K
Luminosity1.32 L ☉
Metallicity
The propertiesAnalogue of the sun
Other designations
Fl 20 LMi
BD + 32 ° 1964 , FK5 1258 , HD 86728 , HIP 49081 , HR 3951 , LHS 2216 , SAO 61808 , GCTP 2366.00, GJ 376, LTT 12671
20 LMi
Database Information
SIMBADdata
ARICNSdata

She has a relatively large movement of her own . Her companion is an old, active red dwarf with a relatively high metallicity [5] . Two stars are separated from each other at a distance of 14.5 arc seconds .

Notes

  1. ↑ 1 2 3 4 Collaboration G. Gaia DR2 - 2018 .-- T. 1345. - P. 0.
    <a href=" https://wikidata.org/wiki/Track:Q51905050 "> </a>
  2. ↑ Aguilera-Gómez C., Ramírez I., Chanamé J. Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert // Astron. Astrophys. - EDP ​​Sciences , 2018 .-- Vol. 614. - P. 55–55. - ISSN 0004-6361 ; 0365-0138 ; 1432-0746 ; 1286-4846 - doi: 10.1051 / 0004-6361 / 201732209
    <a href=" https://wikidata.org/wiki/Track:Q114404 "> </a> <a href=" https://wikidata.org/wiki/Track:Q752075 "> </a> <a href = " https://wikidata.org/wiki/Track:Q65646788 "> </a>
  3. ↑ R. Earle Luck, Heiter U. Dwarfs in the Local Region // Astron. J. / J. G. III - IOP Publishing , 2006. - Vol. 131, Iss. 6. - P. 3069–3092. - ISSN 0004-6256 ; 1538-3881 - doi: 10.1086 / 504080
    <a href=" https://wikidata.org/wiki/Track:Q2915886 "> </a> <a href=" https://wikidata.org/wiki/Track:Q669166 "> </a> <a href = " https://wikidata.org/wiki/Track:Q56639636 "> </a> <a href=" https://wikidata.org/wiki/Track:Q6234745 "> </a>
  4. ↑ R. Earle Luck, Heiter U. Stars within 15 Parsecs: Abundances for a Northern Sample // Astron. J. / J. G. III - IOP Publishing , 2005. - Vol. 129, Iss. 2. - P. 1063–1083. - ISSN 0004-6256 ; 1538-3881 - doi: 10.1086 / 427250
    <a href=" https://wikidata.org/wiki/Track:Q2915886 "> </a> <a href=" https://wikidata.org/wiki/Track:Q669166 "> </a> <a href = " https://wikidata.org/wiki/Track:Q53951943 "> </a> <a href=" https://wikidata.org/wiki/Track:Q6234745 "> </a>
  5. ↑ JE Gizis, DG Monet, IN Reid, JD Kirkpatrick, AJ Burgasser. Two Nearby M Dwarf Binaries from 2MASS // English Monthly Notices of the Royal Astronomical Society . - Oxford University Press , 2000. - Vol. 311 , no. 2 . - P. 385 . - DOI : 10.1046 / j.1365-8711.2000.03060.x .
Source - https://ru.wikipedia.org/w/index.php?title=20_Mallogo_Lva&oldid=100073331


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Clever Geek | 2019