37 Leonis Minoris

Star in the constellation Leo Minor From Wikipedia, the free encyclopedia

37 Leonis Minoris is a single,[9] yellow-hued star in the northern constellation of Leo Minor. It is faintly visible to the naked eye with an apparent visual magnitude of 4.68.[1] The star is moving closer to the Sun with a heliocentric radial velocity of −8 km/s.[1] The annual parallax shift of 5.58±0.24 mas[2] provides a distance estimate of roughly 580 light years.

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
37 Leonis Minoris
Location of 37 Leonis Minoris (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Leo Minor[1]
Right ascension 10h 38m 43.21s[2]
Declination +31° 58 34.4[2]
Apparent magnitude (V) 4.68[1]
Characteristics
Spectral type G2.5 IIa[3]
B−V color index 0.823±0.008[1]
Astrometry
Radial velocity (Rv)−8.0±0.3[1] km/s
Proper motion (μ) RA: +9.76[2] mas/yr
Dec.: −35.56[2] mas/yr
Parallax (π)5.58±0.24 mas[2]
Distance580 ± 30 ly
(179 ± 8 pc)
Absolute magnitude (MV)−1.84[4]
Details
Mass3.72[5] M
Radius24[6] R
Luminosity438[1] L
Surface gravity (log g)2.22[5] cgs
Temperature5,468[5] K
Metallicity [Fe/H]0.03[5] dex
Rotational velocity (v sin i)6.4[7] km/s
Age200[7] Myr
Other designations
37 LMi, BD+32°2061, FK5 1275, HD 92125, HIP 52098, HR 4166, SAO 62173[8]
Database references
SIMBADdata
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The Bright Star Catalogue lists this star with a stellar classification of G2.5 IIa,[3] indicating it is an evolved G-type bright giant. Gray et al. (2001) gave it a class of G1 II,[10] while Keenan and McNeil (1989) assigned this star to the giant class G2.5 IIIa.[11] It has an estimated 3.72 times the mass of the Sun[5] and about 24 times the Sun's radius.[6] The star is around 200 million years old with a projected rotational velocity of 6.4 km/s.[7] It is radiating about 438 times the Sun's luminosity[1] from its enlarged photosphere at an effective temperature of 5,468 K.[5]

References

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