Spectroscopic binary in the constellation Leo Minor
19 Leonis Minoris
Location of 19 LMi (circled)
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS)
Constellation
Leo Minor
Right ascension
09h 57m 41.0544s[1]
Declination
+41° 03′ 20.275″[1]
Apparent magnitude (V)
5.10±0.01[2]
Characteristics
Spectral type
F6 V[3]
U−B color index
0.00[4]
B−V color index
+0.46[4]
Astrometry
Radial velocity (Rv)
−8.6±2.6[5] km/s
Proper motion (μ)
RA: −116.432 mas/yr[1] Dec.: −25.860 mas/yr[1]
Parallax (π)
34.5809 ± 0.0926 mas[1]
Distance
94.3 ± 0.3 ly (28.92 ± 0.08 pc)
Absolute magnitude (MV)
+2.86[6]
Orbit[7]
Period (P)
9.2835 d
Eccentricity (e)
0.048[8]
Periastron epoch (T)
2,443,858.21 JD
Argument of periastron (ω) (primary)
351[8]°
Semi-amplitude (K1) (primary)
18.9 km/s
Semi-amplitude (K2) (secondary)
25.3 km/s
Details
A
Mass
1.29±0.19[9]M☉
Radius
2±0.1[9]R☉
Luminosity
6.41±0.04[1]L☉
Surface gravity (log g)
3.98±0.03[10] cgs
Temperature
6,483±80[11] K
Metallicity [Fe/H]
+0.09[11] dex
Rotational velocity (v sin i)
5[12] km/s
Age
2.474[1] Gyr
B
Mass
1.01[13]M☉
Other designations
19 LMi, AG+41°966, BD+41°2033, FK5 374, GC 13700, GJ 3574, HD 86146, HIP 48833, HR 3928, SAO 43115[14]
Database references
SIMBAD
data
19 Leonis Minoris (19 LMi) is a spectroscopic binary[15] located in the northern constellation Leo Minor. It has an apparent magnitude of 5.1,[2] making it one of the brighter members of the constellation. The system is relatively close at a distance of 94 light years[1] but is drifitng closer with a heliocentric radial velocity of 8.6 km/s.[5]
This spectroscopic binary can be classified as single lined[3] because only the primary's spectrum can be observed clearly, with it having a stellar classification of F6 V.[3] This makes it an ordinary F-type main-sequence star. The companion is probably a G-type main-sequence star of G0,[7] having a mass 101% that of the Sun.[13] The pair have a relatively circular orbit of about 9 days.[13]
19 LMi has 129% the mass of the Sun[9] and an effective temperature of 6,483 K, giving a yellow white hue. The object is somewhat evolved at an age of 2.5 billion years,[1] having a slightly enlarged radius of 2 R☉[9] and a luminosity of 6.4 L☉,[1] high for its class. 19 LMi has an iron abundance 123% that of the Sun,[11] making it slightly metal enriched. It spins modestly with a projected rotational velocity of 5 km/s.[12]
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