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 | |
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]
DR3
was invoked but never defined (see the help page).Tycho2000
was invoked but never defined (see the help page).Abt2008
was invoked but never defined (see the help page).Johnson1966
was invoked but never defined (see the help page).Gontcharov2006
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Batten1980
was invoked but never defined (see the help page).Kraicheva1980
was invoked but never defined (see the help page).Stassun2019
was invoked but never defined (see the help page).Ramirez2013
was invoked but never defined (see the help page).Casagrande2011
was invoked but never defined (see the help page).Nordstrom2004
was invoked but never defined (see the help page).Tokovinin2014
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Pourbaix2004
was invoked but never defined (see the help page).