Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Leo Minor |
Right ascension | 10h 33m 30.91104s[1] |
Declination | +34° 59′ 19.3006″[1] |
Apparent magnitude (V) | 5.58±0.01[2] |
Characteristics | |
Evolutionary stage | subgiant[3] |
Spectral type | A2 V[4] |
U−B color index | +0.04[4] |
B−V color index | +0.02[4] |
Astrometry | |
Radial velocity (Rv) | 7±10[5] km/s |
Proper motion (μ) | RA: −28.397 mas/yr[1] Dec.: −3.072 mas/yr[1] |
Parallax (π) | 6.3892 ± 0.0706 mas[1] |
Distance | 510 ± 6 ly (157 ± 2 pc) |
Absolute magnitude (MV) | −1.02[6] |
Details | |
Mass | 2.40±0.42[7] M☉ |
Radius | 4.85±0.25[8] R☉ |
Luminosity | 323+54 −46[3] L☉ |
Surface gravity (log g) | 3.50±0.25[7] cgs |
Temperature | 9,333+152 −149[3] K |
Metallicity [Fe/H] | −0.03[9] dex |
Rotational velocity (v sin i) | 165±8[10] km/s |
Age | 406+134 −172[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
34 Leonis Minoris (34 LMi), also known as HD 91365 or 11 H. Leonis Minoris is a solitary star[13] located in the northern constellation Leo Minor. It is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.58.[2] Gaia DR3 parallax measurements imply a distance of 510 light-years,[1] and it is currently receding with a poorly constrained heliocentric radial velocity of 7 km/s.[5] At its current distance, 34 LMi's brightness is diminished by interstellar extinction of 0.16 magnitudes and it has an absolute magnitude of −1.02.[6]
The object has received several stellar classifications over the years. Most sources generally agree that it is an early A-type main-sequence star with the classes ranging from A0 to A2.[4][14][10] Anne Cowley and colleagues found that 34 LMi has broad or nebulous absorption lines in its spectrum,[15] which could be a result of rapid rotation. However, D. R. Palmer gave a class of A0 IV,[16] indicating that it is an evolved A-type subgiant.[16] Richard O. Gray and Robert F. Garrison found a class of A1 III-IV, indicating that it has a luminosity class intermediate between a subgiant and giant star.[17]
34 LMi has 2.4 times the mass of the Sun[7] and an enlarged radius of 4.85 R☉.[8] It radiates 323 times the luminosity of the Sun from its photosphere at an effective temperature of 9,333 K.[3] At the age of 406 million years[7] 34 LMi is 1.9% past its main sequence lifetime,[3] meaning that it has evolved to the subgiant branch. The star has a near-solar metallicity at [Fe/H] = −0.03 (93% solar).[9] Like many hot stars 34 LMi spins rapidly, having a projected rotational velocity of 165 km/s.[10]
GaiaDR3
was invoked but never defined (see the help page).Oja1991
was invoked but never defined (see the help page).Zorec2012
was invoked but never defined (see the help page).Osawa1959
was invoked but never defined (see the help page).Kharchenko2007
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Gullikson2016
was invoked but never defined (see the help page).Kervella2004
was invoked but never defined (see the help page).Anders2019
was invoked but never defined (see the help page).Abt1995
was invoked but never defined (see the help page).Verbunt2010
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Cucchiaro1978
was invoked but never defined (see the help page).Cowley1969
was invoked but never defined (see the help page).Palmer1968
was invoked but never defined (see the help page).Gray1987
was invoked but never defined (see the help page).