Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Leo |
83 Leonis A | |
Right ascension | 11h 26m 45.32173s[1] |
Declination | +03° 00′ 47.1566″[1] |
Apparent magnitude (V) | 6.49 |
83 Leonis B | |
Right ascension | 11h 26m 46.27833s[2] |
Declination | +03° 00′ 22.7567″[2] |
Apparent magnitude (V) | 7.58[3] |
Characteristics | |
Spectral type | G9IV-V[4] / K2V[5] |
U−B color index | 1.024 (83 Leonis B)[6] |
B−V color index | 0.913 (83 Leonis B)[6] |
Variable type | None |
Astrometry | |
83 Leonis A | |
Radial velocity (Rv) | 4.18±0.13[1] km/s |
Proper motion (μ) | RA: −725.963(29) mas/yr[1] Dec.: 180.980(30) mas/yr[1] |
Parallax (π) | 55.0090 ± 0.0240 mas[1] |
Distance | 59.29 ± 0.03 ly (18.179 ± 0.008 pc) |
83 Leonis B | |
Radial velocity (Rv) | 3.63±0.13[2] km/s |
Proper motion (μ) | RA: −728.131(34) mas/yr[2] Dec.: 188.554(27) mas/yr[2] |
Parallax (π) | 55.0618 ± 0.0304 mas[2] |
Distance | 59.23 ± 0.03 ly (18.16 ± 0.01 pc) |
Details | |
83 Leonis A | |
Mass | 0.95 ± 0.06[7] M☉ |
Radius | 0.96+0.04 −0.02[8] R☉ |
Luminosity | 0.74[7] L☉ |
Surface gravity (log g) | 4.42[7] cgs |
Temperature | 5509 ± 8.6[9] K |
Metallicity | 0.30[7] |
Age | 8.09 ± 6.75[7] Gyr |
83 Leonis B | |
Mass | 0.85±0.02[3] M☉ |
Radius | 0.78±0.02[3] R☉ |
Luminosity (bolometric) | 0.418 ± 0.057[5] L☉ |
Surface gravity (log g) | 4.57±0.06[3] cgs |
Temperature | 4929±44[3] K |
Metallicity | 0.3±0.03[3] |
Rotation | 40-45 days[10] |
Rotational velocity (v sin i) | 0.41±0.5[3] km/s |
Age | 4.8±4.1[3] Gyr |
Other designations | |
Database references | |
SIMBAD | HD 99491 |
HD 99492 |
83 Leonis, abbreviated 83 Leo, is a binary star system approximately 59 light-years away in the constellation of Leo (the Lion). The primary star of the system is a cool orange subgiant star, while the secondary star is an orange dwarf star. The two stars are separated by at least 515 astronomical units from each other. Both stars are presumed to be cooler than the Sun.
The primary star is also known as HD 99491 and the secondary star as HD 99492. In 2005, an exoplanet was confirmed to be orbiting the secondary star within the system.[12]
GaiaDR3A
was invoked but never defined (see the help page).GaiaDR3B
was invoked but never defined (see the help page).Kane2016
was invoked but never defined (see the help page).Abt1986
was invoked but never defined (see the help page).Meschiari2011
was invoked but never defined (see the help page).Koen2010
was invoked but never defined (see the help page).Luck2017
was invoked but never defined (see the help page).GaiaDR2A
was invoked but never defined (see the help page).Koytyukh2003
was invoked but never defined (see the help page).Stalport2023
was invoked but never defined (see the help page).Marcy2005
was invoked but never defined (see the help page).