Gliese 570

Gliese 570

The quaternary star system Gliese 570. The T-type methane brown dwarf Gliese 570D is indicated with an arrow.
Credit: 2MASS
Location of Gliese 570 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Libra
Right ascension 14h 57m 28.00144s
Declination −21° 24 55.7131
Apparent magnitude (V) 5.75 / 8.07 / 10.5
Characteristics
Spectral type K4V / M1V / M3V / T7V
U−B color index 1.06 /1.22
B−V color index 1.11 / 1.51
Variable type None
Astrometry
A
Radial velocity (Rv)+26.75±0.12 km/s
Proper motion (μ) RA: +1031.472 mas/yr
Dec.: −1723.619 mas/yr
Parallax (π)169.8843±0.0653 mas
Distance19.199 ± 0.007 ly
(5.886 ± 0.002 pc)
Absolute magnitude (MV)6.89
BC
Radial velocity (Rv)+25.9 km/s
Proper motion (μ) RA: +961.78 mas/yr
Dec.: −1677.83 mas/yr
Parallax (π)169.1±0.9 mas
Distance19.3 ± 0.1 ly
(5.91 ± 0.03 pc)
Absolute magnitude (MV)9.19 / 11.05
D
Proper motion (μ) RA: +1038.08 mas/yr
Dec.: −1677.59 mas/yr
Parallax (π)169.30±1.70 mas
Distance19.3 ± 0.2 ly
(5.91 ± 0.06 pc)
Details
A
Mass0.802 ± 0.040 M
Radius0.715±0.009 R
Luminosity (bolometric)0.19±0.01 L
Temperature4505±76 K
Metallicity
Rotational velocity (v sin i)1.50 km/s
B
Mass0.562±0.006 M
C
Mass0.377±0.003 M
D
Mass34.6+7.5
−6.5
 MJup
Radius0.89+0.05
−0.04
 RJup
Luminosity10−5.54±0.03 L
Surface gravity (log g)5.04±0.13 cgs
Temperature786±20 K
Other designations
33 G. Librae, GJ 570, HD 131976, ADS 9446, WDS J14575-2125
A: HR 5568, LAL 27173, HD 131977, BD-20°4125, LHS 387, LTT 5949, GCTP 3375.00, SAO 183040, FK5 1391, LFT 1161, LPM 551, Vys 726, HIP 73184
BC: HD 131976, HIP 73182, LHS 386, LTT 5948, BD-20°4123, SAO 183039, LFT 1160, LPM 550
D: 2MASS J14571496-2121477
Database references
SIMBADA
BC
D
Exoplanet Archivedata
ARICNSdata

Gliese 570 (or 33 G. Librae) is a quaternary star system approximately 19 light-years away. The primary star is an orange dwarf star (much dimmer and smaller than the Sun). The other secondary stars are themselves a binary system, two red dwarfs that orbit the primary star. A brown dwarf has been confirmed to be orbiting in the system. In 1998, an extrasolar planet was thought to orbit the primary star, but it was discounted in 2000.