WASP-12

WASP-12

WASP-12A (left) with WASP-12B and C (right, indicated) taken from Keck AO
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Auriga
Right ascension 06h 30m 32.7966s
Declination +29° 40′ 20.264″
Apparent magnitude (V) 11.560±0.068
Characteristics
Spectral type G0V + M3V + M3V
Apparent magnitude (B) 12.138±0.019
Apparent magnitude (R) ~11.6
Apparent magnitude (J) 10.477±0.021
Apparent magnitude (H) 10.228±0.022
Apparent magnitude (K) 10.188±0.020
Astrometry
Radial velocity (Rv)20.62±1.44 km/s
Proper motion (μ) RA: −1.519(19) mas/yr
Dec.: −6.761(15) mas/yr
Parallax (π)2.4213±0.0166 mas
Distance1,347 ± 9 ly
(413 ± 3 pc)
Orbit
PrimaryWASP-12 A
NameWASP-12 BC
Period (P)393.9 days
Semi-major axis (a)21±AU
Details
A
Mass1.325+0.026
−0.018
 M
Radius1.690+0.019
−0.018
 R
Luminosity4.05+0.54
−0.53
 L
Surface gravity (log g)4.11±0.11 cgs
Temperature6265±50 K
Metallicity [Fe/H]+0.12±0.07 dex
Rotational velocity (v sin i)<1.9 km/s
Age3.05±0.32 Gyr
Details
B
Mass0.38±0.05 M
C
Mass0.37±0.05 M
Other designations
TOI-1725, TIC 86396382, TYC 1891-1178-1, 2MASS J06303279+2940202, UCAC2 42216354
Database references
SIMBADA
BC
Exoplanet Archivedata

WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away in the constellation Auriga. WASP-12 has a mass and radius similar to the Sun and is known for being orbited by a planet that is extremely hot and has a retrograde orbit around WASP-12. WASP-12 forms a triple star system with two red dwarf companions. Both of them have spectral types of M3V and are only 38% and 37% as massive as the Sun, respectively.