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WASP-12

Star in the constellation Auriga From Wikipedia, the free encyclopedia

WASP-12 is a magnitude 11 yellow dwarf star located approximately 1347 light-years away[2] in the constellation Auriga.[4] 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.[7]

Quick Facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
WASP-12
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Auriga[1]
Right ascension 06h 30m 32.7966s[2]
Declination +29° 40 20.264[2]
Apparent magnitude (V) 11.560±0.068[3]
Characteristics
Spectral type G0V or F[citation needed]
Apparent magnitude (B) 12.138±0.019[3]
Apparent magnitude (R) ~11.6[4]
Apparent magnitude (J) 10.477±0.021[5]
Apparent magnitude (H) 10.228±0.022[5]
Apparent magnitude (K) 10.188±0.020[5]
Astrometry
Proper motion (μ) RA: −1.519(19) mas/yr[2]
Dec.: −6.761(15) mas/yr[2]
Parallax (π)2.4213±0.0166 mas[2]
Distance1,347 ± 9 ly
(413 ± 3 pc)
Details
Mass1.434+0.11
−0.09
[6] M
Radius1.657+0.046
−0.044
[6] R
Luminosity4.05+0.54
−0.53
[6] L
Temperature6360+130
−140
[6] K
Metallicity+0.33+0.14
−0.17
[6]
Other designations
TYC 1891-1178-1, 2MASS J06303279+2940202, UCAC2 42216354, Gaia DR2 3435282862461427072[4]
Database references
SIMBADdata
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Planetary system

In 2008, the extrasolar planet WASP-12b was discovered orbiting WASP-12 by the transit method.[8] Its high carbon-to-oxygen ratio indicates that rocky planets might have formed in the star system, and it may be a carbon planet.[9] It is subject to intensive photo-evaporation, and may be completely destroyed within one billion years from now.[10]

In 2015, no indications of additional planets were found in the WASP-12 system.[6]

More information Companion (in order from star), Mass ...
The WASP-12 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 1.41±0.1 MJ 0.0229±0.0008 1.091423±0.000003 0.049±0.015 86.0±3.0[11]° 1.736±0.092[11] RJ
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See also

References

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