HAT-P-24b

HAT-P-24b is an extrasolar planet discovered by the HATNet Project in 2010 orbiting the F8 dwarf star HAT-P-24. It is a hot Jupiter, with a mass three quarters that of Jupiter and a radius 20% larger.

HAT-P-24b
Discovery
Discovered byHATNet Project
Discovery date2010
Transit
Orbital characteristics
0.04651+0.00055
−0.00056
AU
Eccentricity<0.038
3.3552479±0.0000062 d
StarHAT-P-24
Physical characteristics
Mean radius
1.243 +0.072
0.061
RJ
Mass0.723+0.031
−0.030
MJ
Mean density
0.467+0.089
−0.070
g cm−3
10.9 ± 1.1 m/s2 (35.8 ± 3.6 ft/s2)

    The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is probably aligned with the equatorial plane of the star, misalignment equal to 20±16°.

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