| HAT-P-24b | |
| Discoverer: | HATNet Project |
| Discovered: | 2010 |
| Apsis: | astron |
| Semimajor: | AU |
| Period: | d |
| Mean Radius: | 1.243 |
| Density: | g cm−3 |
| Surface Grav: | 10.9± |
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.
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°.