CoRoT-24b
| Discovery | |
|---|---|
| Discovered by | CoRoT space telescope |
| Discovery date | 2011 |
| Transit | |
| Designations | |
| 2MASS 06474141-0343094 b, Gaia DR2 3105404467618982272 b | |
| Orbital characteristics | |
| Epoch J2000 | |
| 0.056 ± 0.002 AU (8,380,000 ± 300,000 km) | |
| Eccentricity | 0 |
| 5.1134 ± 0.0006 d | |
| Inclination | 86.5 ± 2.0 ° |
| Star | CoRoT-24 |
| Physical characteristics | |
Mean radius | 0.33 ± 0.04 RJ |
| Mass | <0.018 MJ |
Mean density | <0.9 g/cm3 |
| 0.4183 G🜨 | |
North pole right ascension | 06h 47m 41.41s |
North pole declination | −03° 43′ 09.48″ |
| Temperature | 1,070 K |
CoRoT-24b is a transiting exoplanet found by the CoRoT space telescope in 2011 and announced in 2014. Along with CoRoT-24c, it is one of two exoplanets orbiting CoRoT-24, making it the first multiple transiting system detected by the telescope. It is a hot Neptune orbiting at a distance of 0.056 AU from its host star.
Properties
CoRoT-24b and CoRoT-24c are similar in size; however, CoRoT-24b is more than four times less massive, indicating its low density. Dr. Lammer's team modelled the planetary system and found that the atmosphere should have already evaporated a long time ago. This led to the conclusion that CoRoT-24b is not as big as previously thought, being perhaps 30 to 60 percent smaller than initially measured.