GJ 1214 b
| Discovery | |
|---|---|
| Discovered by | David Charbonneau, et al. |
| Discovery site | Fred Lawrence Whipple Observatory |
| Discovery date | December 16, 2009 |
| Transit (MEarth Project) | |
| Designations | |
| Enaiposha, Gliese 1214 b | |
| Orbital characteristics | |
| 0.01505±0.00011 | |
| Eccentricity | 0.0062+0.0044 −0.0079 |
| 1.580404531+18 −17 d | |
| Inclination | 88.980°+0.094° −0.085° |
| Semi-amplitude | 14.38+0.57 −0.56 m/s |
| Star | Orkaria/GJ 1214 |
| Physical characteristics | |
| 2.733+0.033 −0.031 R🜨 | |
| Mass | 8.41+0.36 −0.35 M🜨 |
Mean density | 2.20+0.17 −0.16 g/cm3 |
| 10.65+0.71 −0.67 m/s2 (1.09 g) | |
| 19.31+0.53 −0.54 km/s | |
| Albedo | 0.51±0.06 (Bond) |
| Temperature | 553±9 K (280 °C; 536 °F, dayside) 437±19 K (164 °C; 327 °F, nightside) |
GJ 1214 b (sometimes Gliese 1214 b, also named Enaiposha since 2023) is an exoplanet that orbits the star GJ 1214, discovered in December 2009. Its parent star is 48 light-years (15 pc) from the Sun, in the constellation Ophiuchus. At the time of its discovery, GJ 1214 b was the most likely known candidate for being an ocean planet. For that reason, scientists at that time often called the planet a "waterworld". However, a recent study of the planet's internal structure informed by observations taken with the James Webb Space Telescope suggests that a "waterworld" composition is implausible and the planet is more likely to host a thick gaseous envelope consisting of hydrogen, helium, water and other volatile chemicals such as methane or carbon dioxide.
It is a mini-Neptune, meaning it is larger than Earth but is significantly smaller (in mass and radius) than the gas giants of the Solar System. After CoRoT-7b, it was the second planet between Earth and Neptune in mass to have both its mass and radius measured and is the first of a new class of planets with small size and relatively low density. GJ 1214 b is also significant because its parent star is relatively near the Sun and because it transits that parent star, which allows the planet's atmosphere to be studied using spectroscopic methods.