GJ 1214 b

GJ 1214 b / Enaiposha
Size comparison of Enaiposha with Earth (left) and Neptune (right). The actual color of Enaiposha is not yet known.
Discovery
Discovered byDavid Charbonneau, et al.
Discovery siteFred Lawrence Whipple Observatory
Discovery dateDecember 16, 2009
Transit (MEarth Project)
Designations
Enaiposha, Gliese 1214 b
Orbital characteristics
0.01505±0.00011
Eccentricity0.0062+0.0044
−0.0079
1.580404531+18
−17
 d
Inclination88.980°+0.094°
−0.085°
Semi-amplitude14.38+0.57
−0.56
 m/s
StarOrkaria/GJ 1214
Physical characteristics
2.733+0.033
−0.031
 R🜨
Mass8.41+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
Albedo0.51±0.06 (Bond)
Temperature553±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.