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Kepler-22b

Super-Earth exoplanet orbiting Kepler-22

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This artist's conception illustrates Kepler-22b, a planet known to comfortably circle in the habitable zone of a sun-like star. It is the first planet that NASA's Kepler mission has confirmed to orbit
NASA/Ames/JPL-Caltech · Public domain

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Kepler-22b has a radius about twice that of Earth. Its mass and surface composition are unknown, but an Earth-like composition is considered unlikely. It may instead be an ocean planet or have a volatile-rich composition with a liquid or gaseous outer layer. The planet's known orbital parameters are its orbital period, about 290 days, and its inclination, approximately 90°. Its surface temperature may be moderate if it does not experience extreme greenhouse heating. In the absence of an atmosphere, its equilibrium temperature, assuming an Earth-like albedo, would be about 279 K (6 °C; 43 °F), slightly higher than Earth's equilibrium temperature of 255 K (−18 °C; −1 °F).

Physical characteristics

Mass, radius, and temperature

Kepler-22b's radius was initially thought to be 2.4 times that of Earth, but has since been revised to 2.1 R🜨 as of 2023. Its mass and surface composition remain unknown, with only some rough estimates established: at the time of the discovery announcement, it was known to have fewer than 124 Earth masses at the 3-sigma confidence limit, and fewer than 36 Earth masses at 1-sigma confidence. The adopted model in Kipping et al. (2013) does not reliably detect the mass (the upper limit is 52.8 M🜨). As of 2023, the upper limit has been constrained to at most 9.1 M🜨.

Kepler-22b, dubbed by scientists as a "water world", might be an "ocean-like" planet. It might also be comparable to the water-rich planet Enaiposha although Kepler-22b, unlike Enaiposha, is in the habitable zone. An Earth-like composition is ruled out to at least 1-sigma uncertainty by radial velocity measurements of the system; it is thus likely to have a more volatile-rich composition with a liquid or gaseous outer shell; this would make it similar to Kepler-11f, one of the smallest known gas planets. Natalie Batalha, one of the scientists on the Kepler Space Telescope project, has speculated, "If it is mostly ocean with a small rocky core, it's not beyond the realm of possibility that life could exist in such an ocean". This possibility has spurred SETI to perform research on top candidates for extraterrestrial life.

In the absence of an atmosphere, its equilibrium temperature (assuming an Earth-like albedo) would be approximately 279 K (6 °C), compared with Earth's 255 K (−18 °C).

Host star

The host star, Kepler-22, is a G-type star that is 3% less massive than the Sun and 2% smaller in volume. It has a surface temperature of 5,518 K (5,245 °C; 9,473 °F) compared with the Sun, which has a surface temperature of 5,778 K (5,505 °C; 9,941 °F). The star is about 4 billion years old. In comparison, the Sun is 4.6 billion years old.

The apparent magnitude of Kepler-22 is 11.5, which means it is too dim to be seen with the naked eye.

Orbit

The only parameters of the planet's orbit that are currently available are its orbital period, which is about 290 days, and its inclination, which is approximately 90°. From Earth, the planet appears to make a transit across the disk of its host star. In order to obtain further information about the details of the planet's orbit, other methods of planetary detection, such as the radial velocity method, need to be used. While such methods have been performed on the planet since its discovery, these methods have not yet detected an accurate value for the eccentricity of the planet and so (as of 2023) only an upper limit for the eccentricity of the planet has been set by astronomers.

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