Archivo de imágenes de Hubble

Impresión artística del sistema planetario Kepler 138

In this illustration super-Earth Kepler-138 d is in the foreground. To the left, the planet Kepler-138 c, and in the background the planet Kepler 138 b, seen in silhouette transiting its central star. Kepler 138 is a red dwarf star located 218 light-years away. The low density of...

Fecha
Jan 1, 2022
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2022-048-01ggtf3hm9nzb45dc762fw81n5
Por

In this illustration super-Earth Kepler-138 d is in the foreground. To the left, the planet Kepler-138 c, and in the background the planet Kepler 138 b, seen in silhouette transiting its central star. Kepler 138 is a red dwarf star located 218 light-years away. The low density of Kepler-138 c and Kepler-138 d — which are nearly identical in size — means that they must be composed largely of water. They are both twice Earth's mass but have roughly half of Earth's density, and therefore cannot be solid rock. This is based on measurements of their mass versus physical diameter. They are considered a new class of "water planet," unlike any major planet found in our solar system. Kepler-138 b is one of the smallest exoplanets known, having the mass of the planet Mars and the density of rock.

Credits

Illustration

NASA, ESA, Leah Hustak (STScI)

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La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

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