TOI-1685

Autorius (-iai): Karistus

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TOI-1685 is a red dwarf located about 122.82 light-years from the solar system. a single super-Earth sized planet is known to orbit this star every 16.06 hours. Originally confirmed as an oceanic, future studies favored a rocky composition additionally preliminary JWST results are consistent with an airless body. Two planet candidates were present in both papers that confirmed the planet, but later studies refuted both candidates.

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Atidaryti naudojant Celestia (rekomenduojama) arba Atsisiųsti

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