TOI-1685

Autors(-i): Karistus

Izlaišanas datums:

Pēdējoreiz atjaunināts:

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.

Palīdziet mums tulkot šo lapu šeit.

Atvērt programmā Celestia (ieteicams) vai Lejupielādēt

Kā instalēt papildinājumus? Uzziniet šeit.