TOI-199

Autorius (-iai): Karistus

Išleidimo data:

TOI-199 is a binary system composed of a G-type main sequence star and a red dwarf located about 331.81 lightyears from the solar system. The primary component hosts a single, transiting, low density sub-Jupiter with an intermediate period orbit followed by another non-transiting sub-Jupiter within it's habitable zone. Both planets are in a 2:1 MMR.

Padėkite mums išversti šį puslapį čia.

Atidaryti naudojant Celestia (rekomenduojama) arba Atsisiųsti

Kaip įdiegti priedus? Sužinokite čia.