Kepler-1660

Forfatter(e): Pan-STARRS

Utgivelsesdato:

Kepler-1660, also known as KOI-6518, is a distant binary star system of an F-type main sequence star and a red dwarf about 4,014 light-years away in the constellation Lyra. Both stars in the system were orbited by a single gas giant planet seven times more massive than Jupiter, where it completes one orbit once every 232.61 days

Hjelp oss å oversette denne siden her.

Åpne i Celestia (anbefales) eller Last ned

Hvordan installerer du tillegg? Finn ut her.