Kepler-432

Forfatter(e): John van Vliet

Utgivelsesdato:

Kepler-432 is a binary star system comprising of a K-type giant star and a red dwarf about 2,834 light-years away in the constellation Cygnus. The primary star has two confirmed super-Jovians orbiting it, one of which completes an orbit once every 17 days

Hjelp oss å oversette denne siden her.

Åpne i Celestia (anbefales) eller Last ned

Hvordan installerer du tillegg? Finn ut her.