Kepler-35

Forfatter(e): Karistus SolHorizon

Utgivelsesdato:

Sist oppdatert:

Kepler-35, aka KOI-2937, is a binary system composed of a G-type main sequence star and a K-type main sequence star located about 6254.19 lightyears from the solar system. Both stars are orbited by a low-density sub-Jupiter which completes a full revolution in a little over 1/3 of a year.

Hjelp oss å oversette denne siden her.

Åpne i Celestia (anbefales) eller Last ned

Hvordan installerer du tillegg? Finn ut her.