Omega Serpentis

Forfatter(e): Gurren Lagann

Utgivelsesdato:

Omega Serpentis is a binary star system consisting of a G-type giant star and a K-type main-sequence star about 251 light-years away in the constellation Serpens Caput. A planet candidate the size of Jupiter was announced orbiting the larger star of the two in 2005, but its existence wasn't confirmed until 2013

Hjelp oss å oversette denne siden her.

Åpne i Celestia (anbefales) eller Last ned

Hvordan installerer du tillegg? Finn ut her.