Kepler-454

Forfatter(e): Karistus

Utgivelsesdato:

Sist oppdatert:

Kepler-454, aka KOI-273, is a binary system comprised of a G-type main sequence star and a red dwarf located about 752.64 lightyears from the solar system. The brighter and more massive of the pair is currently known to host three planets, a short period, transiting mini-Neptune. As well as two super-Jupiters, one of which orbits within Kepler-454 A's habitable zone. There is an additional candidate cold super-Jupiter on a 48 year orbit.

Hjelp oss å oversette denne siden her.

Åpne i Celestia (anbefales) eller Last ned

Hvordan installerer du tillegg? Finn ut her.