Kepler-25 B

작성자: Karistus

출시일:

Kepler-25 B, aka KOI-1803, is a part of a binary system consisting of an F-type main sequence star and a K-type main sequence star. Serving as the secondary component to the binary. Three candidate planets were detected by Kepler, though two were ruled as false positives, one candidate remains, a possible hot mini-Neptune on a 4.5 day orbit.

이 페이지의 번역에 여기에서 도움을 주세요.

Celestia에서 열기 (권장) 또는 다운로드

애드온을 설치하는 방법은? 여기에서 확인하세요.