Kepler-454

作者：Karistus

发布日期：

上次更新：

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.

点击这里帮助我们翻译这个页面。

在 Celestia 中打开（推荐） 或者 下载

如何安装插件？在这里获取指导。