HAT-P-17

作者：Edasich

发布日期：

HAT-P-17, also known as TOI-1283, is a binary star system consisting of a K-type main-sequence star and a red dwarf about 302.11 light-years away in the constellation Cygnus. Two super-Jovian planets orbit around the primary star, one of which complete an orbit once every 5.9 days

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。