TOI-1937

作者：Karistus

发布日期：

上次更新：

TOI-1937 is a binary system composed of a G-type star and a red dwarf located about 1354 light-years away from the solar system. The primary component of the system hosts a single hot Jupiter that completes an orbit every 22 hours, the planet is both larger than Jupiter (1.2 Jupiter Radii) and more massive (2.01 Jupiter Masses).

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。