TOI-1669

作者：Karistus

發佈日期：

TOI-1669 is a G-type main-sequence star located about 364.49 lightyears from the solar system. A single gas giant, a little over half as massive as Jupiter is known to orbit this star on a mildly eccentric orbit throughout its habitable zone. RV analysis shows a linear trend, which could be potentially caused by a planet on a ~2200-day orbit, but more data is needed. A sub-Neptune-sized candidate planet was spotted by TESS, but remains unconfirmed.

請在此 翻譯 協助翻譯本頁。

在 Celestia 中開啟（建議） 或 下載

如何安裝附加元件？請在此 查閱 了解。