TOI-1669

المؤلف: Karistus

تاريخ الإصدار:

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.

ساعدنا في ترجمة هذه الصفحة هنا.

فتح في Celestia (مستحسن) أو تنزيل

كيفية تثبيت الإضافات؟ تعرّف على ذلك هنا.