HD 97507

Автор(ы): Karistus

Дата релиза:

HD 97507, aka TOI-1203, is a binary system comprised of a G-type main sequence star and a red dwarf located about 211.88 light-years from the solar system. the primary component to the system is currently known to have four planets consisting of a hot, transiting super-Earth, a non-transiting sub-Neptune mass planet, a transiting sub-Neptune, and an outer sub-Saturn mass gas giant. HD 97507 A joins other systems like HD 3167 and TOI-431 where a non-transiting planet is sandwiched between two transiting ones.

Вы можете помочь нам перевести эту страницу здесь.

Открыть в Celestia (рекомендуется) или Скачать

Как установить дополнения? Смотрите здесь.