HD 97507
작성자: Karistus
출시일:
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.
이 페이지의 번역에 여기에서 도움을 주세요.
애드온을 설치하는 방법은? 여기에서 확인하세요.