HD 97507

Author(s): Karistus

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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.

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