Author(s): Karistus

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TOI-199 is a binary system composed of a G-type main sequence star and a red dwarf located about 331.81 lightyears from the solar system. The primary component hosts a single, transiting, low density sub-Jupiter with an intermediate period orbit followed by another non-transiting sub-Jupiter within it's habitable zone. Both planets are in a 2:1 MMR.

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