TOI-1338

Auteur(s): Karistus trappistplanets fyr02

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TOI-1338 is an eclipsing binary comprised of an F-type main sequence star and a red dwarf located about 1,320 lightyears from the solar system. Two planets are currently known to orbit both stars in this system, the inner one being a transiting Neptune mass, sub-Saturn sized gas giant and the outer being a sub-Saturn mass, non-transiting gas giant. TOI-1338 is the first confirmed circumbinary system discovered by TESS, with TOI-1338 c being the first circumbinary planet confirmed solely by the Radial Velocity method.

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