TOI-815

Author(s): Karistus

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TOI-815 is a binary system comprised of a K-type main sequence star and a red dwarf located about 193.86 lightyears from the solar system. two sub-Neptune-sized planets are currently known to orbit the primary component of the binary, the outer planet is just over 3x the mass of the inner one resulting in the planets of the system having wildly different densities. The TOI-815 A b has a structure resembling many other mini-Neptunes, while TOI-815 A c is likely rocky dominated with a thin volatile-rich layer. Both planets of the system are on near-polar orbits.

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