TOI-4633

Author(s): Karistus

Release date:

TOI-4633 is a binary system comprised of two G-type main sequence stars located about 309.1 lightyears from the solar system. at least one planet is known to orbit one of the stars in the system, a sub-Neptune with rather high though very unconstrained mass on a long period orbit near the edge of it's host's habitable zone. There is also an additional candidate gas giant on a 35 day orbit around one of the stars in this system. Due to the proximity of the host stars, it is currently unknown which planet orbits which star or if they both orbit the same star. In this case, they are both modeled around the primary.

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