Author(s): Karistus

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TOI-836 is an orange dwarf star located about 90 light-years away from the solar system. Two hot planets: a mini-Neptune (2.587 Earth Radii) and a super-Earth (1.704 Earth Radii). They were confirmed to be orbiting the star in 2022, Their masses have been observed (4.53 Earth Masses for TOI-836 b, 9.60 Earth Masses for TOI-836 c) and During observations of the system, TTVs (Transit Timing Variations) were observed during transits of TOI-836 c, but none on TOI-836 b. Leading to the possibility that there is a non-transiting third planet within the system.

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