Author(s): Karistus

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TOI-2096 is a red dwarf located about 158.04 lightyears away from the solar system. The star has two slightly eccentric planets orbiting it, a super-Earth (1.2 Earth Radii) and a sub-Neptune (1.9 Earth Radii). the planet's orbits are near a 2:1 MMR (mean-motion resonance), leading to the possibility of measuring the masses of these worlds via Transit Timing Variations.

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