Warm exo-Titans around M dwarfs have photochemical methane lifetimes 10 to 50 times shorter than Titan's, making their detection a priori unlikely.
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The Photochemical Plausibility of Warm Exo-Titans Orbiting M-Dwarf Stars
Warm exo-Titans around M dwarfs have photochemical methane lifetimes 10 to 50 times shorter than Titan's, making their detection a priori unlikely.