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Most significantly, water vapor on K2-18 b can be the most effective proof yet that small planets in the liveable zones of crimson dwarfs can possess atmospheres in any respect. It has the potential to inform us about how atmospheres form and evolve for planets at or close to the liveable zone around crimson dwarf stars, which will be essential for understanding the potential habitability of smaller ‘Earth-sized' planets.” K2-18b was discovered in 2015 and is one in all tons of of tremendous-Earths - planets with masses
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