A team at the Institute for Research on Exoplanets at the Université de Montréal published their findings yesterday. Led by Björn Benneke, their work (which has yet to be peer reviewed) points to the possibility that K2-18 b is habitable thanks to the presence of water and hydrogen, as well as the exoplanet's location in the Goldilocks zone. The Goldilocks zone is a range relative to a star where the temperature is not too hot and not too cold to support life. But while the temperature range and presence of water are good signs, K2-1
K2-18 b is the least massive exoplanet to have water vapor detected in its atmosphere. The planet may even have rain clouds – though the researchers were unable to confirm that yet. If the water condenses into liquid, the drops would fall to the core, then revert to gas as the atmospheric pressure increases. The gas would rise back up to the cloud layer and repeat the cycle.
Benneke and his fellow researchers will follow up their work in the 2020s, after the James Webb Space Telescope was launched in 2021. This new telescope is even more powerful than the Hubble Space Telescope, which the team used to analyze K2-18 b as it passed in front of its star. A more detailed look through the James Webb Space Telescope will help confirm the presence of rain on the planet, and will allow researchers to find even more Earth-like planets.
Each passing decade has led to a discovery that changes how we think about our universe: Dark energy was confirmed in the 2000s and the 2010s as the first true confirmation of a black hole. The 2020s may be the decade when we find that the Earth, with its dry land and liquid oceans, is not as unique as we currently believe.