James Webb Space Telescope Detects Atmospheric Chemical Signatures on Habitable-Zone Exoplanet K2-18b

Astrophysicists analyzing transmission spectroscopy data from the James Webb Space Telescope have confirmed carbon-bearing molecules in the atmosphere of K2-18b. Located 120 light-years from Earth in the constellation Leo, K2-18b orbits within the habitable zone of its cool dwarf star, making it a prime candidate for studying Hycean worlds.

Atmospheric Composition Revealed

The data demonstrates an abundance of methane and carbon dioxide, accompanied by a notable absence of ammonia. This chemical fingerprint supports the hypothesis that K2-18b possesses a hydrogen-rich atmosphere enveloping a liquid ocean mantle.

The Tantalizing Dimethyl Sulfide Signal

Most intriguing to astrobiologists is a potential detection of dimethyl sulfide (DMS)—a molecule that on Earth is produced almost exclusively by marine phytoplankton. Further deep-exposure observations are scheduled to verify the signal at 5-sigma statistical significance.


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