In a groundbreaking scientific breakthrough, researchers using the James Webb Space Telescope have detected what they consider the most compelling evidence yet of potential life beyond our solar system. This discovery was made by identifying the chemical fingerprints of gases in an exoplanet’s atmosphere that, on Earth, are exclusively produced by biological processes. The gases in question, dimethyl sulfide (DMS) and dimethyl disulfide (DMDS), were spotted on the distant planet known as K2-18 b. These compounds are typically generated on Earth by living organisms, notably marine microbes like phytoplankton. This finding suggests that K2-18 b could be home to abundant microbial life, though scientists emphasize that they have not confirmed the presence of actual organisms. They highlight the importance of seeing these results as indicative of a probable biosignature—an indicator of biological activity—while urging caution and calling for further detailed observations.
K2-18 b is a massive exoplanet, approximately 8.6 times the mass of Earth and with a diameter about 2.6 times that of our home planet. It resides in the “habitable zone,” a region where liquid water—a fundamental requirement for life—is likely to exist on a planet’s surface. This exoplanet orbits a red dwarf star, smaller and dimmer than our sun, situated roughly 124 light-years from Earth in the constellation of Leo.
Since the 1990s, astronomers have discovered about 5,800 exoplanets beyond our solar system. Among these, they have theorized the existence of “hycean worlds,” which are characterized by liquid water oceans inhabitable by microorganisms and having hydrogen-rich atmospheres. Initial observations of K2-18 b by the James Webb Space Telescope hinted at the presence of DMS. The latest observations employed an alternative instrument and a different light wavelength, providing stronger evidence of these gases and opening new avenues in the quest to find extraterrestrial life.