The article discusses the search for extraterrestrial life using chemical biosignatures, focusing on the use of telescopes like the James Webb Space Telescope to analyze exoplanet atmospheres. It highlights the challenges in interpreting data and the need for robust criteria for identifying true biosignatures, using the example of dimethyl sulfide (DMS) detection on K2-18b.
The James Webb Space Telescope has detected potential life-associated gases (dimethyl sulfide, dimethyl disulfide) in the atmosphere of planet K2-18b, but scientists urge caution and further investigation to rule out non-biological sources. The findings are considered a potentially revolutionary moment in the search for extraterrestrial life.
