
Organic Compounds and Complex Chemistry Detected in Enceladus's Subsurface Ocean
The study reanalyzes Cassini's high-speed fly-by data of Enceladus, revealing the presence of diverse organic compounds, including aromatics, esters, ethers, and N- and O-bearing species, in freshly ejected ice grains. These findings suggest complex organic chemistry within Enceladus's subsurface ocean, likely driven by hydrothermal processes, and provide insights into the moon's potential habitability.




