An international research team has analysed data from the Cosmic Dust Analyser (CDA) instrument aboard the Cassini spacecraft, obtained during its flyby of Saturn's moon Enceladus. Fresh ice particles ejected from the subsurface ocean were found to contain organic compounds — including aromatic, ether, ester, and alkyl compounds, as well as compounds containing nitrogen and oxygen. This discovery strengthens the hypothesis of hydrothermal activity on the ocean floor and Enceladus's potential habitability.
The icy gas jets erupting from fractures near Enceladus's south pole originate from a global subsurface ocean.
During the Cassini–Huygens mission (2004–2017), the probe repeatedly flew through these jets, analysing the composition of microscopic ice particles.
The fifth flyby (E5) in 2008 proved to be the most informative: the spacecraft passed through the plume at a speed of 17.7 km/s. This high velocity caused intense ionisation of material upon impact, revealing molecular fragments previously undetected during slower flybys (4–12 km/s).
Several types of organic structures were identified in the freshly ejected ice crystals:
Previously, Cassini had already found water, salts, carbon dioxide, methane, ammonia, and phosphates on Enceladus — five of the six elements vital for biochemistry (CHNOPS).
Now the presence of a wide range of organic molecules has been confirmed, including more complex ones than simple hydrocarbons.
The totality of this data points to hydrothermal processes in the moon's interior — similar to those occurring in hot springs at the bottom of Earth's oceans. There, as is known, organic synthesis is concentrated and primitive life forms can emerge.
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