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Lab Radiation Tests Complicate Ocean Origin for Enceladus Organics

New lab simulations indicate Saturn’s trapped particles can generate similar molecules on the moon’s icy surface.

Overview

  • Dr. Grace Richards of INAF presented the findings on September 9 at the EPSC–DPS 2025 meeting in Helsinki.
  • Europlanet-funded experiments at HUN-REN bombarded Enceladus-like ice mixtures of water, carbon dioxide, methane and ammonia cooled to about −200°C with ions to mimic Saturn’s magnetosphere.
  • The irradiation produced carbon monoxide, cyanate, ammonium and precursors to amino acids, several of which match compounds previously detected on the surface and in the plumes.
  • The results show that radiation-driven chemistry could create some plume organics in situ, so Cassini’s detections do not uniquely indicate subsurface ocean chemistry or habitability.
  • Researchers say distinguishing ocean-derived molecules from radiation products will require new targeted measurements, with a dedicated Enceladus mission under ESA’s Voyage 2050 considerations cited as one path forward.