Macromolecular organic compounds from the depths of Enceladus

Abstract

<div lang="en" class="abs"><p class="abs_header">Abstract</p><p>Saturn’s moon Enceladus harbours a global water ocean¹, which lies under an ice crust and above a rocky core². Through warm cracks in the crust³ a cryo-volcanic plume ejects ice grains and vapour into space⁴^–⁷ that contain materials originating from the ocean⁸^,⁹. Hydrothermal activity is suspected to occur deep inside the porous core¹⁰^–¹², powered by tidal dissipation¹³. So far, only simple organic compounds with molecular masses mostly below 50 atomic mass units have been observed in plume material⁶^,¹⁴^,¹⁵. Here we report observations of emitted ice grains containing concentrated and complex macromolecular organic material with molecular masses above 200 atomic mass units. The data constrain the macromolecular structure of organics detected in the ice grains and suggest the presence of a thin organic-rich film on top of the oceanic water table, where organic nucleation cores generated by the bursting of bubbles allow the probing of Enceladus’ organic inventory in enhanced concentrations.</p></div>