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Macromolecular organic compounds from the depths of Enceladus

Author

Listed:
  • Frank Postberg

    (Universität Heidelberg
    Universität Heidelberg
    Institut für Geologische Wissenschaften, Freie Universität Berlin)

  • Nozair Khawaja

    (Universität Heidelberg)

  • Bernd Abel

    (Leibniz-Institute für Oberflächenmodifizierung (IOM))

  • Gael Choblet

    (Université de Nantes)

  • Christopher R. Glein

    (Southwest Research Institute)

  • Murthy S. Gudipati

    (California Institute of Technology)

  • Bryana L. Henderson

    (California Institute of Technology)

  • Hsiang-Wen Hsu

    (University of Colorado)

  • Sascha Kempf

    (University of Colorado)

  • Fabian Klenner

    (Universität Heidelberg)

  • Georg Moragas-Klostermeyer

    (Universität Stuttgart)

  • Brian Magee

    (Southwest Research Institute
    University of Colorado)

  • Lenz Nölle

    (Universität Heidelberg)

  • Mark Perry

    (Johns Hopkins University)

  • René Reviol

    (Universität Heidelberg)

  • Jürgen Schmidt

    (University of Oulu)

  • Ralf Srama

    (Universität Stuttgart)

  • Ferdinand Stolz

    (Leibniz-Institute für Oberflächenmodifizierung (IOM)
    Universität Leipzig)

  • Gabriel Tobie

    (Université de Nantes)

  • Mario Trieloff

    (Universität Heidelberg
    Universität Heidelberg)

  • J. Hunter Waite

    (Université de Nantes)

Abstract

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.

Suggested Citation

  • Frank Postberg & Nozair Khawaja & Bernd Abel & Gael Choblet & Christopher R. Glein & Murthy S. Gudipati & Bryana L. Henderson & Hsiang-Wen Hsu & Sascha Kempf & Fabian Klenner & Georg Moragas-Klosterme, 2018. "Macromolecular organic compounds from the depths of Enceladus," Nature, Nature, vol. 558(7711), pages 564-568, June.
  • Handle: RePEc:nat:nature:v:558:y:2018:i:7711:d:10.1038_s41586-018-0246-4
    DOI: 10.1038/s41586-018-0246-4
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    Cited by:

    1. Yamei Li & Norio Kitadai & Yasuhito Sekine & Hiroyuki Kurokawa & Yuko Nakano & Kristin Johnson-Finn, 2022. "Geoelectrochemistry-driven alteration of amino acids to derivative organics in carbonaceous chondrite parent bodies," Nature Communications, Nature, vol. 13(1), pages 1-14, December.

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