Processing of 72-K water-rich ices by keV and MeV oxygen ions: implications for the Saturnian moon Enceladus

Autor: Philippe Boduch, W.R.M. Rocha, Sergio Pilling, A. N. Agnihotri, Hermann Rothard, M G Rachid

Publikováno v: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 494 (2), pp.2396-2409. ⟨10.1093/mnras/staa778⟩
Rachid, M G, Pilling, S, Rocha, W R M, Agnihotri, A, Rothard, H & Boduch, P 2020, ' Processing of 72-K water-rich ices by keV and MeV oxygen ions : implications for the Saturnian moon Enceladus ', Monthly Notices of the Royal Astronomical Society, vol. 494, no. 2, pp. 2396-2409 . https://doi.org/10.1093/mnras/staa778

The processing of H2O:CO2:CH4 (10:1:1) and H2O:CO2:CH4:NH3 (10:1:1:1) ices at 72 K by oxygen ions was studied in an attempt to simulate the physicochemical effects induced by energetic ions on the surface of Enceladus (or similar cold surfaces in the

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