Production of Oxidants by Ion Bombardment of Icy Moons in the Outer Solar System

Author:

Boduch Philippe1,da Silveira Enio Frota2,Domaracka Alicja1,Gomis Oscar3,Lv Xue Yang1,Palumbo Maria Elisabetta4,Pilling Sergio5,Rothard Hermann1,Seperuelo Duarte Eduardo6,Strazzulla Giovanni4

Affiliation:

1. Centre de Recherche sur les Ions, les Matériaux et la Photonique (CIMAP), CIRIL-GANIL (CEA/CNRS/ENSI CAEN) Université de Caen Basse-Normandie, 14076 Caen, France

2. Departamento de Física, Pontifícia Universidade Católica do Rio de Janeiro, 22451-900 Gávea, RJ, Brazil

3. Centro de Tecnologías Físicas, Universitat Politècnica de València, 46022 Valencia, Spain

4. INAF-Osservatorio Astrofisico di Catania, 95123 Catania, Italy

5. IP&D, UNIVAP, 12299-00001 São Jose dos Campos, SP, Brazil

6. Grupo de Física e Astronomia, CEFET/Química de Nilópolis, 2653-060 Nilópolis, RJ, Brazil

Abstract

Our groups in Brazil, France and Italy have been active, among others in the world, in performing experiments on physical-chemical effects induced by fast ions colliding with solids (frozen gases, carbonaceous and organic materials, silicates, etc.) of astrophysical interest. The used ions span a very large range of energies, from a few keV to hundreds MeV. Here we present a summary of the results obtained so far on the formation of oxidants (hydrogen peroxide and ozone) after ion irradiation of frozen water, carbon dioxide and their mixtures. Irradiation of pure water ice produces hydrogen peroxide whatever is the used ion and at different temperatures. Irradiation of carbon dioxide and water frozen mixtures result in the production of molecules among which hydrogen peroxide and ozone. The experimental results are discussed in the light of the relevance they have to support the presence of an energy source for biosphere on Europa and other icy moons in the outer Solar System.

Funder

European COST Action

Publisher

Hindawi Limited

Subject

Space and Planetary Science,Astronomy and Astrophysics

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