The distribution of CO2 over part of the surface of Iapetus revealed from statistical clustering of a VIMS mosaic.

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Scientific paper

We present a detailed study of an Iapetus mosaic of Cassini-VIMS data with high spatial resolution (0.5 x 0.5 ) [5]. We analyze this set of data using a statistical clustering approach to reduce the analysis of a large number of data ( 104 spectra from 0.35 to 5.10 μm) to the study of seven representative groups accounting for 99.6 % of the surface covered by the original sample. We give special attention to the study of the CO2 band. We find that CO2 absorption is widespread over both the bright and dark regions of Iapetus' surface, and probably represents the trapping of carbon dioxide as a clathrate, hydrate, or adsorbate at the molecular level with other materials. The strength of the CO2 band in the areas where both, H2O- and carbon- bearing materials exist, gives support to the hypothesis that this volatile is formed on the surface of Iapetus as a product of irradiation of these two components.

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