Distribution of CO2 ice on the large moons of Uranus and evidence for compositional stratification of their near-surfaces

@article{Cartwright2015DistributionOC,
  title={Distribution of CO2 ice on the large moons of Uranus and evidence for compositional stratification of their near-surfaces},
  author={Richard J. Cartwright and Joshua P. Emery and Andrew S. Rivkin and David E. Trilling and Noem{\'i} Pinilla-Alonso},
  journal={Icarus},
  year={2015},
  volume={257},
  pages={428-456}
}
Abstract The surfaces of the large uranian satellites are characterized by a mixture of H2O ice and a dark, potentially carbon-rich, constituent, along with CO2 ice. At the mean heliocentric distance of the uranian system, native CO2 ice should be removed on timescales shorter than the age of the Solar System. Consequently, the detected CO2 ice might be actively produced. Analogous to irradiation of icy moons in the Jupiter and Saturn systems, we hypothesize that charged particles caught in… Expand
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