Collisional Evolution of the Enceladus Neutral Cloud

Cassidy, T. A.; Johnson, R. E.; Hendrix, A. R.

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NASA NTRS · 20110020651

Collisional Evolution of the Enceladus Neutral Cloud

Cassidy, T. A.·Johnson, R. E.·Hendrix, A. R.

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Abstract

Water vapor ejected from Saturn's small moon Enceladus easily escapes its meager gravity to form a Saturn-encircling cloud with a low collision rate. Observations show that the cloud is quite broad in the radial direction, and we show here that collisions, though quite rare, may be largely responsible for this radial spreading. We modeled this cloud using the Direct Simulation Monte Carlo method, as fluid methods would be inappropriate for such a tenuous gas.

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Cassidy, T. A., Johnson, R. E., Hendrix, A. R.. 2011-07-11. Collisional Evolution of the Enceladus Neutral Cloud. https://ntrs.nasa.gov/citations/20110020651

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