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The Enceladus and OH Tori at Saturn

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R. E. Johnson1, H. T. Smith1, O. J. Tucker1, M. Liu1, M. H. Burger2, E. C. Sittler2 and R. L. Tokar3

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The remarkable observation that Enceladus, a small icy satellite of Saturn, is actively venting has led to the suggestion that ejected water molecules are the source of the toroidal atmosphere observed at Saturn for over a decade using the Hubble Space Telescope (HST). Here we show that the venting leads directly to a new feature, a narrow Enceladus neutral torus. The larger torus, observed using HST, is populated by charge exchange, the process that limits the lifetime of the neutrals in the Enceladus torus.


Subject headings

planets and satellites: individual (Enceladus, Saturn)


Dates

Issue 2 (2006 June 20)

Received 2006 April 10, accepted for publication 2006 May 12

Published 2006 June 14



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