2006•The Astrophysical JournalOpen access

The Enceladus and OH Tori at Saturn

R. E. Johnson, Howard Todd Smith, Orenthal J. Tucker, M. Liu, M. Bürger, Edward C Sittler Jr, Robert L. Tokar

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Abstract

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.

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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.

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Available abstract

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.

Key concepts: Enceladus, Physics, Saturn, Torus, Astrobiology, Astronomy, Titan (rocket family), Atmosphere (unit)

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