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Hydrothermal plume dynamics on Europa: Implications for chaos formation

Journal of Geophysical Research: Planets American Geophysical Union (AGU) 109:E3 (2004) 2003JE002073

Authors:

Jason C Goodman, Geoffrey C Collins, John Marshall, Raymond T Pierrehumbert

Abstract:

Hydrothermal plumes may be responsible for transmitting radiogenic or tidally generated heat from Europa's rocky interior through a liquid ocean to the base of its ice shell. This process has been implicated in the formation of chaos regions and lenticulae by melting or exciting convection in the ice layer. In contrast to earlier work, we argue that Europa's ocean should be treated as an unstratified fluid. We have adapted and expanded upon existing work describing buoyant plumes in a rotating, unstratified environment. We discuss the scaling laws governing the flow and geometry of plumes on Europa and perform a laboratory experiment to obtain scaling constants and to visualize plume behavior in a Europa‐like parameter regime. We predict that hydrothermal plumes on Europa are of a lateral scale (at least 25–50 km) comparable to large chaos regions; they are too broad to be responsible for the formation of individual lenticulae. Plume heat fluxes (0.1–10 W/m2) are too weak to allow complete melt‐through of the ice layer. Current speeds in the plume (3–8 mm/s) are much slower than indicated by previous studies. The observed movement of ice blocks in the Conamara Chaos region is unlikely to be driven by such weak flow.
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An intense stratospheric jet on Jupiter

Nature 427 (2004) 132-135

Authors:

SB Calcutt, Achtergerg, Flasar, Kunde
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Exploring the Saturn System in the Thermal Infrared: The Composite Infrared Spectrometer

Chapter in The Cassini-Huygens Mission, Springer Nature (2004) 169-297

Authors:

FM Flasar, VG Kunde, MM Abbas, RK Achterberg, P Ade, A Barucci, B Bézard, GL Bjoraker, JC Brasunas, S Calcutt, R Carlson, CJ Césarsky, BJ Conrath, A Coradini, R Courtin, A Coustenis, S Edberg, S Edgington, C Ferrari, T Fouchet, D Gautier, PJ Gierasch, K Grossman, P Irwin, DE Jennings, E Lellouch, AA Mamoutkine, A Marten, JP Meyer, CA Nixon, GS Orton, TC Owen, JC Pearl, R Prangé, F Raulin, PL Read, PN Romani, RE Samuelson, ME Segura, MR Showalter, AA Simon-Miller, MD Smith, JR Spencer, LJ Spilker, FW Taylor
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Retrievals of jovian tropospheric phosphine from Cassini/CIRS

ICARUS 172:1 (2004) 37-49

Authors:

PGJ Irwin, P Parrish, T Fouchet, SB Calcutt, FW Taylor, AA Simon-Miller, CA Nixon
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Glacial flow of floating marine ice in “Snowball Earth”

Journal of Geophysical Research: Oceans American Geophysical Union (AGU) 108:C10 (2003) 2002JC001471

Authors:

Jason C Goodman, Raymond T Pierrehumbert

Abstract:

Simulations of frigid Neoproterozoic climates have not considered the tendency of thick layers of floating marine ice to deform and spread laterally. We have constructed a simple model of the production and flow of marine ice on a planetary scale, and determined ice thickness and flow in two situations: when the ocean is globally ice‐covered (“hard snowball”) and when the tropical waters remain open (“soft snowball”). In both cases, ice flow strongly affects the distribution of marine ice. Flowing ice probably carries enough latent heat and freshwater to significantly affect the transition into a Snowball Earth climate. We speculate that flowing marine ice, rather than continental ice sheets, may be the erosive agent that created some Neoproterozoic glacial deposits.
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