Search Publications

Cryovolcanism on Titan: New results from Cassini RADAR and VIMS
DOI: 10.1002/jgre.20062 Bibcode: 2013JGRE..118..416L

Barnes, J. W.; Janssen, M. A.; Lunine, J. I. +13 more

The existence of cryovolcanic features on Titan has been the subject of some controversy. Here we use observations from the Cassini RADAR, including Synthetic Aperture Radar (SAR) imaging, radiometry, and topographic data as well as compositional data from the Visible and Infrared Mapping Spectrometer (VIMS) to reexamine several putative cryovolca…

2013 Journal of Geophysical Research (Planets)
Cassini 116
Convection-driven compaction as a possible origin of Enceladus's long wavelength topography
DOI: 10.1002/jgre.20079 Bibcode: 2013JGRE..118..908B

Besserer, J.; Nimmo, F.; Roberts, J. H. +1 more

The long wavelength surface topography of Enceladus shows depressions about 1 km in depth and ∼102 km wide. One possible cause of this topography is spatially variable amounts of compaction of an initially porous ice shell, driven by spatial variations in heat flux. Here, we show that the heat flux variations associated with convection …

2013 Journal of Geophysical Research (Planets)
Cassini 43
A 1-D model of physical chemistry in Saturn's inner magnetosphere
DOI: 10.1002/jgre.20106 Bibcode: 2013JGRE..118.1567F

Delamere, P. A.; Bagenal, F.; Fleshman, B. L. +1 more

Water vapor spewed out of Enceladus' geysers spreads across the Saturn system through dissociation, charge exchange, and neutral-neutral collisions. The combined effects of impact ionization by suprathermal electrons, charge-exchange between ions and neutrals, and radial transport of the plasma produce the observed distribution of ions and their t…

2013 Journal of Geophysical Research (Planets)
Cassini 19
Estimates of fluvial erosion on Titan from sinuosity of lake shorelines
DOI: 10.1002/jgre.20153 Bibcode: 2013JGRE..118.2198T

Perron, J. Taylor; Tewelde, Yodit; Ford, Peter +2 more

Titan has few impact craters, suggesting that its surface is geologically young. Titan's surface also has abundant landforms interpreted to be fluvial networks. Here we evaluate whether fluvial erosion has caused significant resurfacing by estimating the cumulative erosion around the margins of polar lakes. A scarcity of detailed topographic data …

2013 Journal of Geophysical Research (Planets)
Cassini 11
Correction to: "Geophysical implications of the long-wavelength topography of the Saturnian satellites"
DOI: 10.1002/jgre.20162 Bibcode: 2013JGRE..118.2594N

Nimmo, F.; Thomas, P. C.; Bills, B. G.

2013 Journal of Geophysical Research (Planets)
Cassini 0