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- W1510383710 abstract "On Cassini’s 121st orbit, the onboard ISS camera acquired high-resolution (15-30 m/pxl) images in Enceladus’south polar province. The imaging sequence was specifically designed to study one of the source regions ofEnceladus’ erupting plumes, Baghdad Sulcus. To facilitate the analysis, we derived a digital elevation modelin an active section (76°S/323°E) across Baghdad Sulcus. The model reveals that there is a V-shaped troughup to 500 m deep in the center of this section, with flanking slopes of 30° (SW-facing) and > 32° (NE-facing,this slope is in shadow). The slopes do approach angle of repose, but the morphology on the SW slope (blockyterrain with lineation patterns and even benches at angles to the maximum slope) suggests that this is not a slopeundergoing angle-of-repose control. The trough, therefore, may owe its shape primarily to faulting, with onlysome modification by deposition of icy particles by the plume-forming gas. Blocky covering, which includes blocksizes of up to 50 m, is not restricted to the trough but also occurs at about the same size and frequency distributionaway from it. This suggests that the blocks are not related to the venting process, which concentrates in the trough.Rather, the association of the blocky surfaces with multiple patterns of lineations (presumably fractures and faults)suggests they are outcrops of fault-related ice blocks or lithified detritus undergoing some form of erosion. Apotential erosion process may include seismic shaking.The V-shaped trough is partly accompanied by an elevated flanking ridge, which is indicative for rift zones andhints at an extensional origin of Baghdad Sulcus. Alternatively, fault-block rotation at large strains could have ledto the elevated ridge." @default.
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- W1510383710 date "2010-05-01" @default.
- W1510383710 modified "2023-09-22" @default.
- W1510383710 title "The morphology of an active zone near Enceladus' south pole and implications" @default.
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