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- W89711638 abstract "Gulick, A. Davatzes, K. Kolb and the HiRISE team. 1 NASA Ames/SETI Institute, MS 239-20, NASA Ames Research Center, Moffett Field, CA 94035, (email: vgulick@mail.arc.nasa.gov), 2 LPL, University of Arizona, Tucson, AZ. Introduction: The surface of Mars has been extensively modified at all scales by fluvial processes. The High Resolution Imaging Science Experiment (HiRISE) camera onboard the Mars Reconnaissance Orbiter is extending our understanding of these features to scales more familiar to a terrestrial geologists. Here we briefly summarize some of the fluvial observations of gullies in HiRISE images obtained so far. Gullies: Some of the most spectacular HiRISE images have been of gullies formed on the interior slopes of impact craters and elsewhere. Additional observations of gully morphology in various locations on Mars has provided insight to formation mechanisms involved. Notable features seen in the images include theater heads in some cases, multiple elevations for source regions (Figure 1), source regions originating" @default.
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- W89711638 date "2007-07-01" @default.
- W89711638 modified "2023-09-25" @default.
- W89711638 title "Some Insights on Gully Morphology and Formation on Mars from HiRISE" @default.
- W89711638 hasPublicationYear "2007" @default.
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