EP036
Shaping Landscapes of the Solar System: Environmental Flows on Other Planets
Shaping Landscapes of the Solar System: Environmental Flows on Other Planets
Session ID#: 81798
Session Description:
Quantitative models for surface processes have been derived for Earth systems. When applied to other planetary bodies, these Earth-based models can provide critical insights into the geologic history of the Solar System. In return, planetary surfaces across the Solar System offer a unique opportunity to test these models under conditions often unachievable on Earth. We invite a range of contributions in the field of planetary surface processes with an emphasis on fluid and granular flows (fluvial, eolian, glacial, mass wasting, coastal, etc.) and that use laboratory experiments, theoretical and numerical modeling, and planetary-exploration data from orbiters, landers, and rovers. This session’s goal is to explore the interplay between quantitative models for planetary surface processes and new planetary exploration data that often challenge these models. We intend this session to foster more collaboration between members of the PS and EPSP sections.
Co-Organized:
- P - Planetary Sciences
Index Terms:
1825 Geomorphology: fluvial [HYDROLOGY]
1826 Geomorphology: hillslope [HYDROLOGY]
5415 Erosion and weathering [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5419 Hydrology and fluvial processes [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
Primary Convener: Marisa C Palucis, Dartmouth College, Department of Earth Sciences, Hanover, NH, United States
Conveners: Alexander M Morgan, Smithsonian Institution, Center for Earth and Planetary Studies, National Air and Space Museum, Washington, DC, United States and Mathieu Gaetan Andre Lapotre, Stanford University, Geological Sciences, Stanford, CA, United States
Primary Liaison: Marisa C Palucis, Dartmouth College, Department of Earth Sciences, Hanover, NH, United States
See more of: Earth and Planetary Surface Processes
