P41A:
Fluvial Landforms and Sedimentary Deposits on Planetary Surfaces

Submit an Abstract to this Session

Session Title - en français: Morphologies fluviales et dépôts sédimentaires sur les surfaces planétaires

Session ID#: 6807

Session Description:
This session solicites studies focusing on the geometry, setting and evolution of fluvial, lacustrine landforms and their corresponding sedimentary deposits on planetary surfaces.
We especially welcome analyses from orbital or in situ data from Mars and Titan, as well as terrestrial field studies of planetary analogues.
Studies coupling chemistry and/or mineralogy with morphology are solicited as well, including most recent results from the Opportunity and Curiosity rover missions.

Session Description - en français: Cette session sollicite des études sur la géometrie, la mise en place et l'évolution de morphologies fluviales et lacustres, et leurs dépôts sédimentaires, sur les surfaces planétaires. Nous encourageons particulièrement les études basées sur des analyses orbitales ou in situ de Mars et Titan, et les études de terrain sur des analogues planétaires. Nous sollicitions également les études couplant minéralogie et/ou chimie avec la morphologie, incluant les résultats récents de rovers Opportunity et Curiosity.

OSPA Liaison:  Nicolas Mangold, LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France
Chairs:  Alan D Howard, University of Virginia Main Campus, Charlottesville, VA, United States and Nicolas Mangold, LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France
Primary Convener:  Nicolas Mangold, LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France
Convener:  Alan D Howard, University of Virginia Main Campus, Charlottesville, VA, United States
Index Terms:

5419 Hydrology and fluvial processes [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
6207 Comparative planetology [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6225 Mars [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6281 Titan [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
Co-Sponsor(s):
  • ES - Earth Surface Processes
  • SG - Sedimentary Geology and Paleobiology

Abstracts Submitted to this Session:

Fluvial to Lacustrine Facies Transitions in Gale Crater, Mars (34294)
Dawn Y Sumner, University of California, Davis, Earth and Planetary Sciences, Davis, United States, Rebecca M. E. Williams, Planetary Science Institute, Tucson, United States, Juergen Schieber, Indiana University Bloomington, Bloomington, IN, United States, Marisa C Palucis, Dartmouth College, Department of Earth Sciences, Hanover, NH, United States, Dorothy Z Oehler, Johnson Space Center, Houston, TX, United States, Nicolas Mangold, LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France, Linda C Kah, University of Tennessee, Department of Earth and Planetary Sciences, Knoxville, TN, United States, Sanjeev Gupta, Imperial College London, London, SW7, United Kingdom, John P Grotzinger, California Institute of Technology, Pasadena, CA, United States, John A Grant III, Smithsonian National Air and Space Museum, Center for Earth and Planetary Studies, Washington, DC, United States, Lauren A Edgar, USGS, Astrogeology, Flagstaff, United States and William E Dietrich, University of California Berkeley, Department of Earth and Planetary Science, Berkeley, United States
Chemistry of sedimentary rocks at Gale crater, Mars: Alpha Particle X-ray Spectrometer (APXS) constraints. (Invited) (34422)
Lucy M Thompson1, Ralf Gellert2, Mariek E Schmidt3, Jeff A. Berger4, Nick Boyd2, Beverley E. Elliott5, Betina Pavri6, Glynis M Perrett2, John G Spray5, Scott Van Bommel2 and Albert Yen6, (1)University of New Brunswick, Fredericton, NB, Canada, (2)University of Guelph, Guelph, ON, Canada, (3)Brock University, St Catharines, ON, Canada, (4)University of Western Ontario, London, ON, Canada, (5)University of New Brunswick, Planetary and Space Science Centre, Fredericton, NB, Canada, (6)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
Phyllosilicates in fluvial-lacustrine sediments in Gale Crater as revealed by the Curiosity rover. (35930)
Richard J Leveille, McGill University, Department of Earth and Planetary Sciences, Montreal, QC, Canada
The chemistry of sediments at the Lower Aeolis Mons (Mt Sharp) from ChemCam/Curiosity observations (34220)
Nicolas Mangold1, Olivier Forni2, Diana L Blaney3, Ralph Milliken4, Marion Nachon5, Olivier Gasnault6, Martin FISK7, John P Grotzinger8, Joel Hurowitz9, Linda C Kah10, Laetitia Le Deit5, Stephane Le Mouelic11, Scott M McLennan12, Sylvestre Maurice13, Kathryn Stack3,8, Dawn Y Sumner14, Lucy M Thompson15, Roger C Wiens16 and MSL science team, (1)LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France, (2)Institut de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, France, (3)Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Brown University, Providence, United States, (5)University of Nantes, Nantes, France, (6)IRAP, CNRS, Université de Toulouse, UPS-OMP, Toulouse Cedex 4, France, (7)Oregon State Univ, Corvallis, OR, United States, (8)California Institute of Technology, Pasadena, CA, United States, (9)Stony Brook University, Geosciences, Stony Brook, NY, United States, (10)University of Tennessee, Department of Earth and Planetary Sciences, Knoxville, TN, United States, (11)CNRS, Paris Cedex 16, France, (12)Stony Brook University, Stony Brook, NY, United States, (13)IRAP, CNRS, Université de Toulouse, UPS-OMP, Toulouse, France, (14)University of California, Davis, Earth and Planetary Sciences, Davis, United States, (15)University of New Brunswick, Fredericton, NB, Canada, (16)Space Science and Applications, Los Alamos, United States
Fresh Shallow Valleys in Northern Arabia Terra, Mars: Implications for the Post-Noachian Climate (34304)
Sharon A. Wilson1,2, Alan D Howard1, Jeffrey M Moore3 and John A Grant III2, (1)University of Virginia Main Campus, Charlottesville, VA, United States, (2)Smithsonian National Air and Space Museum, Center for Earth and Planetary Studies, Washington, DC, United States, (3)NASA Ames Research Center, Moffett Field, CA, United States
Ancient Martian Lakestands and Fluvial Processes in Iani Chaos: Geology of Light-Toned Layered Deposits and their Relationship to Ares Vallis Outflow Channels (33394)
Luca Guallini, University of Bern, Physics Institute Space Research and Planetary Sciences, Bern, Switzerland, Martha S Gilmore, Wesleyan University, Earth and Environmental Sciences, Middletown, CT, United States, Lucia Marinangeli, University D'Annunzio, DiSPUTER, TeleLab, Chieti Scalo, Italy and Nicolas Thomas, University of Bern, Bern, Switzerland
Formation of Fluvial Gravel Pavements as an Explanation for Persistence of Ancient Cratered Terrain on Titan (34005)
Alan D Howard, University of Virginia Main Campus, Charlottesville, VA, United States, Sylvain Breton, University of Lyon, Lyon, France and Jeffrey M Moore, NASA Ames Research Center, Moffett Field, CA, United States
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