V31C:
Sulfur (Bio)geodynamic Cycles on Earth and Terrestrial Planets II Posters

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Session ID#: 13340

Session Description:
Sulfur is exchanged between the Earth’s surface and the mantle via subduction zones, magmatism, volcanic degassing, hydrothermalism, biological sulfate reductions and continental weathering. It also plays important roles in geological processes on other terrestrial planets. Yet, its transport and storage from the oceans and continents into the deep Earth, and secular changes in the mode of S-exchange between different igneous and surficial reservoirs remain discussed. Sulfur behavior is also related to its multiple valence states, implying complex interplays with redox state, and affecting sulfur partitioning between minerals, melts and fluids. This session seeks contributions from geochemistry, petrology, laboratory experiments, and field geology addressing the fate of sulfur in various geodynamic settings on terrestrial planets. We will also address the role of sulfur in the redox evolution and biochemical cycles, volcanic degassing, the distribution of chalcophile elements and ore-deposit formation, and coupling with other key volatiles such as carbon and halogens.


Primary Convener:  Julia Ribeiro, Guangzhou Institute of geochemistry, Guangzhou, China
Conveners:  Shuo Ding, Rice University, Earth, Environmental and Planetary Sciences, Houston, TX, United States, Fabrice Gaillard, CNRS-Orléans, Orléans, France and Paul J Wallace, University of Oregon, Department of Earth Sciences, Eugene, United States
Chairs:  Julia Ribeiro, Guangzhou Institute of geochemistry, Guangzhou, China and Shuo Ding, Rice University, Earth, Environmental and Planetary Sciences, Houston, TX, United States
OSPA Liaison:  Julia Ribeiro, Guangzhou Institute of geochemistry, Guangzhou, China
Co-Organized with:
Volcanology, Geochemistry and Petrology, Planetary Sciences, and Study of Earth's Deep Interior
Index Terms:

Abstracts Submitted to this Session:

Albert S Yen1, Douglas W Ming2, Ralf Gellert3, David W Mittlefehldt2, David T Vaniman4, Lucy M Thompson5, Richard V Morris2, Benton C Clark6 and Raymond E Arvidson7, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)NASA Johnson Space Center, Houston, TX, United States, (3)University of Guelph, Guelph, ON, Canada, (4)Planetary Science Institute Tucson, Tucson, AZ, United States, (5)University of New Brunswick, Fredericton, NB, Canada, (6)Space Science Institute, Boulder, CO, United States, (7)Washington University in St Louis, St. Louis, MO, United States
Shuo Ding, Rice University, Earth, Environmental and Planetary Sciences, Houston, TX, United States, Taylor Hough, Rice University, Department of Earth, Environmental, and Planetary Sciences, Houston, TX, United States and Rajdeep Dasgupta, Rice University, Department of Earth, Environmental and Planetary Sciences, Houston, United States
Xiaofei Pu, University of Michigan Ann Arbor, Ann Arbor, United States, Rebecca Ann Lange, University of Michigan, Department of Earth and Environmental Sciences, Ann Arbor, United States and Gordon M Moore, University of Michigan Ann Arbor, Ann Arbor, MI, United States
Giada Iacono-Marziano1, Fabrice Gaillard2, Thomas Lefebvre3 and Clement Ferraina3, (1)ISTO, UMR 7327 Université d'Orléans-CNRS-BRGM, Orléans, France, (2)CNRS, Paris Cedex 16, France, (3)ISTO Institut des Sciences de la Terre d'Orléans, Orléans Cedex 2, France
Trevor R Ireland1, Janaina Avila2, Callum Macfarlane3, Peter Holden3 and Pascal Philippot4, (1)Australian National University, Research School of Earth Sciences, Canberra, ACT, Australia, (2)Australian National University, Earth Science, Canberra, Australia, (3)Australian National University, Research School of Earth Sciences, Canberra, Australia, (4)Institut de Physique du Globe de Paris, Sorbonne-Paris Cité, Université Paris Diderot, CNRS, Paris, France