MR011
The History of Volatiles in Rocky Planetary Interiors and Their Surface Expression

Session ID#: 157196

Session Description:
Highly volatile elements (e.g., H, C, N, S) are critical for the internal dynamics and surface environment of rocky planets and essential for life as we know it. During accretion and solidification, the delivery, partitioning, and loss of these volatile elements in rocky planetary interiors set the initial conditions for their subsequent evolution. After planet formation, their distribution, storage, and cycling between interior reservoirs (core and mantle) and near-surface/surface reservoirs (crust, ocean, atmosphere) regulate material circulation and thermal evolution of the interior as well as tectonics and climate of the surface. This session aims to bring together observational, experimental, and theoretical contributions about the history of highly volatile elements in rocky planetary interiors, with an emphasis on implications for the surface environment and habitability of the Earth and other rocky planets within and beyond the Solar System.
Co-Organized:
  • DI - Study of Earth's Deep Interior
Index Terms:

1099 General or miscellaneous [GEOCHEMISTRY]
3699 General or miscellaneous [MINERALOGY AND PETROLOGY]
3999 General or miscellaneous [MINERAL PHYSICS]
5499 General or miscellaneous [PLANETARY SCIENCES: SOLID SURFACE PLANETS]

Primary Convener:  Junjie Dong, Harvard University, Department of the History of Science, Cambridge, MA, United States; Harvard University, Department of Earth and Planetary Sciences, Cambridge, MA, United States
Conveners:  Cara Vennari, Lawrence Livermore National Laboratory, Livermore, United States, Susannah Dorfman, Michigan State University, Department of Earth and Environmental Sciences, East Lansing, MI, United States; Michigan State University, Department of Physics and Astronomy, East Lansing, MI, United States and Bin Chen, University of Hawaii at Manoa, Hawaii Institute of Geophysics and Planetology, Honolulu, United States
Student/Early Career Convener:  Jesse Tao Gu, Harvard University, Department of Earth and Planetary Sciences, Cambridge, MA, United States
 
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Shashank Prabha Mohan, Kenneth T Koga, Antoine Mathieu and Franck Pointud, Université Clermont Auvergne, CNRS, IRD, OPGC, Laboratoire Magmas et Volcans, Clermont-Ferrand, France
 
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Claire Guimond1, Oliver Shorttle1 and John F Rudge2, (1)University of Cambridge, Cambridge, United Kingdom, (2)University of Cambridge, Department of Earth Sciences, Cambridge, United Kingdom
 
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Yoshinori Miyazaki, California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States
 
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Tingting Gu1, Martha G Pamato2, Davide Novella2, Matteo Alvaro3, John Fournelle4, Frank E. Brenker5, Wang Wuyi6 and Fabrizio Nestola7, (1)Purdue University, Department of Earth, Atmospheric, and Planetary Sciences, West Lafayette, IN, United States, (2)University of Padova, Department of Geosciences, Padova, Italy, (3)University of Pavia, Department of Earth and Environmental Sciences, Pavia, Italy, (4)University of Wisconsin Madison, Dept. of Geoscience, Madison, United States, (5)Geothe University, Frankfurt, Germany, (6)Gemological Institute of America, New York, United States, (7)University of Padua, Department of Geosciences, Padua, Italy
 
Hot and Cold Hydrous Sulfates: Phase Transitions in Epsomite and Melanterite at Elevated Pressures and Extreme Temperatures (1079453)
Máté Garai1, Brian Gulick2, Christian Shushok2, Audrey Burch2, Zhenxian Liu3 and Elizabeth Colette Thompson2, (1)The University of the South, Dept. of Physics and Astronomy, Sewanee, United States, (2)The University of the South, Dept. of Earth and Environmental Systems, Sewanee, United States, (3)University of Illinois Chicago, Department of Physics, Chicago, United States
 
Earth’s Earliest Atmosphere and Volatile Loss During Accretion (1082180)
Jesse Tao Gu, Harvard University, Department of Earth and Planetary Sciences, Cambridge, MA, United States, Bo Peng, University of Toronto, Department of Astronomy and Astrophysics, Toronto, Canada, Jisheng Zhang, University of Chicago, Department of Astronomy and Astrophysics, Chicago, IL, United States, Xuan Ji, University of Chicago, Department of the Geophysical Sciences, Chicago, IL, United States, Hong Yang, Stanford University, Department of Geological Sciences, Stanford, CA, United States, Susana Hoyos, Massachusetts Institute of Technology, Earth, Atmospheric and Planetary Sciences, Cambridge, MA, United States, Marc M Hirschmann, University of Minnesota Twin Cities, Department of Earth and Environmental Sciences, Minneapolis, United States and Edwin S Kite, University of Chicago, Department of the Geophysical Sciences, Chicago, United States
 
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Anne Davis and Razvan Caracas, University of Oslo, The Center for Earth Evolution and Dynamics (CEED), Oslo, Norway
 
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William R Palfey, California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States, George R Rossman, California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, United States, Sonjong Hwang, California Institute of Technology, Chemical Engineering, Pasadena, United States and Wiliiam A. Goddard III, California Institute of Technology, Materials and Process Simulation Center (MSC), Pasadena, United States
 
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Olivia Pardo1, William R Palfey2, Vasilije V Dobrosavljevic2, Wolfgang Sturhahn1, Zhenxian Liu3, George R Rossman1, Thomas Toellner4 and Jennifer M Jackson1, (1)California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, United States, (2)California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States, (3)University of Illinois Chicago, Department of Physics, Chicago, United States, (4)Argonne National Laboratory, Advanced Photon Source, Lemont, United States
 
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Tomona Oishi, The University of Tokyo, Department of Earth Science and Astronomy, Tokyo, Japan, Tsuyoshi Komiya, University of Tokyo, Department of Earth Science and Astronomy, Tokyo, Japan, Hirochika Sumino, Geochemical Research Center, Graduate School of Science, University of Tokyo, Tokyo, Japan and Hiroyuki Kagi, Univ Tokyo, Tokyo, Japan
 
Partitioning of Nitrogen in Reduced Magmatic Systems: Implications for early differentiation of rocky bodies in the Inner Solar System (1112738)
Aindrila Pal, 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, TX, United States
 
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Xiyuan Bao1, Zebin Cao2, Kenneth Christopher Gourley3, Sara Gutierrez4, Yuanyuan Liang5, Dongyuan Zhou6, Bruce A Buffett7, Tushar Mittal8, Jie Li9, Raymond Pierrehumbert10, Laura Schaefer11, James Van Orman4 and Bradford J Foley12, (1)University of California Los Angeles, Earth, Planetary, and Space Sciences, Los Angeles, CA, United States, (2)University of Illinois at Urbana Champaign, Geology, Urbana, IL, United States, (3)University of Arizona, Department of Geosciences, Tucson, United States, (4)Case Western Reserve University, Cleveland, OH, United States, (5)Washington University in St Louis, Department of Earth and Planetary Sciences, St. Louis, MO, United States, (6)University of Michigan Ann Arbor, Earth and Environmental Sciences, Ann Arbor, United States, (7)University of California Berkeley, Earth and Planetary Science, Berkeley, CA, United States, (8)Penn State, Earth and Planetary Science, University Park, United States, (9)University of Michigan Ann Arbor, Department of Earth and Environmental Sciences, Ann Arbor, MI, United States, (10)University of Oxford, Atmospheric, Oceanic and Planetary Physics, Oxford, United Kingdom, (11)Stanford University, Geological Sciences, Stanford, CA, United States, (12)Pennsylvania State University, Department of Geosciences, University Park, United States
 
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Qingyang Hu, Center for High Pressure Science & Technology Advanced Research, Beijing, China, Shengcai Zhu, Sun Yat-sen University, Guangzhou, China, Junwei Li, Center for High Pressure Science and Technology Advanced Researh, Beijing, China and Yanhao Lin, Center for High Pressure Science & Technology Advanced Research, Shanghai, China
 
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Jie Deng, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States; Princeton University, Department of Geosciences, Princeton, United States, Haiyang Niu, NWPU Northwestern Polytechnical University, School of Materials Science and Engineering, Xi'an, China, Mingyi Chen, NWPU Northwestern Polytechnical University, Xi'an, China and Lars P Stixrude, University of California Los Angeles, Department of Earth, Planetary and Space Sciences, Los Angeles, United States
 
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Pranabendu Moitra, University of Arizona, Tucson, AZ, United States, Ananya Mallik, University of Arizona, Geosciences, Tucson, AZ, United States, Jessica Barnes, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States and Jeffrey C Andrews-Hanna, Colorado School of Mines, Golden, CO, United States
 
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Kara Brugman, Carnegie Institution for Science, Earth & Planets Laboratory, Washington, D.C., United States, Anat Shahar, Carnegie Institution for Science, Washington DC, United States, James Badro, Institut de Physique du Globe de Paris, Paris, France and George D Cody, Carnegie Institution for Science, Earth and Planets Laboratory, Washington, DC, United States
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