MR011:
Liquids and Melting in Earth and Planetary Interiors





Session ID#: 24777

Session Description:
The study of liquids is critical to understanding the interiors of Earth and other planets. In the Earth, partial silicate melting can occur from the top of the mantle to the core-mantle boundary, and Earth and many other planets have partially molten iron-rich cores. Additionally, core formation may have occurred in a magma ocean. This session focuses on the melting process, liquids, and their effects and properties in deep planetary interiors. Topics may include, but are not limited to: partial melting processes, magma oceans, melting curves, structural and chemical properties of liquids and glasses, and the implications of melt on planetary processes. We encourage contributions from experimental and theoretical studies of liquids and melting, as well as those from seismological observations and geodynamical consequences of melt in the deep Earth and other planets.
Primary Convener:  Rebecca A. Fischer, University of Chicago, Chicago, IL, United States
Conveners:  Thomas S Duffy, Princeton University, Department of Geosciences, Princeton, NJ, United States and Bethany Chidester, University of Chicago, Chicago, IL, United States

Cross-Listed:
  • DI - Study of the Earth's Deep Interior
Index Terms:

1015 Composition of the core [GEOCHEMISTRY]
3924 High-pressure behavior [MINERAL PHYSICS]
3939 Physical thermodynamics [MINERAL PHYSICS]
5460 Physical properties of materials [PLANETARY SCIENCES: SOLID SURFACE PLANETS]

Abstracts Submitted to this Session:

Donald B Dingwell, Ludwig Maximilians University of Munich, Munich, Germany, Kai-Uwe Hess, Ludwig Maximilian University of Munich, Munich, Germany, Martin C Wilding, Aberystwyth University, Aberystwyth, United Kingdom and Richard A. Brooker, University of Bristol, School of Earth Sciences, Bristol, United Kingdom
Guoyin Shen, Chuanlong Lin, Stanislav V Sinogeikin and Jesse Smith, HPCAT, Carnegie Institution of Washington, Argonne, IL, United States
Guillaume Morard1, Silvia Boccato2, Angelika D. Rosa2, Simone Anzellini3, Francesca Miozzi Ferrini1, Henry Laura2, Gaston Garbarino2, Marion Harmand1, Francois J Guyot1, Eglantine Boulard1, Innokenty Kantor2, Tetsuo Irifune4 and Raffaella Torchio2, (1)IMPMC Institut de Minéralogie et de Physique des Milieux Condensés, Paris Cedex 05, France, (2)ESRF European Synchrotron Radiation Facility, Grenoble, France, (3)Diamond Light Source, Didcot, United Kingdom, (4)Geodynamics Research Center, Matsuyama, Japan
Saurav Bista, Stanford University, Stanford, CA, United States and Jonathan F Stebbins, Stanford University, Geological Sciences, Stanford, CA, United States
Marzena Anna Baron1,2, Oliver T Lord3, Robert Myhill3, Andrew Thomson4, Weiwei Wang4, Reidar G Tronnes2 and Michael J Walter5, (1)Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC) - UMR CNRS 7590, Paris Cedex 5, France, (2)University of Oslo, Centre for Earth Evolution and Dynamics, Oslo, Norway, (3)University of Bristol, School of Earth Sciences, Bristol, United Kingdom, (4)University College London, London, United Kingdom, (5)University of Bristol, School of Earth Sciences, Bristol, BS8, United Kingdom
Suraj K Bajgain and Mainak Mookherjee, Florida State University, Earth, Ocean and Atmospheric Sciences, Tallahassee, FL, United States
Paul D Asimow, California Institute of Technology, Pasadena, CA, United States, Oleg V Fat'yanov, California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States, Chang Su, Chinese Academy of Sciences, Institute of Geochemistry, Guiyang, China and Xiao-juan Ma, Southwest Jiaotong University, Key Laboratory of Advanced Technologies of Materials, Chengdu, China
Man Xu1, Zhicheng Jing1, Julien Chantel1, Tony Yu2, Yanbin Wang2 and Peixiu Jiang1, (1)Case Western Reserve University, Cleveland, OH, United States, (2)The University of Chicago, Argonne, IL, United States
Suyu Fu1, Jing Yang2, Vitali Prakapenka3, Youjun Zhang4, Eran Greenberg5 and Jung-Fu Lin1, (1)University of Texas at Austin, Austin, TX, United States, (2)The University of Texas at Austin, Geological Sciences, Austin, TX, United States, (3)The University of Chicago, Argonne, IL, United States, (4)Center for high pressure science and technology advanced researth, Shanghai, China, (5)University of Chicago, GeoSoilEnviroCARS, Chicago, IL, United States
Yoshio Kono1, Yuki Shibazaki2, Curtis Kenney-Benson3, Yanbin Wang4 and Guoyin Shen3, (1)Carnegie Institution for Science Washington, Washington, DC, United States, (2)Tohoku University, Sendai, Japan, (3)Carnegie Instituion of Washing, Argonne, IL, United States, (4)The University of Chicago, Argonne, IL, United States
Megan S Duncan, Geophysical Laboratory of the Carnegie Institution for Science, Washington, DC, United States, Nicholas C Schmerr, University of Maryland, College Park, MD, United States and Yingwei Fei, Carnegie Institution for Science Washington, Geophysical Laboratory, Washington, DC, United States
Rostislav Hrubiak, Carnegie Institution of Washington, High Pressure Collaborative Access Team (HPCAT), Argonne, IL, United States, Yue Meng, Carnegie Inst Washington, HPCAT, Washington, DC, United States and Guoyin Shen, Carnegie Instituion of Washing, Argonne, IL, United States
Zhicheng Jing1, Man Xu1, Peixiu Jiang1, Tony Yu2 and Yanbin Wang2, (1)Case Western Reserve University, Cleveland, OH, United States, (2)The University of Chicago, Argonne, IL, United States
Joshua P Townsend1, Seth Root1, Luke Shulenburger1, Raymond W Lemke1, Richard G Kraus2, Stein B Jacobsen3, Dylan Spaulding4, Erik Davies5 and Sarah T Stewart5, (1)Sandia National Laboratories, Albuquerque, NM, United States, (2)Lawrence Livermore National Lab, Reno, NV, United States, (3)Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States, (4)Harvard University, Cambridge, MA, United States, (5)University of California Davis, Davis, CA, United States
Xenia Ritter1, Carmen Sanchez-Valle1, Mickael Laumonier2, Andrew King3, Nicolas Guignot3, Fabrice Gaillard4,5, David Sifre6 and Jean-Philippe Perrillat7, (1)University of Münster, Institute for Mineralogy, Münster, Germany, (2)Laboratoire Magmas et Volcans, Clermond-Ferrand, France, (3)SOLEIL Synchrotron, Gif sur Yvette, France, (4)CNRS-Orléans, Orléans, France, (5)ISTO Institut des Sciences de la Terre d'Orléans, Orléans Cedex 2, France, (6)European Synchrotron Radiation Facility, Grenoble, France, (7)Laboratoire de Géologie de Lyon - Université Claude Bernard Lyon1, Villeurbanne, France
Olivier Bollengier, University of Washington Seattle Campus, Seattle, WA, United States, J Michael Brown, University of Washington, Earth and Space Sciences, Seattle, WA, United States and Steve Vance, Jet Propulsion Laboratory, Pasadena, CA, United States
Razvan Caracas, CNRS Lyon, Lyon, France and Sarah T Stewart, Harvard Univ, Cambridge, MA, United States