MR23B:
Liquids in Planetary Interiors: Experiments, Calculations, and Modeling II

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Session ID#: 15965

Session Description:
The study of liquids of geophysical interest is important to understanding the present state of the Earth and other planets, as well as their evolution through time. Partial melting of silicates could occur all across the mantle, in the upper mantle as well as at the core-mantle boundary, and liquid iron alloys are largely present in planetary cores. This session will be dedicated to the study of melting phenomena, partial melts and fluids. Topics will include, but are not limited to, melting curves, structural, thermo-physical and chemical properties of liquid silicates and iron alloys under high pressure, and their implications for planetary interiors. We would like to open this session to experimental work (either static or dynamic compression) and theoretical calculations on liquids and melts, as well as to seismological observations and geophysical modeling highlighting the fundamental role played by bulk liquid or partial melting in planetary interiors.
Primary Convener:  Guillaume Morard, IMPMC Institut de Minéralogie et de Physique des Milieux Condensés, Paris Cedex 05, France
Conveners:  Tony Yu, The University of Chicago, Center for Advanced Radiation Sources, Chicago, United States, Yoichi Nakajima, Kumamoto University, Kumamoto, Japan and Daniele Antonangeli, Sorbonne Université - MNHN - CNRS - IMPMC, Paris, France
Chairs:  Guillaume Morard, IMPMC Institut de Minéralogie et de Physique des Milieux Condensés, Paris Cedex 05, France and Yoichi Nakajima, Kumamoto University, Kumamoto, Japan
OSPA Liaison:  Daniele Antonangeli, Sorbonne Université - MNHN - CNRS - IMPMC, Paris, France

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

3924 High-pressure behavior [MINERAL PHYSICS]
3939 Physical thermodynamics [MINERAL PHYSICS]

Abstracts Submitted to this Session:

Jonathan F Stebbins, Stanford University, Geological Sciences, Stanford, CA, United States
Donato Belmonte1, Giulio Armando Ottonello1, Marino Vetuschi Zuccolini1 and Marco Attene2, (1)University of Genoa, Genoa, Italy, (2)CNR National Research Council, IMATI, Rome, Italy
James William Harold Braithwaite1, Lars P Stixrude2, Eero Holmstrom1 and Carlos Pinilla3, (1)University College London, London, United Kingdom, (2)University College London, Earth Sciences, London, United Kingdom, (3)Universidad del Norte, Physics and Geosciences, Puerto Colombia, Colombia
Bin Chen, University of Hawaii at Manoa, Honolulu, United States, Xiaojing Lai, China University of Geosciences, Wuhan, China, Jianwei Wang, Louisiana State University, Baton Rouge, LA, United States, Feng Zhu, University of Michigan Ann Arbor, Department of Earth and Environmental Sciences, Ann Arbor, MI, United States, Jiachao Liu, Michigan State University, Earth and Environmental Sciences, East Lansing, United States and Yoshio Kono, Carnegie Institution for Science Washington, Washington, DC, United States
Anne Pommier, University of California San Diego, La Jolla, CA, United States, Vera Laurenz, Bayerisches Geoinstitut, University of Bayreuth, Bayreuth, Germany, Prof. Christopher J Davies, Scripps Institution of Oceanography, La Jolla, CA, United States and Daniel J Frost, University of Bayreuth, Bayerisches Geoinstitut, Bayreuth, Germany
Amy Edgington1, Lidunka Vocadlo1, Oliver T Lord2, Ian G Wood3 and Lars P Stixrude3, (1)University College London, London, United Kingdom, (2)University of Bristol, School of Earth Sciences, Bristol, BS8, United Kingdom, (3)University College London, Earth Sciences, London, United Kingdom
Julien Chantel1, Zhicheng Jing2, Man Xu1, Tony Yu3 and Yanbin Wang4, (1)Case Western Reserve University, Cleveland, OH, United States, (2)Case Western Reserve University, Cleveland, United States, (3)The University of Chicago, Center for Advanced Radiation Sources, Chicago, United States, (4)University of Chicago, Chicago, IL, United States