V13E:
Planetary Differentiation Processes Constrained by Metal Stable Isotopes: From Theories to Observations I
Submit an Abstract to this Session
Session ID#: 35727
Session Description:
In the last two decades, analytical methods of metal stable isotopes, ranging from Li to U, have been significantly improved, and metal stable isotopes are extensively used in many fields of geochemistry. Metal stable isotopes can be fractionated by both equilibrium and kinetic processes as controlled by many factors during planetary differentiation. They are powerful tools to study processes that make the Earth, other planets, and the Moon into their current forms. This session invites contributions from (but not limited to) studies on the mechanism of isotope fractionation using experimental and theoretical approaches, observations and applications of metal stable isotopes on terrestrial and extraterrestrial samples, and novel analytical method development.
Primary Convener: Fang Huang, USTC University of Science and Technology of China, Hefei, China
Conveners: Frédéric Moynier, Université Paris Cité, Institut de Physique du Globe de Paris, Paris, France, James M Watkins, University of Oregon, Department of Earth Sciences, Eugene, United States and Shichun Huang, University of Nevada Las Vegas, Las Vegas, NV, United States
Chairs: Shichun Huang, University of Nevada Las Vegas, Las Vegas, NV, United States, Fang Huang, USTC University of Science and Technology of China, Hefei, China, Frédéric Moynier, Université Paris Cité, Institut de Physique du Globe de Paris, Paris, France and James M Watkins, University of Oregon, Department of Earth Sciences, Eugene, United States
OSPA Liaison: Fang Huang, USTC University of Science and Technology of China, Hefei, China
Abstracts Submitted to this Session:
Sune Nielsen, Woods Hole Oceanographic Institution, Department of Geology and Geophysics, Woods Hole, United States, Maureen E E Auro, Woods Hole Oceanographic Institution, Marine Chemistry & Geochemistry, Woods Hole, United States, Tomas Magna, Czech Geological Survey, Prague, Czech Republic, David Michael Davis, Georgia State University, Atlanta, GA, United States, Klaus Mezger, University of Bern, Institut für Geologie, Bern, Switzerland and Adam Robert Sarafian, Corning R&D Corp., Corning, NY, United States
Mary M Reagan, Stanford Earth Sciences, Geological Sciences, Stanford, CA, United States, Anat Shahar, Carnegie Institution for Science, Washington, DC, United States, Stephen M Elardo, Carnegie Institution for Science Washington, Washington, DC, United States, Jin Liu, Yanshan University, Qinhuangdao, China, Yuming Xiao, Geophysical Laboratory, Washington Dc, DC, United States and Wendy L Mao, Stanford University, Earth and Planetary Sciences, Stanford, United States
Nicolas Dauphas1, Mathieu Roskosz2, Michael Y. Hu3, Daniel R Neuville4, Ercan E. Alp5, Justin Hu6, Andrew Heard6 and Jiyong Zhao7, (1)University of Chicago, Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, Chicago, IL, United States, (2)MNHN National Museum of Natural History Paris, Paris, France, (3)Advanced Photon Source, Argonne National Laboratory, Argonne, IL, United States, (4)CNRS, Paris Cedex 16, France, (5)Argonne National Laboratory, Advanced Photon Source, Argonne, United States, (6)University of Chicago, Department of the Geophysical Sciences, Chicago, IL, United States, (7)Advanced Photon Source, Lemont, United States
Corliss Kin I Sio1,2, Mathieu Roskosz3, Nicolas Dauphas4, Neil Bennett5, Timothy D Mock5 and Anat Shahar6, (1)Lawrence Livermore National Laboratory, Livermore, CA, United States, (2)Carnegie Institution of Washingon, Washington, DC, United States, (3)MNHN National Museum of Natural History Paris, Paris, France, (4)University of Chicago, Origins Laboratory, Department of the Geophysical Sciences and Enrico Fermi Institute, Chicago, IL, United States, (5)Carnegie Institution of Washington, Washington, DC, United States, (6)Carnegie Institution of Washington, Washington DC, United States
Emily A Pringle, Scripps Institution of Oceanography, La Jolla, CA, United States; Institut de Physique du Globe de Paris, Paris, France and Frédéric Moynier, Université Paris Cité, Institut de Physique du Globe de Paris, Paris, France
Huimin Yu, University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China, Xiaoyun Nan, Araraquara, SP, Brazil, Jian Huang, BNU Beijing Normal University, Norfolk, VA, United States, Gerhard Wörner, University of Göttingen, Geochemistry and Isotope Geology, Göttingen, Germany and Fang Huang, USTC University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China
Christopher A Parendo1, Stein B Jacobsen1, Katsuyuki Yamashita2 and Osamu Okano2, (1)Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States, (2)Okayama University, Okayama, Japan
Fang Huang1, Wenzhong Wang2, Chen Zhou1, Jinting Kang2 and Zhongqing Wu2, (1)University of Science and Technology of China, Hefei, China, (2)University of Science and Technology of China, School of Earth and Space Sciences, Hefei, China
