*Fumiya Maeda1, Eiji Ohtani1, Seiji Kamada2,1, Tatsuya Sakamaki1, Naohisa Hirao3, Yasuo Ohishi3 (1.Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University, 2.Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, 3.Japan Synchrotron Radiation Research Institute)
Session information
[EE] Poster
S (Solid Earth Sciences) » S-IT Science of the Earth's Interior & Tectonophysics
[S-IT27] [EE] Carbon in Planetary Interiors
Tue. May 23, 2017 3:30 PM - 5:00 PM Poster Hall (International Exhibition Hall HALL7)
convener:Craig E Manning(University of California Los Angeles), Eiji Ohtani(Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University), Hiroyuki Kagi(Geochemical Research Center, Graduate School of Science, University of Tokyo), Konstantin Litasov(V.S. Sobolev Institute of Geology and Mineralogy SB RAS)
The deep carbon cycle in Earth and other planetary bodies including
meteorite parent bodies depends on the structure and stability of
carbon-bearing minerals, melts and fluids at high pressure and temperature.
Recent advances are providing new insights into novel structures and
properties of native carbon phases, carbonate minerals, ices, clathrates,
carbides, and phases containing trace carbon. Carbon solubility in liquids
is important for understanding metal and silicate portions of planetary
interiors, and fluids containing carbon play important roles in elemental
mass transfer. This session highlights the roles of carbon in crystals,
melts and fluids in the deep carbon cycle in the terrestrial planets. We
welcome contributions based on any combination of computational,
experimental, and theoretical mineral physics and petrology, including work
on individual carbon-bearing phases and on their stability and reactivity
with multiphase assemblages.
Artem Chanyshev1, *Konstantin Litasov1, Anton Shatskiy1, Yoshihiro Furukawa2, Anna Likhacheva1, Takashi Yoshino3, Yuji Higo4, Eiji Ohtani2 (1.V.S. Sobolev Institute of Geology and Mineralogy SB RAS, Novosibirsk, Russia, 2.Graduate School of Science, Tohoku University, Sendai, Japan, 3.Institute for Study of the Earth’s Interior, Okayama University, Misasa, Tottori, Japan, 4.SPring-8, Japan Synchrotron Radiation Research Institute, Kouto, Hyogo, Japan)
*Hiroyuki Kagi1, Koji Maruyama1, Kazuki Komatsu1, Toru Yoshino3, Satoshi Nakano2 (1.Geochemical Research Center, Graduate School of Science, University of Tokyo, 2.NIMS, 3.TIRI)
Shatskiy Anton1,2, Ivan Podborodnikov1,2, *Konstantin Litasov1,2, Artem Chanishev1,2, Anton Arefiev1,2, Igor Sharygin1, Nikolay Karmanov1, Eiji Ohtani1,3 (1.V.S. Sobolev Institute of Geology and Mineralogy, Russian Academy of Science, Siberian Branch, , 2.Novosibirsk State University, 3.Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University)
Suguru Takahashi1, *Eiji Ohtani1, Seiji Kamada2, Tatsuya Sakamaki1, Naohisa Hirao3 (1.Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University, 2.Frontier Research Institute of Interdisciplinary Sciences, Tohoku University, 3.Japan Synchrotoron Research Institute)
Anton Shatskiy1, Ivan Podborodnikov1, *Konstantin Litasov1, Artem Chanyshev1, Anton Arefiev1, Igor Sharygin1, Nikolay Karmanov1, Eiji Ohtani2 (1.V.S. Sobolev Institute of Geology and Mineralogy, Russian Academy of Science, 2.Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University)