*Tomokazu Hokada1,2, Daniel J. Dunkley1, Kazuyuki Shiraishi1,2, Yoshikuni Hiroi3,1, Yoichi Motoyoshi1,2 (1.National Institute of Polar Research, 2.The Graduate University for Advanced Studies, SOKENDAI, 3.Chiba University)
Session information
[E] Poster
S (Solid Earth Sciences ) » S-MP Mineralogy & Petrology
[S-MP37] Supercontinents and crustal evolution
convener:Madhusoodhan Satish-Kumar(Department of Geology, Faculty of Science, Niigata University), Krishnan Sajeev(Centre for Earth Sciences, Indian Institute of Science), Tomokazu Hokada(National Institute of Polar Research), Yasuhito Osanai(Division of Evolution of Earth Environments, Faculty of Social and Cultural Studies, Kyushu University)
Supercontinent formation and dispersion has been enigmatic in the Earth's history. Eurasia is one such current supercontinent and incredible progress in the understanding of its geological evolution has been achieved in the past decades. Earlier supercontinents in
the Earth's history such as Gondwana (0.5 Ga), Rodinia (1.0 Ga), Columbia/Nuna (2.0 Ga), Kenorland (2.5 Ga) and Vaalbara (3.1 Ga), have been the focus of several studies, however limited information on older supercontinents has restricted in understanding their tectonic evolution. Several important unsolved issues remain, such as how, when and where these supercontinents formed and how long they remained as such before breaking apart. Additional questions arise on the processes that triggered the fragmentation and unification of continents. In this session, we invite authors around the world to present original new
data as well as review results on the continental scale crustal processes and tectonic evolution that are associated with supercontinent formation events in Earth's history. The well-studied Eurasia and Gondwana supercontinents are of particular focus. Topics of interest include, but not restricted to, extremes in metamorphism, P-T-d-t evolution, magmatism, and the role of fluids. We hope to provide a platform for scientific discussions that will enlighten our understanding of the physical and chemical processes in the continental crust that records episodes of orogenesis that contributed to the formation and evolution of supercontinents.
Taeko Uehara1, *Toshiaki Tsunogae1,2, Thembiso Otladisang Basupi1, Yukiyasu Tsutsumi3 (1.The University of Tsukuba, 2.University of Johannesburg, 3.National Museum of Nature and Science)
*Silpa Ammini Sasidharan1, Madhusoodhan Satish-Kumar1 (1.Department of Geology, Faculty of Science, Niigata University)
*Prakash Chandra Arya1, Krishnan Sajeev1 (1.Indian Institute of Science)
*M A Sanjeewa P K Malaviarachchi1, Madhusoodhan Satish-Kumar2, Toshiro Takahashi2 (1.Department of Geology, Faculty of Science, University of Peradeniya, Sri Lanka, 2.Department of Geology, Faculty of Science, Niigata University, Japan)
*Ryuichi Shinjo1, Tomoki Amuro1, Kohei Oura1, Kazuya Oshiro1, Shiro Tahara1, Harutaka Sakai2 (1.Department of Physics and Earth Sciences, University of the Ryukyus, 2.Department of Geology and Mineralogy, Kyoto University)
*Qian Liu1,2, Toshiaki Tsunogae2,3, Guochun Zhao4,5 (1.JSPS, 2.Tsukuba Univ. , 3.Johannesburg Univ. , 4.HKU, 5.Northwest Univ.)
[SMP37-P08] Native iron and serpentinization of peridotite, Oshika Village, Nagano Prefecture, Japan
*Yuya Takeda1, Seiichiro Uehara2 (1.Department of Earth and Planetary Science, Graduate School of Science, Kyushu University, 2.Department of Earth and Planetary Science, Faculty of Science, Kyushu University)