JpGU-AGU Joint Meeting 2026

Session information

[E] Poster

S (Solid Earth Sciences ) » S-GL Geology

[S-GL24] Crustal evolution in collision zones and its impacts on Earth's habitability

Fri. May 29, 2026 5:15 PM - 7:00 PM Poster Hall (Exhibition Hall 7&8, Makuhari Messe)

When two continents converge, the intervening oceanic basin is progressively consumed, ultimately leading to continental collision. Collision zones witness a succession of deep processes that impact Earth's solid and surficial reservoirs. Deep processes within the crust and mantle of the collision zone shape Earth's habitability through three linked mechanisms: (1) They induce mantle- and crust-derived magmas to drive the growth, reworking, and compositional maturation of the continental crust, constructing a stable physical platform that controls climate, ocean circulation and supports the evolution of life. (2) They facilitate the decomposition of copper-rich sulfide and lithium-rich biotite, releasing metallogenic elements that are then transported and enriched by fluids to form ore deposits, providing indispensable mineral resources for the development of civilizations. (3) They cause the dehydration and decomposition of hornblende and biotite, releasing volatiles (CHNOPS) that act as a climate-regulating valve, maintaining a habitable environment across the Earth's surface through the water-carbon-sulfur cycles. To understand the impact of crustal evolution in collision zones on Earth's habitability, address fundamental questions concerning linked processes within the Earth system, including future research directions, and promote interdisciplinary integration, this session welcomes submissions on, but not limited to, the following aspects: mantle evolution and continental crust formation in collision zones, volatile cycling and metallogenic effects in collision zones, deep C-S-H2O cycling and environmental impacts in collision zones, metamorphic anatexis and climate responses in collision zones, and the dynamics of crustal evolution in collision zones.

5:15 PM - 7:00 PM

*Kwan-Nang Pang1, Yang Sun2, Fang-Zhen Teng3, Shihong Tian4, Sun-Lin Chung1,5, Mohammad Hossein Zarrinkoub6 (1. Institute of Earth Sciences, Academia Sinica, 2. School of Geosciences, Yangtze University, Wuhan 430100, Chin, 3. Isotope Laboratory, Department of Earth and Space Sciences, University of Washington, Seattle, WA 98195, 4. School of Earth Sciences, East China University of Technology, Nanchang 330013, China, 5. Department of Geosciences, National Taiwan University, Taipei 10617, Taiwan, 6. Department of Geology, University of Birjand, Birjand, Iran)

5:15 PM - 7:00 PM

*Roberto F Weinberg1, Pengsheng Dong1, Di-Cheng Zhu2,3 (1. School of Earth, Atmosphere and Environment, Monash University, Clayton, VIC3800, Australia, 2. State Key Laboratory of Geological Processes and Mineral Resources, and School of Earth Science and Resources, China University of Geosciences, Beijing, 100083, China, 3. Frontiers Science Center for Deep Time Digital Earth, China University of Geosciences, Beijing 100083, China)

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