Tin is a strategic key metal widely used in aerospace and high-tech industries. Worldwide, tin ore is mainly of magmatic hydrothermal type, and its formation is usually associated with highly differentiated reducing (ilmenite series) granite. However, the key factors that constrain the scale of tin ore formation have long been controversial, leading to unclear key control factors for the formation of large tin mines.
The 2025 China Geothermal Academic Conference and Deep Earth Energy Gold Stone Forum, initiated by the Earth Science Department of the National Natural Science Foundation of China, hosted by the Geothermal Professional Committee of the Chinese Geophysical Society, and organized by Dalian University of Technology, will be held in Dalian, Liaoning Province from October 11th to 13th, 2025. The aim is to deepen the exchange of the latest progress and achievements in China's geothermal field, promote the integration of cutting-edge theoretical research and engineering practice in geothermal science, and promote technological innovation in the development and utilization of deep earth energy.
Carbon, as a typical variable valence element, is mainly controlled by its oxygen fugacity (fO2) in the mantle. Under high oxygen fugacity conditions, carbon exists in the form of carbonates and CO2, which can significantly lower the mantle solidus line, induce partial melting, and form carbonate melts; In low oxygen fugacity environments, carbon exists in the form of diamond, graphite, or metal carbides, which are relatively stable in their reduced states and have no effect on the mantle solidus. Therefore, constraining mantle oxygen fugacity is crucial for studying deep carbon cycling.
In recent years, organic rich shale microfractures have attracted much attention due to their potential significant impact on hydrocarbon migration and recovery during unconventional shale oil and gas exploration and development, as well as underground in-situ transformation of oil shale (and medium low maturity shale oil). However, many issues regarding the evolution patterns of microcrack networks, the opening and closing times of microcracks, and the storage and migration of fluids within them are still unclear.
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Reporter:李文帅
Time:2023年4月2日(星期二)15:00
Place:钟健报告厅(系楼218)
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Reporter:常燎 研究员(北京大学地球与空间科学学院)
Time:2024年3月26日(星期二)10:00
Place:钟健报告厅(系楼218)