Latest News & Updates
Stay updated with our latest research findings, publications, and team achievements.
Latest News
Stay updated with our recent discoveries, achievements, and announcements
New Research Published in Nature Geoscience
Deep inside Earth, scientists have long puzzled over two giant mysterious regions above the planet’s core known as “large low shear-wave velocity provinces” (LLSVPs), along with smaller patches called “ultra-low velocity zones” (ULVZs). These regions look very different from the rest of the mantle in seismic images, but their origin has remained unclear. Our new research suggests they may have formed from an ancient “basal magma ocean” at the bottom of Earth’s mantle, which was gradually mixed with material exsolved from the core. This process, which we call a “basal exsolution contaminated magma ocean” (BECMO), prevented the buildup of unrealistic iron-rich layers and instead produced mantle structures that match what seismologists observe today. Computer models show that solidified BECMO material could explain both the vast LLSVPs and the smaller ULVZs. The BECMO also carries distinctive chemical signals—such as silicon, tungsten, and helium isotopes—that are often detected in volcanic rocks at ocean islands like Hawaii and Iceland. This means the same process may connect Earth’s deepest mantle to the volcanic activity we see at the surface, offering a unified explanation for some of the planet’s most enduring geochemical and geophysical mysteries.
Key Research Findings
• Core exsolution suppresses the crystallization of ferropericlase, helping reconcile models of magma ocean solidification with seismic observations.
• Geodynamic modeling shows these processes can produce mantle structures consistent with the anomalies we see in the lowermost mantle.
• This deep reservoir carries isotopic signals (Si, W, He) from the core — possibly explaining certain ocean island basalt sources.
• The framework has implications for other planets with long-lived basal magma oceans and core–mantle interactions.
Dr. Yuan started his new position as an assistant professor at Texas A&M
Dr. Yuan completed his O.K. Earl Postdoc research at Caltech before joining the Department of Geology and Geophysics at Texas A&M University, where he established the IMPACT Lab—Intelligent Modeling of Planetary Accretion, Convection, and Tectonics. He is also a core member of the Research in Artificial Intelligence for Science and Engineering (RAISE) Initiative at Texas A&M. The IMPACT Lab seeks to uncover how initial conditions, mantle dynamics, and geochemical differentiation shape Earth and other planets. By integrating cutting-edge AI/ML approaches with interdisciplinary geophysical and geochemical models, the lab aims to address fundamental questions about planetary formation, interior evolution, and long-term habitability.
Invited presentation at University of Chicago
Dr. Yuan was honored to be invited to deliver a departmental colloquium at the University of Chicago. Among the distinguished audience members was Nobel laureate Jack Szostak, renowned for his pioneering contributions to our understanding of the origin of life. Before the lecture, Dr. Yuan had the rare opportunity to engage in an extended and thought-provoking discussion with Professor Szostak, exploring how his own findings on planetary dynamics and early Earth processes may provide new perspectives on prebiotic chemistry and the conditions that made life possible. This exchange underscored the interdisciplinary significance of Dr. Yuan’s work, bridging planetary science, geodynamics, and questions at the very heart of biology.
Key Research Findings
• Interdisciplinary relevance – Dr. Yuan’s research on planetary dynamics and early Earth processes offers new insights that connect geophysics with prebiotic chemistry, helping to frame conditions under which life could emerge.
Featured in Science Magazine
Dr. Qian Yuan was interviewed by Science magazine for the article, Ancient crystals point to a surprisingly early start for plate tectonics. In the piece, he offered expert commentary on how these new findings fit into the broader debate about the onset of plate tectonics and the thermal and chemical evolution of the early Earth. His perspective highlighted both the strengths of the new evidence and the challenges of interpreting ancient signals from Earth’s formative history.
Key Research Findings
• While the zircon evidence is intriguing, it must be tested against geodynamic models to confirm whether Earth’s mantle could have sustained plate tectonics so early
Powering Up: Our New NVIDIA GeForce RTX 5080 Has Arrived
The arrival of the NVIDIA GeForce RTX 5080 marks a major boost for our AI-powered geodynamics research. Its advanced GPU architecture dramatically accelerates neural network training, enabling us to process vast geophysical datasets and run complex mantle convection simulations more efficiently. This computational power allows us to integrate machine learning with high-resolution geodynamic models, uncovering patterns and predictions that were previously out of reach. Looking ahead, we plan to acquire 10 NVIDIA H100 GPUs in the coming months, which will further expand our ability to push the frontier of AI-driven Earth and planetary science.
Key Research Findings
• Enhanced AI capabilities – The new NVIDIA GeForce RTX 5080 accelerates neural network training and high-resolution geodynamic simulations, enabling faster and more advanced AI-powered research.
• Scaling up resources – The planned purchase of 10 NVIDIA H100 GPUs will significantly expand computational capacity, positioning the lab to tackle larger datasets and more complex planetary science problems.
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AGU Fall Meeting 2025
📍 New Orleans, Louisiana
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Goldschmidt Conference 2026
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