IMPACT-Lab Overview
Our research focuses on Intelligent Modeling of Planetary Accretion, Convection, and Tectonics (IMPACT). We aim to uncover how initial conditions, mantle dynamics, and geochemical differentiation have shaped Earth and other planets. By leveraging cutting-edge AI/ML techniques together with interdisciplinary geophysical and geochemical models, we seek to answer fundamental questions about planetary formation, interior evolution, and long-term habitability.
Research Areas
Simulate how Earth and planetary bodies form, evolve, and diversify
Moon-forming Giant Impact
Earth’s evolution began 4.5 billion years ago with the Moon-forming impact between Earth and the hypothesized planet Theia. We explore whether contine...
AI-powered Geodynamics
Neural operators enable geodynamic models to tackle both forward and inverse mantle convection, greatly accelerating simulations while maintaining acc...
Mars Dynamics
The internal structure of Mars, including its core, mantle, and crust, holds the key to explaining the planet’s hemispheric dichotomy and its long-ter...
Mantle Heterogeneities
The structure, morphology, and evolution of deep mantle heterogeneities—particularly the Large Low Shear Velocity Provinces (LLSVPs) and Ultra-Low Vel...
Tectonic Magmatism
Tectonic magmatism is a primary window into mantle–crust interactions, recording how melts ascend, react, and reshape the lithosphere. The differentia...
Ore-forming Magma Chamber Processes
Understanding their origin, the physical and chemical processes within magma chambers, and their tectonic context not only advances fundamental igneou...
Our Approach
We use cutting-edge AI and advanced computational methods to explore the dynamic processes that shape rocky planets across multiple scales and through deep time.
Research Impact
Collaborate With Us
Interested in our research? We welcome collaborations, student applications, and research partnerships — reach out to us at qyuan@tamu.edu