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Format
Hybrid Event
Location and Room
Mitchell Earth Sciences, 350/372
Address
397 Panama Mall, Stanford, CA 94305
Volatiles, such as water, CO2, and certain organic compounds, are not just life's building blocks but also regulate the climates and habitability on planetary bodies. By constraining results from current spacecraft exploration through data analysis and experiments, developing new space instrumentation, and exploring theoretical concepts, I seek to determine the key geological processes that affect the retention, loss, and chemical evolution of volatiles on planetary bodies.
In this seminar, I focus on our Red Neighbor as the focal point for comparison with Earth’s evolution. The contrast between the currently frozen Mars and the geological evidence for liquid water in its deep past raises significant questions about atmospheric and hydrospheric depletion over geological timescales on the red planet. The Perseverance rover is currentl
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