Research
We are working to better understand the atmosphere and hydrologic cycle of Saturn’s moon Titan, a unique yet Earth-like world with an exotic but recognizable hydrologic cycle based on methane. Titan is the only body in the Solar System besides Earth with a massive nitrogen atmosphere and stable surface liquids, and its climate system plays an important role in many observable phenomena. In addition to having an atmosphere full of organic molecules, Titan likely hosts a sub-surface water ocean; it is therefore a key target for astrobiological exploration.
Our main tool to investigate Titan is our ever-evolving climate model, the Titan Atmospheric Model, a general circulation model that is now coupled to a self-consistent surface hydrology model. We supplement our simulations with theory and analysis of observations of Titan, a wealth of which is available from the Cassini mission.
We also investigate various aspects of other Solar System worlds, including the atmospheres of Jupiter, Uranus and Neptune, as well as Earth’s water cycle with a particular focus on atmospheric rivers. Generally, we are interested in a broad, mechanistic understanding of climate, and bridging terrestrial climate and planetary sciences.
Collaborations
Dragonfly is a rotorcraft lander that will explore Titan in the 2030s. It is NASA’s fourth New Frontiers Program mission selection. This amazing mission will sample Titan’s surface materials, investigate prebiotic chemistry, and monitor, and make measurements of the atmosphere—including during flights.
ARTMIP is the Atmospheric River Tracking Method Intercomparison Project, a project to compare methods for detecting atmospheric rivers. The goal is to better understand and quantify uncertainties in atmospheric river science based on methodology. ARTMIP also maintains a series of detection catalogues and corresponding datasets.