This research identifies potentially habitable rocky exoplanets by measuring their densities, water content, and internal heating through orbital interactions and transit observations. Using these techniques, several promising ocean and volcanic worlds have been identified as targets for the James Webb Space Telescope in the search for extraterrestrial life and habitable environments.

This research develops methods to detect and study exomoons, moons orbiting planets outside our solar system. By combining high-contrast imaging with indirect detection techniques, the work aims to identify exomoons, analyze their atmospheres, and search for biosignatures such as oxygen and methane that could indicate extraterrestrial life.

This research investigates the tilt of exoplanets to understand their formation and evolution. By developing a new measurement method, it identifies a Uranus-like tilted planet and enables broader study of planetary systems. These insights help reveal climates, histories, and potential habitability of distant worlds beyond our solar system.

The researcher studies how clouds on distant exoplanets affect their climates and potential for life. Working with NASA, they model how exotic materials—like iron or sapphire clouds—absorb and reflect light. They found particle shape greatly influences temperature and habitability, helping determine whether alien worlds could support liquid water and life.