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About

Dr. Paul Morgan is a pioneering planetary scientist whose work has fundamentally advanced our understanding of Martian geology and thermal evolution. His primary research focuses on planetary heat flow, geophysical instrumentation, and the subsurface properties of terrestrial bodies. Morgan's most significant contribution is his leadership in developing the Heat Flow and Physical Properties Package (HP3) for NASA's InSight mission, which aimed to achieve the first-ever direct measurement of Mars' planetary heat flow—a critical parameter for understanding the planet's formation and tectonic history. This landmark instrument, designed to penetrate up to 5 meters into the Martian subsurface, represents a decade of innovative engineering and scientific collaboration. The associated 2018 paper detailing HP3 has garnered 146 citations, underscoring its foundational role in planetary science. Despite the instrument's eventual challenges with the Martian regolith, Morgan's work set a new benchmark for in-situ geophysical measurements on another world. His research continues to shape mission design and our comprehension of planetary interiors, making him a key figure in the next generation of Mars exploration.