T. R. Watters

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About

T. R. Watters is a leading figure in planetary tectonics, with a career dedicated to unraveling the deformation histories of rocky bodies across the solar system. His primary research focuses on the structural geology of the Moon, Mercury, and Mars, where he investigates how global contraction and tidal stresses shape planetary surfaces. A landmark contribution is his 2024 study on the tectonics and seismicity of the lunar south polar region, which has already garnered 28 citations. This work demonstrates that lobate thrust fault scarps—evidence of ongoing contractional deformation—are present even in the polar regions, implying the Moon is tectonically active today. By linking these surface features to shallow moonquakes, Watters has fundamentally reshaped our understanding of lunar geodynamics and the hazards they pose for future exploration. His broader influence is evident in his role as an editor and contributor to foundational texts like *Planetary Tectonics*, which synthesizes decades of discoveries from robotic missions. With a career spanning the dawn of planetary geology to the Artemis era, Watters remains a pivotal voice in interpreting the forces that mold airless worlds.