K. R. Ramsley

Papers

Total Citations

H-Index

About

K. R. Ramsley is a planetary scientist whose research focuses on the long-term evolution and physical processes shaping the surfaces of airless bodies, including the Moon, asteroids, and Mercury. His most-cited work, "Survival times of meter-sized rock boulders on the surface of airless bodies" (2015, 83 citations), provides a foundational framework for understanding how boulders fragment and degrade under micrometeoroid bombardment and thermal cycling over millions of years. This study has become a key reference for interpreting surface age and regolith development on planetary bodies, directly informing missions like NASA's Lunar Reconnaissance Orbiter and asteroid sample-return efforts. Ramsley’s broader contributions include modeling impact gardening, electrostatic dust transport, and the thermal history of small bodies, often bridging laboratory experiments with remote sensing data. His work has been instrumental in refining our understanding of how airless worlds evolve, with implications for future human exploration and resource utilization on the Moon. Through rigorous quantitative modeling and interdisciplinary collaboration, Ramsley has established himself as a leading voice in planetary surface processes, helping to decode the silent, slow-motion geology of our solar system’s most ancient landscapes.