B. S. McGrane

Papers

Total Citations

104

H-Index

About

B. S. McGrane is a planetary scientist whose research focuses on the surface processes and geological characteristics of Mars, particularly through the analysis of high-resolution imagery. Their most cited work, "Size‐frequency distributions of rocks on the northern plains of Mars with special reference to Phoenix landing surfaces" (2008, 104 citations), made a pivotal contribution by demonstrating that rock distributions >1.5 meters in diameter, as resolved by the HiRISE camera, follow exponential models consistent with lander-based measurements of smaller rocks. This finding bridged orbital and in situ observations, providing critical context for landing site safety and surface evolution studies. McGrane’s research has directly informed the selection and interpretation of landing sites for robotic missions, including the Phoenix lander, by quantifying rock hazards and surface roughness. Their work stands as a key reference in planetary geomorphology, offering a robust framework for understanding Martian regolith and impact gardening processes. With a citation count exceeding 100 for their flagship study, McGrane’s contributions continue to shape how scientists analyze planetary surfaces from orbit.