We are converging on a model for how the topography of airless bodies evolves, including process and rate. This understanding provides a framework for constraining the age of individual craters, features, and surfaces. Landform evolution was much faster on Mercury than the Moon. This may have important consequences for understanding early Mercury history.
Rate of Surface Evolution on the Moon and Mercury
2019
59 pages
Report
Keine Angabe
Englisch
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