Linking local lithologies to a larger landscape on Mars
NASA's Mars 2020 rover is continuing to explore a boundary visible from orbit dividing bright, fractured outcrop from darker, smoother regolith (also known as a contact).
Regolith is the unconsolidated, heterogeneous layer of fragmented mineral and rock material that overlies coherent bedrock on planetary surfaces, including Earth, the Moon, Mars, asteroids, and other solid bodies. As a substance, it comprises varying proportions of rock fragments, mineral grains, dust, ice, and, on some planets, secondary alteration products such as clays or salts. Regolith forms primarily through mechanical and chemical weathering, impact comminution, and volcanic or sedimentary processes, and its physical properties—such as grain size distribution, porosity, cohesion, and volatile content—critically influence surface-atmosphere interactions, geotechnical behavior, resource potential, and the performance of in situ exploration and construction activities.
NASA's Mars 2020 rover is continuing to explore a boundary visible from orbit dividing bright, fractured outcrop from darker, smoother regolith (also known as a contact).
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