Research news on impact cratering

Impact cratering is the process by which hypervelocity collisions of extraterrestrial bodies (e.g., asteroids, comets, meteoroids) with a planetary surface excavate material and form characteristic circular depressions. It involves three main stages: contact and compression, where shock waves propagate and generate extreme pressures and temperatures; excavation, during which target material is displaced outward and upward, forming a transient cavity and ejecta; and modification, where gravitational collapse and rock rheology reshape the transient cavity into a final crater morphology. Impact cratering is a fundamental geologic process that influences crustal structure, surface evolution, and volatile redistribution on solid bodies throughout the Solar System.

Primordial mini-moons may explain meteorite composition

A new Southwest Research Institute-led study proposes a solution to a longstanding puzzle in planetary science: What caused the concentration, assembly, and preservation of millimeter-sized, spherical mineral grains within ...

Discrepancies in AI lunar crater catalogs discovered

A new Southwest Research Institute-led study compared eight AI-generated lunar crater catalogs, discovering that many of their published performance metrics drop sharply when the databases are evaluated using the same scientific ...

How NASA taught four astronauts to read the moon

How do you teach someone to look at the moon? Not glance at it, the way we all have on a clear night, but truly read it, the way a geologist reads a hillside. That was the challenge NASA set itself before Artemis II, because ...

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