Page 9: 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.

A new mission watches meteoroids hit the far side of the moon

Sometimes, it's hard to remember that Earth is constantly being bombarded by literally tons of space debris daily. The larger bits form what we know as shooting stars, and most burn up in the atmosphere. Still, throughout ...

New lunar map can help guide future sample return missions

Billions of years ago, a giant asteroid struck the moon with so much energy that it melted rock until it was super-heated and white-hot, or what scientists call impact melt. This eventually cooled and hardened, creating a ...

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