Page 12: 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.

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 ...

Atmospheric oxidation and the creation of modern Mars

Like Earth, Mars was formed about 4.5 billion years ago, but its early surface was very different than today's. Mars' surface then had high rates of meteorite and asteroid impacts from the period known as the Late Heavy Bombardment. ...

Fifteen years later, scientists locate a lunar impact site

In 2009, NASA intentionally crashed a spacecraft into the moon and used a small trailing spacecraft to observe the results: The Lunar Crater Observation and Sensing Satellite (LCROSS) was designed to search for frozen lunar ...

page 12 from 13