Page 4: 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.

Massive impact could be the cause of our lopsided moon

Our nearest neighbor, the moon, is still something of a mystery to us. For decades, scientists have wondered why it appears so lopsided, with dark volcanic plains on the near side (the side we see) and rugged, cratered mountains ...

The hidden danger of lunar micrometeoroid storms

The moon has no significant atmosphere, no weather, and no wind. Yet it faces an invisible bombardment more relentless than any terrestrial storm, a constant rain of micrometeoroids, tiny fragments of rock and metal traveling ...

What a Martian ice age left behind

Traveling up from the Mars equator toward its north pole, we find Coloe Fossae: a set of intriguing scratches within a region marked by deep valleys, speckled craters, and signs of an ancient ice age.

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