Hyper-velocity impacts on rubble pile asteroids
Most asteroids in the size range of approximately 100m to 100km are rubble piles, aggregates of rocky material held together mainly by gravitational forces, and only weak cohesion. They contain high macroporosities, indicating a large amount of void space in their interiors. How these voids are dist...
Main Author: | |
---|---|
Other Authors: | |
Published: |
University of Kent
2015
|
Subjects: | |
Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.682120 |