Morphology and Scaling of Impact Craters in Granular Media
Authors:
- Kristi E. HollowayKHKristi E. Holloway
- Piotr HabdasPHPiotr Habdas
- 4 September 2003
- journal article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 91 (10) , 104301
Abstract
We present the results of experiments on impact craters formed by dropping a steel ball vertically into a container of small glass beads. As the energy of impact increases, we observe a progression of crater morphologies analogous to that seen in craters on the moon. We find that both the diameter and the depth of the craters are proportional to the 1/4 power of the energy. The ratio of crater diameter to rim-to-floor depth is constant for low-energy impacts, but increases at higher energy, similar to what is observed for lunar craters.Keywords
This publication has 12 references indexed in Scilit:
- Low-Speed Impact Craters in Loose Granular MediaPhysical Review Letters, 2003
- Granular jetsPhysics of Fluids, 2001
- IMPACT CRATER COLLAPSEAnnual Review of Earth and Planetary Sciences, 1999
- How Sandcastles FallPhysical Review Letters, 1998
- Crater formation in the laboratory: An introductory experiment in error analysisAmerican Journal of Physics, 1998
- Maximum angle of stability in wet and dry spherical granular mediaPhysical Review E, 1997
- The Scaling of Impact Processes in Planetary SciencesAnnual Review of Earth and Planetary Sciences, 1993
- Experimental planetary impact researchInternational Journal of Impact Engineering, 1987
- Terrace width variations in complex lunar cratersGeophysical Research Letters, 1986
- The origin of lunar cratersEarth, Moon, and Planets, 1975