Ray Systems in Granular Cratering.
Tapan Sabuwala1, Christian Butcher2, Gustavo Gioia1
1Continuum Physics Unit, Okinawa Institute of Science and Technology Graduate University, Onna-son, Okinawa 904-0495, Japan.
Physical Review Letters
|July 14, 2018
Summary
Surface undulations transform ejecta blankets into ray systems during granular cratering. The number of rays correlates with impactor size and surface wavelength, offering insights into planetary cratering.
Area of Science:
- Planetary Science
- Geophysics
- Fluid Dynamics
Background:
- Classical granular cratering experiments yield uniform ejecta blankets.
- The influence of surface topography on ejecta patterns has been largely unaddressed.
Purpose of the Study:
- To investigate how surface undulations affect ejecta patterns in granular cratering.
- To understand the formation mechanism of rayed crater systems.
Main Methods:
- Conducted numerous granular cratering experiments.
- Performed computational simulations of the cratering process.
- Analyzed the relationship between impactor size, surface wavelength, and ray system characteristics.
Main Results:
- Surface undulations transform uniform ejecta blankets into ray systems.
- The number of rays in a ray system is directly proportional to the impactor diameter (D) and inversely proportional to the surface undulation wavelength (λ).
- Ejecta forming ray systems originate from a narrow annular region around the impact site.
Conclusions:
- Surface topography is a critical factor in determining ejecta patterns.
- The findings provide a physical model for the formation of rayed craters observed on planetary bodies.
- This research may help explain enigmatic ray systems on the Moon and other celestial bodies.
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