1. Effect of projectile shape and interior structure on crater size in strength regime
- Author
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Kadono, T., Arakawa, M., Tsujido, S., Yasui, M., Hasegawa, S., Kurosawa, K., Shirai, K., Okamoto, C., Ogawa, K., Iijima, Y., Shimaki, Y., and Wada, K.
- Subjects
Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,Physics - Geophysics - Abstract
Experiments on crater formation in the strength regime were conducted using projectiles of various shapes with an aspect ratio of ~1, including both solid and hollow interiors. The surface diameter, inner (pit) diameter, and depth of the craters on basalt and porous gypsum targets were measured. Using the bulk density of the projectile, the surface diameter and depth for basalt and the pit diameter and depth for porous gypsum were scaled using the pi-scaling law for crater formation in the strength regime. The numerical code iSALE was used to simulate the impact of projectiles of various shapes and interior structure with similar bulk densities. Results show that the distributions of the maximum (peak) pressure experienced and particle velocity in the targets were similar regardless of projectile shape and interior structure, implying that the dimensions of the final craters were almost identical. This is consistent with the experimental results. Thus, we conclude that the size of the craters formed by the impact of projectiles with different shape and interior structure can be scaled using a conventional scaling law in the strength regime, using bulk density as projectile density., Comment: 38 pages, 9 figures, 4 tables, 1 supporting information, accepted for publication in Earth, Planets and Space
- Published
- 2022
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