Technical lecture about meteorite craters, 2019-12-03

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Peter Jedicke
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Technical lecture about meteorite craters, 2019-12-03

Post by Peter Jedicke » December 2nd, 2019, 4:38 pm

There will be a PhD Public Lecture on Tuesday 2019-12-03 at 13:00 in room 100 by
Ryan Hopkins
(supervised by Dr. Gordon Osinski)
on the topic
Numerical simulations of complex crater formation in layered and mixed targets

Numerical simulations of hypervelocity impact events provide a unique method of analyzing the mechanics that govern crater formation. This thesis describes modifications that were made to the impact Simplified Arbitrary Lagrangian Eulerian (iSALE) shock-physics code to more accurately simulate meteorite impacts into layered target sequences.

Meteorite impacts occur frequently in layered targets but resolving thin layers in the target sequence is computationally expensive and usually neglected in numerical simulations. To address this limitation iSALE was modified to include an anisotropic yield criterion and rotation scheme to simulate the effect of thin, weak layers interspersed in the target. This method reduces computational cost while replicating the morphology of the craters formed in high-resolution simulations with multiple weak layers modelled in the target geometry. Simulating layering via material anisotropy tends to increase the diameter and reduce the depth of the crater relative to a crater formed in an unlayered, isotropic target. Layering also appears to be partially responsible for suppressing central uplift formation during crater modification.

Comparisons of terrestrial impact structures suggest those that formed in sedimentary or mixed targets tend to have a smaller depth-diameter ratio relative to craters formed in purely crystalline targets. Furthermore, several terrestrial complex craters that formed in relatively thick sedimentary sequences (e.g., Haughton, Ries, Zhamanshin) do not have a central peak. An additional suite of ~60 simulations of impacts into mixed sedimentary-crystalline targets were created to further study the influence of the sedimentary layer on crater formation. The enhanced lateral motion of the weakened sedimentary material results in a crater that has a greater final diameter and reduced final depth relative to a crater formed in a purely crystalline target. Stratigraphic uplift tends to increase in thicker sedimentary targets, but the most uplifted material tends to be found at further radial distances from the point of impact.
Peter Jedicke, FRASC
London Centre Honorary President

"It could be true that my interest in abstractions is now being forgiven on grounds of senility." (Marilynne Robinson, "Gilead")

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