#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Using and Improving Impact Models
Wednesday, March 15, 2023, 8:20 AM
Montgomery Ballroom
Chairs:
Veronica Bray
Maria Gritsevich
Maria Gritsevich
Moderator:
Greg Gosselin
8:20 AM
Session Introduction
8:25 AM
Jia W. Y.*
Luo X. Z.
Ding M.
Zhu M. H.
Effects of Megaregolith Porosity Structure on the Gravity Signature of Lunar Craters: Insights from Numerical Simulations
[#1920]
Porous lunar megaregolith. Different pre-impact porosities and thickness of the top porous layer. Different gravity anomalies of impact craters.
Porous lunar megaregolith. Different pre-impact porosities and thickness of the top porous layer. Different gravity anomalies of impact craters.
8:35 AM
Hundal C. B.*
Evans A. J.
Mustard J. F.
Factor Analysis Applied to Gravity Profiles of Lunar Impact Craters
[#2197]
Impact craters greatly influence crustal porosity. We improve crater signal isolation in GRAIL data by reducing to zonal harmonics and applying factor analysis.
Impact craters greatly influence crustal porosity. We improve crater signal isolation in GRAIL data by reducing to zonal harmonics and applying factor analysis.
8:45 AM
Luo X.-Z.*
Zhu M.-H.
Ding M.
Manske L.
Luther R.
et al.
Numerical Simulations of Shock Melting in Oblique Impacts
[#1427]
We performed a systematic suite of numerical simulations to quantify melt production for oblique impacts on the Moon.
We performed a systematic suite of numerical simulations to quantify melt production for oblique impacts on the Moon.
8:55 AM
Collins G. S.*
Miljković K.
Wójcicka N.
Rajšić A.
Lognonné P.
et al.
Modeling the 150-m Diameter "Christmas Eve" Impact Crater on Mars
[#2297]
Meteoroids falling, all around us / Scientists singing, having fun / It’s the reason for deeper understanding / Merry Christmas Eve crater everyone.
Meteoroids falling, all around us / Scientists singing, having fun / It’s the reason for deeper understanding / Merry Christmas Eve crater everyone.
9:05 AM
Panel Q&A
9:25 AM
Harwell M. L.*
Stewart S. T.
Citron R. I.
Caldwell W. K.
Plesko C. S.
Gaining Insights into Impact Events Through Rheology Regime Tracking
[#2838]
Tracking rheology / Gives insights into impacts / Nice animations.
Tracking rheology / Gives insights into impacts / Nice animations.
9:35 AM
Gao Y.*
Zhu M.-H.
Luther R.
Wünnemann K.
Numerical Simulation of Impact-Induced Seismic Wave Generation and Propagation Using a Coupled Approach
[#1990]
We use iSALE and classical seismic wave simulation coupled approach to implement numerical simulation of impact-induced seismic wave generation and propagation.
We use iSALE and classical seismic wave simulation coupled approach to implement numerical simulation of impact-induced seismic wave generation and propagation.
9:45 AM
Lee S.*
Johnson B. C.
Spatial Variation of Dwell Time Induced by a Hypervelocity Impact
[#2320]
We tested the spatial dwell time variation in a target to get a better understanding of impact process and check the validity of old estimation for dwell time.
We tested the spatial dwell time variation in a target to get a better understanding of impact process and check the validity of old estimation for dwell time.
9:55 AM
Rajsic A.*
Johnson B. C.
Hay H. C. F. C.
Collins G. S.
Reproducing Crater Morphologies Using the Melosh Model of Acoustic Fluidisation
[#1813]
We investigate the acoustic fluidization process during crater collapse using iSALE-2D shock physics code to simulate simple to complex crater transition.
We investigate the acoustic fluidization process during crater collapse using iSALE-2D shock physics code to simulate simple to complex crater transition.
10:05 AM
Panel Q&A
10:25 AM
Rae A. S. P.*
Kenkmann T.
Collins G. S.
Poelchau M. H.
Padmanabha V.
et al.
Rate-Dependent Strength and the Scaling of Impact Craters
[#1571]
Strain rate controls strength / Strength controls crater scaling / My FORTRAN’s working!
Strain rate controls strength / Strength controls crater scaling / My FORTRAN’s working!
10:35 AM
Du J.*
Minton D. A.
Blevins A. M.
Modeling the Realistic Rim Outlines of Fresh Lunar Craters Based on Their Power Spectral Densities
[#1290]
We create a crater rim that mimics a real lunar crater based on its power spectral density, from which the simple-to-complex transition can be found at D = 20 km.
We create a crater rim that mimics a real lunar crater based on its power spectral density, from which the simple-to-complex transition can be found at D = 20 km.
10:45 AM
Yamamoto Y.*
Arakawa M.
Yasui M.
Hasegawa S.
Yokota Y.
Impact Experiments for Crater Size Scaling Laws on Rubble-Pile Asteroids
[#2081]
We conducted impact experiments on granular targets composed by low-strength coarse-grains to study the effects of size and strength on the crater scaling law.
We conducted impact experiments on granular targets composed by low-strength coarse-grains to study the effects of size and strength on the crater scaling law.
10:55 AM
Sandtorf-McDonald J. R.*
Chevrier V. F.
Clathrate Crater Profiles: Impact Modeling in Clathrate-Rich Locations
[#2635]
This work uses iSALE shock physics program to model differences between craters produced in water ice and methane clathrate target surfaces.
This work uses iSALE shock physics program to model differences between craters produced in water ice and methane clathrate target surfaces.
11:05 AM
Panel Q&A
11:25 AM
Session Closure
*presenter