#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Impact Ejecta Products and Processes: What Goes Up Must Come Down
Tuesday, March 14, 2023, 2:15 PM
Montgomery Ballroom
Chairs:
Ania Losiak
Chris Cline
Chris Cline
Moderator:
Nacia Luo
2:15 PM
Session Introduction
2:20 PM
Blance A. J.*
Rothery D. A.
Balme M. R.
Wright J.
Galluzzi V. A.
Far Greater Population of Flow Deposits Around Mercurian Impact Craters than Previously Known
[#2322]
Global survey of flow features around craters on Mercury, identifing at least 39 examples. Distribution, characteristics, and potential origins considered.
Global survey of flow features around craters on Mercury, identifing at least 39 examples. Distribution, characteristics, and potential origins considered.
2:30 PM
Burley J. M.*
Tornabene L. L.
Osinski G. R.
Grant J. A.
El-Maarry M. R.
Distal Flows Associated with Some of the Best-Preserved Craters on Mars: Implications for Extensive Impact-Related Landscape Modification (an Update)
[#1593]
Updated analysis of impact craters on Mars with expansive distal flow deposits (DFDs): Consistent flow phenomena within several distal ejecta zones is reported.
Updated analysis of impact craters on Mars with expansive distal flow deposits (DFDs): Consistent flow phenomena within several distal ejecta zones is reported.
2:40 PM
Neish C. D.*
Virkki A. K.
The Unusual Surface Texture of Venusian Impact Ejecta
[#1052]
Melt flows like lava / Smooths venusian ejecta / Botox for craters.
Melt flows like lava / Smooths venusian ejecta / Botox for craters.
2:50 PM
Alexander A. M.*
Grimm R. E.
Kirchoff M. R.
Formation of Layered-Ejecta Craters During Martian Glaciations: Insights from Numerical Modeling
[#2795]
We model impacts with iSALE 2D to asses the minimum thickness of surface ice needed to form layered-ejecta craters on Mars.
We model impacts with iSALE 2D to asses the minimum thickness of surface ice needed to form layered-ejecta craters on Mars.
3:00 PM
Panel Q&A
3:20 PM
Nypaver C. A.*
Thomson B. J.
Moersch J. E.
Kring D. A.
A Drone-Based Thermophysical Investigation of Barringer Meteorite Impact Crater Ejecta
[#2479]
Meteor Crater / Drone-based thermal inertia / What can it tell us?
Meteor Crater / Drone-based thermal inertia / What can it tell us?
3:30 PM
Prieur N. C.*
Amaro B.
Gonzalez E.
Rubanenko L.
Xiao Z.
et al.
Distribution of Impact-Generated Boulders on Planetary Surfaces: Influence of Target Fracturation and Lithology
[#2903]
A CNN is used to detect boulders around fresh impact craters. This database helps us understand the effect of target properties on crater ejection mechanisms.
A CNN is used to detect boulders around fresh impact craters. This database helps us understand the effect of target properties on crater ejection mechanisms.
3:40 PM
Grindrod P. M.*
Davis J. M.
Harris E.
Fawdon P.
Favaro E. A.
et al.
Extensive Secondary Cratering in the ExoMars Landing Site at Oxia Planum
[#1113]
Small craters abound / Perhaps most from Mojave / ExoMars can test.
Small craters abound / Perhaps most from Mojave / ExoMars can test.
3:50 PM
Chertok M. A.*
Lucey P. G.
Costello E. S.
Ireland S. M.
Mare Protolith Properties and Secondary Impacts Inferred from Rocky Crater Populations
[#1339]
We identify controls on rock abundance in crater ejecta by inspecting the size-frequency distributions of rocky crater populations across the lunar maria.
We identify controls on rock abundance in crater ejecta by inspecting the size-frequency distributions of rocky crater populations across the lunar maria.
4:00 PM
Panel Q&A
4:20 PM
Miklavcic P. M.*
Lee M.
Tokar E.
Askari H.
Examining Froude Number as a Scaling Factor for Granular Media in Changing Gravity Using Dynamic Resistive Force Theory
[#2863]
Dynamic Resistive Force Theory is modified to study Froude number scaling for oblique granular impacts in varying gravity. Discrete simulations verify findings.
Dynamic Resistive Force Theory is modified to study Froude number scaling for oblique granular impacts in varying gravity. Discrete simulations verify findings.
4:30 PM
Yamaguchi Y.*
Nakamura A. M.
Laboratory Experiments on Effect of Target Properties on Impact Ejecta Escaping from Martian Surface
[#1304]
We performed impact experiments to study the size-velocity-ejection angle relationship for ejecta faster than kilometers per second and its dependence on target properties.
We performed impact experiments to study the size-velocity-ejection angle relationship for ejecta faster than kilometers per second and its dependence on target properties.
4:40 PM
Cline C. J.*
Cintala M. J.
Anderson J. L. B.
Bart G. D.
Using Controlled Impact Experiments to Understand the Effects of Cohesive Blocks on the Cratering Process
[#1042]
Chaotic surface / Impact is inescapable / Ejecta motif.
Chaotic surface / Impact is inescapable / Ejecta motif.
4:50 PM
Dobson M. J.
Schulz T.
Koeberl C.*
Campbell K. A.
Rowe M.
et al.
Earth's Oldest Preserved Extraterrestrial Impact Deposit? Evidence for a Large Impactor 3.48 Billion-Year-Ago (Dresser Formation, Pilbara Craton, Australia)
[#1628]
Spherule-rich horizons in the ~3.48 Ga Dresser Formation, Pilbara Craton contain textural and preliminary geochemical results suggesting an impact origin.
Spherule-rich horizons in the ~3.48 Ga Dresser Formation, Pilbara Craton contain textural and preliminary geochemical results suggesting an impact origin.
5:00 PM
Panel Q&A
5:20 PM
Session Closure
*presenter