#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Poster Session: Martian Impact Craters
Tuesday, March 14, 2023, 6:30 PM
Town Center Exhibit Hall
Boyce J. M.*
Mouginis-Mark P. J.
Why are the Ramparts of Martian Impact Crater So High Relief?
[#1008]
We propose that martian ejecta ramparts are high relief compared with their landslide counterparts because of the high velocity of the ejecta flows.
We propose that martian ejecta ramparts are high relief compared with their landslide counterparts because of the high velocity of the ejecta flows.
Gao A. L.*
Daubar I. J.
Bart G. D.
Etgen A. D.
Characterizing Wind Streaks from Fresh Impacts on Mars
[#1402]
Wind streaks, linear streaks originating from some fresh impact craters on Mars, can provide insight into local wind conditions and topography.
Wind streaks, linear streaks originating from some fresh impact craters on Mars, can provide insight into local wind conditions and topography.
Rajsic A.*
Lagain A.
Anderson S.
Golombek M.
Warner N.
et al.
Rocky Ejecta Craters as a Proxy for the Evolution of Regolith on Mars
[#1843]
We use rocky ejecta craters to estimate regolith thickness in different geological units on Mars to estimate temporal evolution of regolith.
We use rocky ejecta craters to estimate regolith thickness in different geological units on Mars to estimate temporal evolution of regolith.
Peng Z.*
Rao M. N.
Nyquist L. E.
Geochemical and Mineralogical Characteristics of Zagami Impact Melts
[#1583]
This study is focus on a Zagami thin section. A combination of analytical techniques to investigate impact on geochemical and mineral constituents of Zagami.
This study is focus on a Zagami thin section. A combination of analytical techniques to investigate impact on geochemical and mineral constituents of Zagami.
Piatek J. L.*
Tornabene L. L.
Modification of Martian Crater Ejecta Facies Observed in Thermophysical Datasets
[#2760]
Mars, dusty, windy / Deposits, erodes craters / IR reveals.
Mars, dusty, windy / Deposits, erodes craters / IR reveals.
Lagain A.*
Bouley S.
Zanda B.
Miljković K.
Rajšić A.
et al.
The Ejection Site of Northwest Africa (NWA) 7034 and Paired Stones Revealed by 90 Million Impact Craters
[#1336]
Automatic identification of more than 90 million impact craters allows pinpointing the ejection site of NWA7034.
Automatic identification of more than 90 million impact craters allows pinpointing the ejection site of NWA7034.
Kamal Z. K.*
Ojha L. O.
Constraining Impact-Induced Demagnetization in Martian Crust with MAVEN Spherical Harmonics and Curie Depths
[#3031]
We take a closer look at demagnetization signatures in MAVEN data around impact-craters on Mars to better understand the timing of the dynamo’s demise.
We take a closer look at demagnetization signatures in MAVEN data around impact-craters on Mars to better understand the timing of the dynamo’s demise.
Robbins S. J.*
Megameter-Scale Crater Mismatch on Moon and Mars: Where Have Mars' Giant Craters Gone, if They Ever Existed?
[#2712]
From the Moon to Mars / A massive crater problem / How do we solve it?
From the Moon to Mars / A massive crater problem / How do we solve it?
Branco H. C.*
Miljkovic K.
Plesa A. C.
Scaling Relationships for Impact Basins on Mars
[#1348]
We derived preliminary impact scaling relationships for Mars’ basins based on numerical simulations for a range of impact conditions.
We derived preliminary impact scaling relationships for Mars’ basins based on numerical simulations for a range of impact conditions.
Sansom E. K.
Neidhart T.
Miljković K.*
Collins G. S.
Eschenfelder J.
et al.
Diversity of New Martian Crater Clusters Informs Meteoroid Atmospheric Interactions
[#2193]
A large diversity in crater cluster properties from 634 impact sites on Mars (including 557 newly mapped), inform atmospheric filtering effects.
A large diversity in crater cluster properties from 634 impact sites on Mars (including 557 newly mapped), inform atmospheric filtering effects.
Dohm J. M.*
Fink W.
Williams J.-P.
Mahaney W. C.
Ferris J. C.
et al.
Chicxulub-and Gale-Like Nicholson Impact
[#2163]
Gale and Nicholson impacts on Mars are interpreted to have impacted into half ocean and half land, similar to Chicxulub on Earth.
Gale and Nicholson impacts on Mars are interpreted to have impacted into half ocean and half land, similar to Chicxulub on Earth.
*presenter