#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Lunar Surface Processes: Volcanoes, Craters, and Regolith
Thursday, March 16, 2023, 8:20 AM
Waterway Ballroom 1
Chairs:
Rebecca Ghent
Julie Stopar
Julie Stopar
Moderator:
Hannes Bernhardt
8:20 AM
Session Introduction
8:25 AM
Lawrence D. J.*
Stockstill-Cahill K. R.
Jozwiak L. M.
Peplowski P. N.
Wilson J. T.
Enhanced Thorium Abundances at Lunar Irregular Mare Patches
[#2284]
Moderately enhanced thorium abundances (3 to 8 ppm) are observed in the areas around lunar irregular mare patches.
Moderately enhanced thorium abundances (3 to 8 ppm) are observed in the areas around lunar irregular mare patches.
8:35 AM
Byron B. D.*
Elder C. M.
Glotch T. D.
Hayne P. O.
Pigue L. M.
et al.
Observations of Rock-Poor Material at Lunar Red Spots: Insights from Thermal Infrared and Radar Data Sets
[#2650]
We analyze lunar red spots with thermal IR and radar data. They are generally rock-poor with low thermal inertia and low CPR, due in part to pyroclastics.
We analyze lunar red spots with thermal IR and radar data. They are generally rock-poor with low thermal inertia and low CPR, due in part to pyroclastics.
8:45 AM
Rajasekhar R. P.*
Bhattacharya S.
Pathak S.
Naik S. S.
Bhiravarasu S. S.
et al.
Evidence for Young Lunar Volcanism in Mare Vaporum Region from Multi-Wavelength Remote Sensing Observations
[#2249]
synergistic study of two domes located in the Mare Vaporum region was carried out using CH-2 TMC and complimentary remote sensing data sets from recent missions.
synergistic study of two domes located in the Mare Vaporum region was carried out using CH-2 TMC and complimentary remote sensing data sets from recent missions.
8:55 AM
Morgan G. M.*
Campbell B. A.
Weitz C.
Jawin E. R.
Berman D.
et al.
Volcanic History of Mare Crisium: A Multiwavelength Radar Perspective
[#2847]
We will discuss the results of integrating Earth-based and Mini-RF bistatic data to map out volcanic deposits/structures within Mare Crisium.
We will discuss the results of integrating Earth-based and Mini-RF bistatic data to map out volcanic deposits/structures within Mare Crisium.
9:05 AM
Panel Q&A
9:25 AM
Cuevas-Quiñones S.*
Bramson A. M.
Rubanenko L.
Automated Crater Morphology Characterization on the Moon Using an Unsupervised Neural Network
[#2468]
We test the use of an autoencoder for systematic characterization of crater morphology and find it can distinguish well-defined crater rims from degraded rims.
We test the use of an autoencoder for systematic characterization of crater morphology and find it can distinguish well-defined crater rims from degraded rims.
9:35 AM
Ghent R. R.*
Costello E. S.
Parker A. H.
Characteristics of the Moon's Young Crater Population: Caught Between a Rock and a Rayed Place
[#2690]
Many lunar rays at equator / Are they born there faster? / Or do they die faster elsewhere? / We try to find the answer / (Rocks don’t seem to care).
Many lunar rays at equator / Are they born there faster? / Or do they die faster elsewhere? / We try to find the answer / (Rocks don’t seem to care).
9:45 AM
Liu T.*
Michael G.
Wünnemann K.
The Timeline of Early Lunar Bombardment Constrained by the Evolving Compositions of Differently-Aged Melt
[#1249]
The impact rate function of early lunar bombardment more likely has an exponential tail-off.
The impact rate function of early lunar bombardment more likely has an exponential tail-off.
9:55 AM
Chakraborty T.*
Putrevu D.
Bhiravarasu S. S.
Das A.
Pandey D. K.
et al.
Investigating the Effect of Crater Evolution Process on the Radar Scattering Behaviour of the Lunar Craters Using Chandrayaan-2 Dual-Frequency SAR Data
[#2006]
The abstract reveals dominance of crater degradation process on change in the physical nature of various impact craters leading to radar scattering variability.
The abstract reveals dominance of crater degradation process on change in the physical nature of various impact craters leading to radar scattering variability.
10:05 AM
Panel Q&A
10:25 AM
Powell T. M.*
Williams J.-P.
Greenhagen B. T.
Hayne P. O.
Paige D. A.
Discovery of a Lunar Cold Spot at the Apollo 16 South Ray Crater
[#2780]
We identify a cold spot around the Apollo 16 South Ray crater. Astronaut footprint depths and thermal modeling indicate a decrease in regolith density.
We identify a cold spot around the Apollo 16 South Ray crater. Astronaut footprint depths and thermal modeling indicate a decrease in regolith density.
10:35 AM
Frizzell E. S.*
Hartzell C. M.
Material Property and Particle Distribution Effects on Unconfined Inertial Dilation
[#2737]
Simulations investigating the expression of surface dilation as the result of granular shocks with the motivation of understanding lunar cold spot formation.
Simulations investigating the expression of surface dilation as the result of granular shocks with the motivation of understanding lunar cold spot formation.
10:45 AM
Weirich J. R.*
Domingue D. L.
Chuang F. C.
Sickafoose A. A.
Richardson M. D.
et al.
Reiner Gamma Swirl: Bright Albedo Features Trend Lower than Surrounding Topography
[#1271]
We find the bright on-swirl units are 4 meters lower than the dark off-swirl units at Reiner Gamma. Perhaps elevation plays a role during swirl formation.
We find the bright on-swirl units are 4 meters lower than the dark off-swirl units at Reiner Gamma. Perhaps elevation plays a role during swirl formation.
10:55 AM
Bürger J.*
Blum J.
Gundlach B.
Hayne P. O.
Läuter M.
et al.
Derivation of Lunar Regolith Properties from LRO/Diviner Data and Thermophysical Modeling
[#1185]
We present a microphysical thermal model for the lunar regolith and derived regolith properties, such as grain radius and stratification properties.
We present a microphysical thermal model for the lunar regolith and derived regolith properties, such as grain radius and stratification properties.
11:05 AM
Panel Q&A
11:25 AM
Session Closure
*presenter