#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Physical Properties in the Artemis Exploration Zone
Wednesday, March 15, 2023, 8:20 AM
Waterway Ballroom 1
Chairs:
Ariel Deutsch
Brad Thomson
Brad Thomson
Moderator:
Hannes Bernhardt
8:20 AM
Session Introduction
8:25 AM
O'Brien P.*
Hayne P. O.
Landis M. E.
Byrne S.
Seasonal Illumination at the Lunar Poles: Partial Double Shadows and Super-Volatile Stability
[#2668]
What illumination conditions are necessary for the existence of ultra-cold traps on the Moon?
What illumination conditions are necessary for the existence of ultra-cold traps on the Moon?
8:35 AM
Lucas M. P.*
Neal C. R.
Long-Fox J.
Britt D.
The Road to the Artemis Base Camp via Applied Science: Estimating the Bulk Density of Lunar Regolith Stratigraphy Through Cone Penetrometer Testing of Simulants
[#1977]
The density of lunar regolith layers can be estimated via cone penetrometer readings of simulants in the lab, which will guide future infrastructure development.
The density of lunar regolith layers can be estimated via cone penetrometer readings of simulants in the lab, which will guide future infrastructure development.
8:45 AM
Connolly J. F.*
Carrier W. D.
Updating Lunar Subsurface Geotechnical Properties Based Upon Nonlinear Winkler Modeling of Apollo and Lunokhod Measurements
[#1029]
Analysis of Apollo and Lunokhod geotechnical measurements yielded an updated understanding of how lunar soil behaves nonlinearly with depth. Updates LSB figures.
Analysis of Apollo and Lunokhod geotechnical measurements yielded an updated understanding of how lunar soil behaves nonlinearly with depth. Updates LSB figures.
8:55 AM
Deutsch A. N.*
Bickel V. T.
The Elongation of Small Craters on Steep Lunar Slopes: Do Polar Volatiles Enhance Elongation and Mass Wasting?
[#2524]
We analyze the elongation of small lunar craters formed on polar vs. lower-latitude slopes, and discuss how volatiles may enhance crater elongation.
We analyze the elongation of small lunar craters formed on polar vs. lower-latitude slopes, and discuss how volatiles may enhance crater elongation.
9:05 AM
Barker M. K.*
Mazarico E.
Neumann G. A.
Smith D. E.
Zuber M. T.
et al.
A New Look at the Topography of the Lunar South Pole with LOLA
[#1532]
New and improved LOLA altimetry at the lunar south pole reveals a diversity of terrains characterized by their roughness on hectometer to kilometer scales.
New and improved LOLA altimetry at the lunar south pole reveals a diversity of terrains characterized by their roughness on hectometer to kilometer scales.
9:15 AM
Patterson G. W.*
Bhiravarasu S. S.
Fassett C. I.
Thomson B. J.
Cahill J. T. S.
et al.
Availability of LRO Mini-RF and Chandrayaan-2 DFSAR Data for Artemis Landing Zone Characterization
[#2397]
Mini-RF and DFSAR data are valuable for identifying landing hazards and constraining the dielectric properties of regolith within the Artemis landing zones.
Mini-RF and DFSAR data are valuable for identifying landing hazards and constraining the dielectric properties of regolith within the Artemis landing zones.
9:25 AM
Panel Q&A
9:50 AM
Transition to New Session
*presenter
