#LPSC2023
#LPSC2023
Program with Links to Abstracts
Schedule Overview
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Special Session: The Geology of the Artemis Exploration Zone
Tuesday, March 14, 2023, 2:15 PM
Waterway Ballroom 1
Chairs:
David Kring
Carolyn van der Bogert
Carolyn van der Bogert
Moderator:
Margaret Landis
2:15 PM
Session Introduction
2:20 PM
Kring D. A.*
Impact Melting, Excavation, and Redeposition of Crustal Components Within the Artemis Exploration Zone: Implications for EVA Sampling
[#2180]
EVA sampling in the Artemis exploration zone provides an opportunity to explore the formation and impact-modification of the lunar crust.
EVA sampling in the Artemis exploration zone provides an opportunity to explore the formation and impact-modification of the lunar crust.
2:30 PM
Schmitt H. H.
Petro N. E.*
Considerations for High Latitude Landing Sites in Conjunction with Artemis Landings at the Lunar South Pole
[#2230]
Artemis crewed exploration should consider challenging landing sites at lower latitudes enable studies of permanent shadow and possible surface bound volatiles.
Artemis crewed exploration should consider challenging landing sites at lower latitudes enable studies of permanent shadow and possible surface bound volatiles.
2:40 PM
Patterson R. V.*
Lapen T. J.
Kring D. A.
Lemelin M.
Meier M. L.
Determining Ages of Rocks Accessible Within the Artemis Exploration Zone
[#2121]
We examine lithologies present within the Artemis zone, sample collection strategies, and discuss geochronological methods for return sample analyses.
We examine lithologies present within the Artemis zone, sample collection strategies, and discuss geochronological methods for return sample analyses.
2:50 PM
Bernhardt H.*
Robinson M. S.
A Geomorphic Map-Based Traverse Proposal on the Shackleton-de Gerlache Ridge Using a Sequential Risk/Science Assessment
[#1673]
Based on a geomorphic map and hazard assessment, we devised a science-focused traverse on the Shackleton-de Gerlache ridge that accepts successively more risks.
Based on a geomorphic map and hazard assessment, we devised a science-focused traverse on the Shackleton-de Gerlache ridge that accepts successively more risks.
3:00 PM
Panel Q&A
3:20 PM
Tripathi P.*
Goodwin A.
Peña-Asensio E.
Sutherland J.
Mason K.
et al.
Modeled EVA Traverses into Permanently Shadowed Regions near Shackleton Crater Rim and Connecting Ridge
[#1413]
This study evaluates the accessibility of PSRs as targets for EVA within a region near Shackleton crater, a potential site for Artemis crewed landings.
This study evaluates the accessibility of PSRs as targets for EVA within a region near Shackleton crater, a potential site for Artemis crewed landings.
3:30 PM
Longo A. Z.*
High-Value Science Targets in the Malapert Massif Artemis III Landing Region
[#2399]
Malapert Massif presents several enticing targets for Artemis III, including a PSR, an enigmatic low-albedo feature, and exposed crystalline massif material.
Malapert Massif presents several enticing targets for Artemis III, including a PSR, an enigmatic low-albedo feature, and exposed crystalline massif material.
3:40 PM
Moye C. G.*
Jolliff B. L.
Compositional Mixing Model for Estimating Proportions of South Pole Aitken Basin Material at Artemis 3 Candidate Landing Regions
[#2973]
We present a compositional mixing model to estimate the proportion of South Pole Aitken Basin material at the Artemis III candidate landing regions.
We present a compositional mixing model to estimate the proportion of South Pole Aitken Basin material at the Artemis III candidate landing regions.
3:50 PM
Thoresen F.*
Cowley A.
Mineralogy of the Moon Using Unsupervised Learning of the Moon Mineral Mapper (M3) Spectral Data
[#2239]
An unsupervised learning algorithm is made to cluster spectra from the Moon Mineral Mapper (M3).
An unsupervised learning algorithm is made to cluster spectra from the Moon Mineral Mapper (M3).
4:00 PM
Panel Q&A
4:20 PM
Moriarty D. P.*
Petro N. E.
Mineralogical Diversity of the Artemis Exploration Zone
[#2304]
Compositional remote sensing data suggests the presence of mantle-derived ejecta from the South Pole–Aitken Basin present within the Artemis Exploration Zone.
Compositional remote sensing data suggests the presence of mantle-derived ejecta from the South Pole–Aitken Basin present within the Artemis Exploration Zone.
4:30 PM
Landis M. E.*
Hayne P. O.
Williams J.-P.
Greenhagen B. T.
Paige D. A.
Predicted Buried Water Ice Stability Regions for the Moon's Poles from the Diviner Lunar Radiometer
[#1613]
We combine Diviner data and simple thermal and vapor diffusion models to predict where, within 30° of the lunar poles, buried water ice could be stable.
We combine Diviner data and simple thermal and vapor diffusion models to predict where, within 30° of the lunar poles, buried water ice could be stable.
4:40 PM
Thomson B. J.*
Fassett C. I.
Bhiravarasu S. S.
Neish C. D.
Nypaver C. A.
et al.
Characterization of Lunar Ice Stability Region (ISR) Host Craters: Size Distribution and Age Constraints
[#2560]
We find more small craters (<3 km) hosting ISRs in the N vs. the S. Because smaller craters are younger, any volatiles present within must be recently emplaced.
We find more small craters (<3 km) hosting ISRs in the N vs. the S. Because smaller craters are younger, any volatiles present within must be recently emplaced.
4:50 PM
Costello E. S.*
Lucey P. G.
Modeling the Production and Destruction of Cold Traps at the Human Scale of Artemis Exploration
[#1676]
Cold traps made, unmade / Complicating history / Where we will walk soon.
Cold traps made, unmade / Complicating history / Where we will walk soon.
5:00 PM
Panel Q&A
5:20 PM
Session Closure
*presenter