#LPSC2023
#LPSC2023

Program with Links to Abstracts
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Poster Session: Lunar Surface Processes 1
Thursday, March 16, 2023, 6:30 PM
Town Hall Exhibit Area
Mahanti P.*
Robinson M. S.
Williams J. P.
Mazarico E.
Details of Shadows — Subpixel Secondary Illumination in Shackleton and Spudis Permanently Shadowed Regions
[#2610]
Larger PSR areas with dim illuminations levels can contain smaller regions that are dimmer and potentially better cold traps with lower stability temperatures.
Larger PSR areas with dim illuminations levels can contain smaller regions that are dimmer and potentially better cold traps with lower stability temperatures.
Wöhler C.
Bhatt M.
Arnaut M.*
Ganesh S.
Aravind K.
et al.
Spectropolarimetric Properties of the Lunar Swirl Reiner Gamma and Western Oceanus Procellarum
[#1609]
This study discusses new telescopic multi-band spectropolarimetric imaging data of the lunar swirl Reiner Gamma and surrounding areas.
This study discusses new telescopic multi-band spectropolarimetric imaging data of the lunar swirl Reiner Gamma and surrounding areas.
Vines S. K.*
Waller C. D.
Fatemi S.
Anderson B. J.
Halekas J.
et al.
Modeling Plasma Interactions with the Reiner Gamma Magnetic Anomaly in Anticipation of the Arrival of Lunar Vertex
[#2150]
We present modeled magnetic field vectors and plasma fluxes in preparation for lunar vortex observations within the Reiner Gamma magnetic anomaly.
We present modeled magnetic field vectors and plasma fluxes in preparation for lunar vortex observations within the Reiner Gamma magnetic anomaly.
Kreslavsky M. A.*
Zubarev A.
Nadezhdina I.
Bondarenko N.
Non-Diffusive Regolith Transport on the Moon
[#1834]
A number of morphologies on the Moon indicate a dominant role of non-diffusive non-local regolith transport processes.
A number of morphologies on the Moon indicate a dominant role of non-diffusive non-local regolith transport processes.
Jhoti E.*
Powell T. M.
Paige D. A.
A Semi-Analytical Model for the Thermal Emission Phase Function of the Moon
[#2912]
Bowl craters on Moon / Model temperatures well / For extreme angles.
Bowl craters on Moon / Model temperatures well / For extreme angles.
Tai Udovicic C. J.*
Edwards C. S.
Ghent R. R.
Submicroscopic Iron Accumulation is Correlated with Local Iron Content
[#2832]
Our Moon space weathers / Shapes iron from near and far / Which one dominates?
Our Moon space weathers / Shapes iron from near and far / Which one dominates?
Sato H.*
Ohtake M.
Latitudinal Trend of the Lunar South Pole
[#1824]
Using our new south polar mosaic of the Kaguya MI, we examined the latitudinal dependence of the space weathering and geological structures above 40°S.
Using our new south polar mosaic of the Kaguya MI, we examined the latitudinal dependence of the space weathering and geological structures above 40°S.
Ikeda A.*
Kumagai H.
Morota T.
Production Processes of Boulders and Regolith on Lunar Crater Slopes Inferred from Topographic Feature and Rock Abundance
[#1303]
Our estimates of lunar crater slope conditions suggest that thermal fatigue in boulder sources has an important role for regolith production and movement.
Our estimates of lunar crater slope conditions suggest that thermal fatigue in boulder sources has an important role for regolith production and movement.
Pérez-Cortés S. L.*
Bramson A. M.
Nypaver C. A.
Patterson G. W.
Virkki A. K.
et al.
Comparison of Lunar Rockfalls Events in Different Geologic Settings Using Mini-RF Data
[#2492]
We are mapping mass-wasting events in different geologic settings on the lunar surface to investigate what factors trigger them and affect their morphology.
We are mapping mass-wasting events in different geologic settings on the lunar surface to investigate what factors trigger them and affect their morphology.
Aussel B.*
Rüsch O.
Lunar Rock Detection and Analysis for Characterizing Erosion Processes
[#1924]
We are developing a Mask R-CNN model that can detect rocks on LROC NAC cutouts. After detection, we model the reflectance profile across the boulder.
We are developing a Mask R-CNN model that can detect rocks on LROC NAC cutouts. After detection, we model the reflectance profile across the boulder.
Nypaver C. A.*
Thomson B. J.
Watters T. R.
Elder C. M.
Cahill J. T.
et al.
Lunar Boulder Fields as an Indicator of Recent Tectonic Activity
[#2824]
Wrinkle ridge boulders. Are they common on the Moon? How did they get there?
Wrinkle ridge boulders. Are they common on the Moon? How did they get there?
Marshal R. M.*
Rüsch O.
Wöhler C.
Wohlfarth K.
Velichko S.
et al.
Photometry of Rock-Rich Surfaces on Airless Bodies
[#1650]
Rocks on an airless / Body, can texture tell tales / Of transformation?
Rocks on an airless / Body, can texture tell tales / Of transformation?
Diotte F.*
Lemelin M.
Cloutis E. A.
Creating Microscopic Digital Elevation Models of Planetary Regolith Using Monocular Images and Convolutional Neural Networks
[#2294]
A deep learning algorithm is applied to monocular images of martian soils taken by the Microscopic Imager to study the soil’s surface microtopography.
A deep learning algorithm is applied to monocular images of martian soils taken by the Microscopic Imager to study the soil’s surface microtopography.
Suresh K.*
Iyer K. V.
Alurkar M. S.
Amitabh
An Improved Approach for Digital Elevation Model Generation Using Chandrayaan-2 Terrain Mapping Camera-2 (TMC-2) and Quality Assessment
Terrain Mapping Camera-2 (TMC-2) and Quality Assessment
[#1831]
This paper discusses about the improved approach of generating DTM with <50m of height accuracy.
This paper discusses about the improved approach of generating DTM with <50m of height accuracy.
Iqbal W.*
Hiesinger H.
van der Bogert C. H.
Heyer T.
Geology of Cone Crater for the Calibration of Lunar Chronology
[#1046]
Geologic analysis of Apollo 14 landing traverse.
Geologic analysis of Apollo 14 landing traverse.
Roseborough T. A.*
Henriksen M. R.
Bernhardt H.
Robinson M. S.
1:10,000 Morphologic Map of Tycho Crater Central Peak
[#2806]
Tycho central peak / Mapped on high-res DTM / What are unit slopes?
Tycho central peak / Mapped on high-res DTM / What are unit slopes?
Iqbal W.*
Gebbing T.
Borisov D.
Hiesinger H.
van der Bogert C. H.
New Geological Maps of the Apollo 14 and Apollo 16 Landing Sites
[#2000]
Updated geologic maps of the areas surrounding the Apollo 14 and 16 landing sites.
Updated geologic maps of the areas surrounding the Apollo 14 and 16 landing sites.
Mest S. C.*
Petro N. E.
Ostrach L. R.
Jolliff B. L.
Yingst R. A.
Update on the Geologic Mapping of the Apollo Lunar Quadrangle (LQ-24), Eastern South Pole-Aitken Basin
[#2803]
We present the updated geologic map of the Apollo Quadrangle (LQ-24) of the Moon.
We present the updated geologic map of the Apollo Quadrangle (LQ-24) of the Moon.
Roseborough T. A.*
Gonzales N. R.
Schoonover A. R.
Tewary V.
Woody J. A.
et al.
Apollo 16 and 17 Spatio-Temporal Traverse Mapping
[#2869]
Apollo missions! / Mapped the last two, using NACs / And mission data.
Apollo missions! / Mapped the last two, using NACs / And mission data.
Mikolajewski S.*
Hiesinger H.
van der Bogert C. H.
Schmedemann N.
Traversing the Rima Bode Region: An Updated Geological Map
[#2034]
We present our updates in mapping the Rima Bode region, as well as an investigated landing site.
We present our updates in mapping the Rima Bode region, as well as an investigated landing site.
Archinal B. A.*
Weller L. A.
Richie J. O.
Lee E. M.
Bennett K. A.
et al.
Controlled High-Resolution LROC NAC Polar Mosaics
[#2333]
The creation of controlled 1 mpp LRO LROC NAC polar mosaics, from 85° latitude, including 9 mpp illumination controlled mosaics at every 10° of solar longitude.
The creation of controlled 1 mpp LRO LROC NAC polar mosaics, from 85° latitude, including 9 mpp illumination controlled mosaics at every 10° of solar longitude.
Horvath T.*
Powell T. M.
Paige D. A.
High Resolution Mapping Method for Point-Based Planetary Datasets Using Effective Field of View Modeling
[#2734]
We used the known field of view of the Diviner instrument to develop a method that more properly represents the temperature data when creating thermal maps.
We used the known field of view of the Diviner instrument to develop a method that more properly represents the temperature data when creating thermal maps.
Shubham S.*
Cohen B. A.
Arevalo R.
Identifying Chemically Distinct Classes of Lunar Rocks Using Dimensionality Reduction Algorithms
[#2809]
We use unsupervised machine learning algorithms: PCA, and t-SNE to classify chemically distinct groups of lunar rocks using major oxide data.
We use unsupervised machine learning algorithms: PCA, and t-SNE to classify chemically distinct groups of lunar rocks using major oxide data.
Bernhardt H.*
Clark J. D.
Robinson M. S.
The Aristarchus Plateau as a Basis to Discuss Resuming Lunar Geologic Mapping After an Over Four-Decades-Long Lull
[#1104]
We use the complex Aristarchus plateau to discuss updated guidelines and techniques for a new generation of regional geologic maps of the Moon.
We use the complex Aristarchus plateau to discuss updated guidelines and techniques for a new generation of regional geologic maps of the Moon.
Meyer H. M.*
Clark J.
Robinson M. S.
Denevi B. W.
Revisiting the "Weird Terrain" on the Moon
[#1531]
Moon’s complex terrain / “Weird” you say, questions remain / With maps we redress.
Moon’s complex terrain / “Weird” you say, questions remain / With maps we redress.
Concepcion V. E.*
Hayne P. O.
Using Diviner Data to Analyze Characteristics of Overlapping Cold Spots Caused by a Serendipitous Lunar Impact
[#2428]
After an impact / On the surface of the Moon / Does a cold spot form?
After an impact / On the surface of the Moon / Does a cold spot form?
Bondarenko N. V.*
Possible Lack of Small Craters in “Elephant Hide” Areas on the Moon: A Case Study
[#2709]
Lack of 5–8-m-diameter craters on steep slopes points to the possibility that up to 1 m thick regolith layer is involved into “elephant hide” texture formation.
Lack of 5–8-m-diameter craters on steep slopes points to the possibility that up to 1 m thick regolith layer is involved into “elephant hide” texture formation.
*presenter