#LPSC2023
#LPSC2023

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Poster Session: Lunar Surface Processes
Wednesday, March 15, 2023, 6:30 PM
iPosters/Gather.town
Allen C. C.*
Mare Lavas and Mascons — A Tale of Two Basins
[#1381]
The compositions and timing of mare basalts flows vary among lunar impact basins and are likely influenced by the presence or absence of mascons.
The compositions and timing of mare basalts flows vary among lunar impact basins and are likely influenced by the presence or absence of mascons.
Liu T.*
Allibert L.
Luther R.
Wünnemann K.
Zhu M.-H.
et al.
The Synergetic Effect of the Potential Procellarum and the South-Pole Aitken Impact on the Formation of the Lunar Nearside-Farside Asymmetries
[#1251]
The systematic simulations including the Procellarum impact, the SPA impact will quantitatively estimate the integrated outcome of two early major events.
The systematic simulations including the Procellarum impact, the SPA impact will quantitatively estimate the integrated outcome of two early major events.
Basilevsky A. T.*
Li Yu.
Fang L. G.
Surface Morphology Inside the PSR Part of Lunar Polar Crater Shoemaker in Comparison with that of the Sunlit Areas
[#1457]
A geological analysis was made of hillshade images of four study areas inside PSR part of polar crater Shoemaker and at the Lunokhod-2 region and Apollo 16 site.
A geological analysis was made of hillshade images of four study areas inside PSR part of polar crater Shoemaker and at the Lunokhod-2 region and Apollo 16 site.
Honniball C. I.*
Burgdorf M. J.
Lucey P. G.
Mueller T.
Chen Y.
et al.
Lunar Observations from 5 to 8 Microns with SOFIA and the Suomi Cross-Track Infrared Sounder: Water and Christiansen Feature Results
[#2114]
Comparison of lunar spectral shapes observed by SOFIA and CrIS from 5 to 8 µm and results of molecular water at 6 µm and the Christiansen feature.
Comparison of lunar spectral shapes observed by SOFIA and CrIS from 5 to 8 µm and results of molecular water at 6 µm and the Christiansen feature.
Magnarini G.*
Grindrod P. M.
Mitchell T. M.
Evidence of Recent Slope Deformation and the Lasting Effect of Local Subsurface Geometry in the Taurus-Littrow Valley, Apollo 17 Landing Site
[#1055]
Slope deformation is the product of recent tectonism associated with the Lee-Lincoln fault, coupled with the influence of the valley subsurface geometry.
Slope deformation is the product of recent tectonism associated with the Lee-Lincoln fault, coupled with the influence of the valley subsurface geometry.
Ambily G.*
Durga Prasad K.
Diurnal Temperature Variations of Latitudinally and Geologically Distinct Sites on the Moon
[#2231]
We have processed LOLA & Diviner datasets onboard LRO, of four distinct sites and diurnal temperature variations of the lunar surface were studied and presented.
We have processed LOLA & Diviner datasets onboard LRO, of four distinct sites and diurnal temperature variations of the lunar surface were studied and presented.
Maganti T.*
Chakraborty T.
Putrevu D.
Bhiravarasu S. S.
Das A.
et al.
First Ever Circular Polarization Ratio (CPR) and Radar Scattering Map of Lunar Poles in L-Band Using Full-Pol Chandrayaan-2 DFSAR Data
[#1993]
DFSAR’s fully polarimetric dataset “frequently utilised polarimetric products” mosaics were generated for regional studies of the lunar surface features.
DFSAR’s fully polarimetric dataset “frequently utilised polarimetric products” mosaics were generated for regional studies of the lunar surface features.
Cai Y.*
Guo J.
Estimation of the Dielectric Characteristics of Lunar Subsurface Layers Using the Kaguya Lunar Radar Sounder
[#2071]
we used the data from the 5 MHz Lunar Radar Sounder (LRS) carried on SELENE to estimate the relative dielectric constant of lunar subsurface layers.
we used the data from the 5 MHz Lunar Radar Sounder (LRS) carried on SELENE to estimate the relative dielectric constant of lunar subsurface layers.
Dsouza H.*
Kumar S.
Polarimetric Analysis of de Gerlache Crater Using Chandrayaan-2 DFSAR Data
[#1449]
Data from L-band DFSAR onboard Chandrayaan-2 was used to analyse the polarimetric scattering behaviour on the surface of de Gerlache crater.
Data from L-band DFSAR onboard Chandrayaan-2 was used to analyse the polarimetric scattering behaviour on the surface of de Gerlache crater.
Pandey D. K.*
Putrevu D.
Chakraborty T.
Das A.
Bhiravarasu S. S.
et al.
Joint Estimation of High Resolution Lunar Dielectric Constant and Surface Roughness Using Full-Polarimetric Data from Chandrayaan-2 Dual Frequency SAR
[#2012]
In this study, we adopted a two-layer physical radar scattering model for joint estimation of dielectric constant and surface roughness using DFSAR data.
In this study, we adopted a two-layer physical radar scattering model for joint estimation of dielectric constant and surface roughness using DFSAR data.
Shukla S.*
Patterson G. W.
Dutton N. T.
Himani T. P.
Maiti A.
Quantitative Constraints of Near Surface Roughness on Lunar Water Ice Under Bistatic Radar Configuration
[#1267]
Near-surface roughness controls the bistatic radar scattering and imposes quantitative constraints on the physical form and abundance of water ice on the Moon.
Near-surface roughness controls the bistatic radar scattering and imposes quantitative constraints on the physical form and abundance of water ice on the Moon.
Srivastava A.*
Chauhan M.
Mare Smythii: A Detailed Look at the Eastern Limb of the Moon Using High-Resolution Data
[#2338]
Mare Smythii, on the nearside-farside transition zone of the Moon, is geologically investigated for its wide morphological as well as mineralogical variability.
Mare Smythii, on the nearside-farside transition zone of the Moon, is geologically investigated for its wide morphological as well as mineralogical variability.
Panwar N.*
Srivastava N.
Geology of Scaliger Crater Region: Implications for Magmatism in the Australe North Basin
[#2022]
Australe North is a pre-Nectarian basin first identified by GRAIL. The study probes the magmatic history of this basin by investigating the Scaliger Crater region.
Australe North is a pre-Nectarian basin first identified by GRAIL. The study probes the magmatic history of this basin by investigating the Scaliger Crater region.
Surkov Y.*
Kaydash V.
Shkuratov Y.
Videen G.
Mall U.
Assessment of Abundance of Mg-Spinel Using M3 Data: The Theophilus Crater Peak
[#1454]
The new approach to assess abundance of Mg-spinel in the lunar regolith is presented. It was tested on the region of the Theophilus crater peak.
The new approach to assess abundance of Mg-spinel in the lunar regolith is presented. It was tested on the region of the Theophilus crater peak.
Ojha S. P.*
Dagar A.
Bhattacharya S.
Desai N. M.
Kumar A. S. K.
Lunar Surface Hydration Estimation over Compton-Belkovich Volcanic Complex (CBVC) Region Using Chandrayaan-2 IIRS Observations
[#2132]
In this study, the lunar surface hydration estimation over the Compton-Belkovich region is estimated using thermally corrected Chandrayaan-2 IIRS observations.
In this study, the lunar surface hydration estimation over the Compton-Belkovich region is estimated using thermally corrected Chandrayaan-2 IIRS observations.
Nodjoumi G.*
Luzzi E.
Massironi M.
Pozzobon R.
Rossi A. P.
A Semi-Automated Method for Displacement-to-Length Scaling of Faults Populations
[#2024]
This work presents an open-source, Jupyter-based semi-automated method for displacement-to-length scaling of fault populations.
This work presents an open-source, Jupyter-based semi-automated method for displacement-to-length scaling of fault populations.
Sinha R. K.*
Rani A.
Ruj T.
Bhardwaj A.
Lobate Scarp in the Vicinity of Chandrayaan-3 Landing Site in the Southern High Latitudes of the Moon: Insights into Formation Age and Seismicity
[#1135]
The proposed primary landing site of the Chandrayaan-3 mission could have experienced shallow moonquakes of cumulative moment magnitude of 9.2 during the past ~50 Ma.
The proposed primary landing site of the Chandrayaan-3 mission could have experienced shallow moonquakes of cumulative moment magnitude of 9.2 during the past ~50 Ma.
Devaraj A.*
Narendranath S.
Kartha S. S.
Pillai N. S.
Tadepalli S. P.
Global Oxygen Distribution on the Lunar Surface: First Results Using Chandrayaan-2
[#2026]
We present the first results on the global distribution of oxygen on the Lunar surface. The XRF spectra from CLASS onboard Chandrayaan-2 was used for analysis.
We present the first results on the global distribution of oxygen on the Lunar surface. The XRF spectra from CLASS onboard Chandrayaan-2 was used for analysis.
Nguyen D. T.*
Jacquemoud S.
Lucas A.
Coustance S.
Marcq S.
et al.
Photometric Characterization of Planetary Surfaces: When the Earth Meets the Moon
[#1239]
Photometry was applied on multi-angular remote sensing data of Earth and the Moon, to extract surface characteristics, including the surface roughness.
Photometry was applied on multi-angular remote sensing data of Earth and the Moon, to extract surface characteristics, including the surface roughness.
Sikes C.*
Sunshine J. M.
Newcombe M.
Formation of the Spinel-Rich Sinus Aestuum Dark Mantle Deposits
[#1789]
Strange spinels are seen / Mapping and melting reveal / Scraps of lunar past.
Strange spinels are seen / Mapping and melting reveal / Scraps of lunar past.
Moriarty D. P.*
James P.
North A.
Wagner N.
Evidence for Widespread Silicic Lithologies Across the Gruithuisen-Mairan Region
[#2346]
Integrated compositional remote sensing analyses demonstrate the presence of silicic, thorium-bearing lithologies across Mare Imbrium and the Mairan highlands.
Integrated compositional remote sensing analyses demonstrate the presence of silicic, thorium-bearing lithologies across Mare Imbrium and the Mairan highlands.
Moitra H.*
Pathak S.
Gupta S.
Bhattacharya S.
Investigation of Multiple Basaltic Volcanism Events in the Floor of the Wolf Crater Complex
[#2944]
Multiple in situ basaltic eruptions have occurred within the central depression of Wolf crater complex that stand over a time period between 2.0 and 2.8 Ga.
Multiple in situ basaltic eruptions have occurred within the central depression of Wolf crater complex that stand over a time period between 2.0 and 2.8 Ga.
Zhang M.*
Fa W.
Eke V. R.
Modeling the Evolution of Regolith Thickness: Implications for Growth Rate and Spatial Distribution
[#1188]
A Monte Carlo based Lunar Topography and Regolith Evolution Model (LTREM) is developed to simulate the growth rate and spatial distribution of lunar regolith.
A Monte Carlo based Lunar Topography and Regolith Evolution Model (LTREM) is developed to simulate the growth rate and spatial distribution of lunar regolith.
*presenter