#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Lunar Volatiles and Where to Find Them
Thursday, March 16, 2023, 2:15 PM
Waterway Ballroom 1
Chairs:
Paul Lucey
Lauren Jozwiak
Lauren Jozwiak
Moderator:
Lingzhi Sun
2:15 PM
Session Introduction
2:20 PM
Schorghofer N.*
Rufu R.
Past Extent of Lunar Permanently Shadowed Areas
[#1806]
Building on recent results by Farhat et al. (2022), we calculate the axis tilt of the Moon and the extent of perennially shadowed areas over the last 3.5 Gyr.
Building on recent results by Farhat et al. (2022), we calculate the axis tilt of the Moon and the extent of perennially shadowed areas over the last 3.5 Gyr.
2:30 PM
Cannon K. M.*
Deutsch A. N.
Revisiting Ice Stratigraphies at the Lunar Poles
[#1259]
We revisit models of stochastic ice deposition at the lunar poles based on new findings about ballistic hopping and obliquity evolution.
We revisit models of stochastic ice deposition at the lunar poles based on new findings about ballistic hopping and obliquity evolution.
2:40 PM
Reach W. T.*
Lucey P. G.
Honniball C. I.
Arredondo A.
Malaret E. R.
Molecular Water in the Lunar Far South Using 6-Micron Spectral Imaging
[#1121]
We present the results of SOFIA observations in 2022 February, relating the distribution of surficial water with topographic features in the lunar far south.
We present the results of SOFIA observations in 2022 February, relating the distribution of surficial water with topographic features in the lunar far south.
2:50 PM
Ohtake M.*
Nakauchi Y.
Tanaka S.
Yamamoto M.
Onodera K.
et al.
Natural Water Ejection from the Lunar Surface Identified at the Polar Regions
[#1933]
We identified natural water ejection at the lunar polar region by using Spectral Profiler data onboard SELENE suggesting vigorous volatile migration.
We identified natural water ejection at the lunar polar region by using Spectral Profiler data onboard SELENE suggesting vigorous volatile migration.
3:00 PM
Panel Q&A
3:20 PM
López Días V.*
Pfister L.
Barnich F.
Lindner R.
Hissler C.
Water Ice Behavior Under Lunar Polar Harsh Environment — Theoretical and Experimental O-H Water Ice Kinetic Isotope Fractionation During Sublimation
[#2935]
The study of sublimation and related kinetic isotope fractionation helps to better understand the lunar water cycle and the raw data from future lunar missions.
The study of sublimation and related kinetic isotope fractionation helps to better understand the lunar water cycle and the raw data from future lunar missions.
3:30 PM
Poston M. J.*
Experimental Insights into Argon and Water Interactions with Lunar-Relevant Materials
[#2738]
Ultra-high vacuum thermal desorption experimental results of pre- and post- ion-irradiated lunar simulants.
Ultra-high vacuum thermal desorption experimental results of pre- and post- ion-irradiated lunar simulants.
3:40 PM
Flom A. J.*
Lucey P. G.
Honniball C. I.
Ferrari-Wong C. M.
Head J. W.
Variations in the Depth of the 3um Hydration Band During Lunar Eclipse: Implications for the Hypothesis of Ballistic Migration of Water
[#2763]
The lunar 3-µm hydration band increases strongly during the falling temperatures of a lunar eclipse, which appears to invalidate the hypothesis of ballistic migration of water.
The lunar 3-µm hydration band increases strongly during the falling temperatures of a lunar eclipse, which appears to invalidate the hypothesis of ballistic migration of water.
3:50 PM
Laferriere K. L.*
Bramson A. M.
Gleason A.
Temperature Driven Transport of Lunar Hydration on Diurnal Timescales
[#1047]
We simulate OH/H2O formation, migration and loss processes on the lunar surface to understand and interpret observations of diurnally variable hydration.
We simulate OH/H2O formation, migration and loss processes on the lunar surface to understand and interpret observations of diurnally variable hydration.
4:00 PM
Panel Q&A
4:20 PM
Poppe A. R.*
Halekas J. S.
Harada Y.
Is There a Dense Carbon-Dioxide Exosphere at the Moon?
[#1624]
We explore evidence that the Moon possesses a relatively dense carbon-dioxide exosphere due to neutral recycling of solar wind carbon ions.
We explore evidence that the Moon possesses a relatively dense carbon-dioxide exosphere due to neutral recycling of solar wind carbon ions.
4:30 PM
Himani T. P.*
Lewis K. W.
Patterson G. W.
Dutton N. T.
Rivera-Valentin E. G.
et al.
Examining the Dielectric Constant and Polarization Properties of Surficial Water Ice in the Lunar South Pole
[#1574]
Determining if dielectric constant inversion from radar data supports the existence of surficial water ice in certain PSRs of the lunar south pole.
Determining if dielectric constant inversion from radar data supports the existence of surficial water ice in certain PSRs of the lunar south pole.
4:40 PM
de Castro N.*
Li S.
Characterizing Spectral Features of Water Ice, Lunar Regolith Analogues, and Their Mixtures at the VNIR Region
[#2282]
Experiments on water ice and regolith simulant mixtures in the VNIR range as a function of particle size of water ice, viewing geometry, and water ice content.
Experiments on water ice and regolith simulant mixtures in the VNIR range as a function of particle size of water ice, viewing geometry, and water ice content.
4:50 PM
Ferrari-Wong C. M.*
Lucey P. G.
Honniball C. I.
Cold-Trapped Methane in Regions of Permanent Shadow (PSRs)
[#1835]
Methane at the poles / Frozen in the lunar cold / Waiting to be found.
Methane at the poles / Frozen in the lunar cold / Waiting to be found.
5:00 PM
Panel Q&A
5:20 PM
Session Closure
*presenter