#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Martian Hydrated Minerals and Aqueous Alteration
Wednesday, March 15, 2023, 2:15 PM
Waterway Ballroom 4
Chairs:
Rachel Slank
Adrian Brown
Adrian Brown
Moderator:
Christian Tate
2:15 PM
Session Introduction
2:20 PM
Safari M.*
Zimmermann N.
Nekvasil H.
Magmatic Gas-Induced Alteration of the Martian Basaltic Crust: Insights from Experiments
[#1403]
This work explores the magmatic gas-rock interactions and the contribution of gas-driven alteration products of common minerals to the martian fines and soils.
This work explores the magmatic gas-rock interactions and the contribution of gas-driven alteration products of common minerals to the martian fines and soils.
2:30 PM
Ralston S. J.*
Peretyazhko T. S.
Sutter B.
Ming D. W.
Morris R. V.
et al.
Phyllosilicate Formation on Early Mars via Open-System Acid Alteration of Basaltic Glass
[#1496]
Martian smectite clays / Could have formed by acid rain / Carbonates: unsolved.
Martian smectite clays / Could have formed by acid rain / Carbonates: unsolved.
2:40 PM
Szynkiewicz A.*
Moore R. D.
Evaluation of Water Activity Timescales on Mars Using Quantities of Sulfate Minerals Deposited in Meridiani Planum, Valles Marineris, and North Polar Dunes
[#2805]
If Mars was cold and dry in the past, it would have taken hundreds of millions of years to account for the sulfate minerals currently present on its surface.
If Mars was cold and dry in the past, it would have taken hundreds of millions of years to account for the sulfate minerals currently present on its surface.
2:50 PM
Bishop J. L.*
Parente M.
Saranathan A. M.
Gross C.
Itoh Y.
et al.
Diverse Phyllosilicate and Sulfate Assemblages in the Mawrth Vallis Channel
[#1913]
Discovery of several new assemblages of phyllosilicates and sulfates in the channel cutting through Mawrth Vallis indicates changing geochemical conditions.
Discovery of several new assemblages of phyllosilicates and sulfates in the channel cutting through Mawrth Vallis indicates changing geochemical conditions.
3:00 PM
Panel Q&A
3:20 PM
Das D.*
Turner S. M. R.
Gasda P. J.
Schwenzer S. P.
Palandri J.
et al.
Simulating Evaporative Wet and Dry Cycles in Gale Crater, Mars Using Thermochemical Modeling Techniques
[#2440]
Ten thousand tempers / Of wavering wet and wry / Shape smidge salt on Mars.
Ten thousand tempers / Of wavering wet and wry / Shape smidge salt on Mars.
3:30 PM
Archer P. D.*
Jakubek R. S.
Clark J. V.
Patterson R. V.
Casbeer P. D.
Using Secondary Minerals in a Hawaiian Lava Tube to Inform Salt Precipitation on Mars
[#2765]
In a lava tube / Basalt is altered, salts form / Maybe like on Mars?
In a lava tube / Basalt is altered, salts form / Maybe like on Mars?
3:40 PM
Shumway A. O.*
Catling D. C.
Toner J. D.
Regolith Inhibits Salt Crystallization in Magnesium Perchlorate Brine, Suggesting More Persistent and Habitable Brines on Mars
[#2478]
Mars-like brines in regolith act unlike ideal mixes of brine + regolith. Precipitation is inhibited, so brines may persist at drier conditions when in regolith.
Mars-like brines in regolith act unlike ideal mixes of brine + regolith. Precipitation is inhibited, so brines may persist at drier conditions when in regolith.
3:50 PM
Das E.*
Glotch T. D.
Edwards C. S.
Ye C.
Milliken R. E.
et al.
Investigating the Age, Abundance and Origin of Chloride Salt-Bearing Deposits on Mars
[#1680]
New insights into the formation of ubiquitous chloride deposits on Mars from global-scale abundance mapping and geochemical modeling.
New insights into the formation of ubiquitous chloride deposits on Mars from global-scale abundance mapping and geochemical modeling.
4:00 PM
Panel Q&A
4:20 PM
Caudill C. M.*
Osinski G. R.
Tornabene L. L.
EXOMARS Rosalind Franklin Rover Investigations: Analysis of Pancam Simulated Data for Assessment of In Situ Hydrated Mineralogy
[#2546]
This work seeks to support the PanCam team in determining which spectral combination best highlights hydrous minerals for its future surface explorations.
This work seeks to support the PanCam team in determining which spectral combination best highlights hydrous minerals for its future surface explorations.
4:30 PM
Brossier J.*
Altieri F.
De Sanctis M. C.
Frigeri A.
Ferrari M.
et al.
Characterizing Clay-Rich Terrains in Oxia Planum and North Xanthe Terra: An Updated Overview of the Infrared Signatures
[#1056]
We report an in-depth spectral analysis of clay-rich outcrops in Oxia Planum and north Xanthe Terra, both found along the circum-Chryse Planitia region.
We report an in-depth spectral analysis of clay-rich outcrops in Oxia Planum and north Xanthe Terra, both found along the circum-Chryse Planitia region.
4:40 PM
Ju E. M.*
Liu C. Q.
Ling Z. C.
Comparative Spectroscopic Study of Pyroxene and Hydrated Minerals Mixtures Relevant to Zhurong MarSCoDe SWIR Data Interpretation
[#1819]
This study focuses on the comparison of martian SWIR data with laboratory spectra for the study and quantification of mineral composition.
This study focuses on the comparison of martian SWIR data with laboratory spectra for the study and quantification of mineral composition.
4:50 PM
Comellas J. M.*
Sharma S. K.
Gasda P. J.
Cousin A.
Mayhew L.
et al.
The Identification of Serpentinization on Mars with Mars2020 SuperCam Instrument
[#2940]
Awash in red light / Hidden serpentinites thrive / Ripe for discov’ry.
Awash in red light / Hidden serpentinites thrive / Ripe for discov’ry.
5:00 PM
Panel Q&A
5:20 PM
Session Closure
*presenter