#LPSC2023
#LPSC2023

Program with Links to Abstracts
Schedule Overview
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Poster Session: Mars
Wednesday, March 15, 2023, 6:30 PM
iPosters/Gather.town
Lucas A.*
Rohilla S.
Mangeney A.
Bourdon L.
Sainton G.
et al.
Seismic Detectability of Avalanches on Mars
[#1559]
We discuss the seismic detectability of mass wasting on Mars.
We discuss the seismic detectability of mass wasting on Mars.
Lucas A.*
Daubard I. J.
Le Teuff M.
Posiolova L. V.
Sainton G.
et al.
Discussion on Seismically Triggered Avalanches on Mars
[#1288]
We discuss the avalanche rate after a large marsquake detected by SEIS.
We discuss the avalanche rate after a large marsquake detected by SEIS.
Apuzzo A. A.*
Frigeri A.
Salvini F. S.
Brossier J. B.
De Sanctis M. C.
et al.
Directional Analysis of Fractures at Oxia Planum, Mars
[#1169]
Study the directional statistics of the fractures across the ExoMars landing site.
Study the directional statistics of the fractures across the ExoMars landing site.
Lin Yu.*
Zhao J.
Wang Le.
Huang Jun.
Zhang Liang.
et al.
Evaluation of Small-Sized Mounds Formation Mechanisms in China’s Zhurong Landing Region
[#1242]
In this study, we made a detailed investigation and discuss the origin of the small-sized mounds as well as pits occurring on them in the Zhurong landing area.
In this study, we made a detailed investigation and discuss the origin of the small-sized mounds as well as pits occurring on them in the Zhurong landing area.
Liu C. Q.*
Ling Z. C.
Liu P.
Shi E. B.
Xin Y. Q.
et al.
Chemical Compositions of Soils and Rocks Observed by Zhurong Rover in the First 300 Sols
[#1952]
This work focuses on the further analysis of chemical compositions of martian soils and rocks obtained by MarSCoDe of the Tianwen-1 mission.
This work focuses on the further analysis of chemical compositions of martian soils and rocks obtained by MarSCoDe of the Tianwen-1 mission.
Vitai Á.*
Topographic Analysis Based Identification of Flat Sediments in a Crater Near Rabe on Mars
[#1955]
Topographic analysis was used to determine whether sediment was present in the target crater. I did this using my own python code based on elevation data.
Topographic analysis was used to determine whether sediment was present in the target crater. I did this using my own python code based on elevation data.
Gupta S.*
Bell J. F.
Caravaca G.
Mangold N.
Stack K.
et al.
Fine-Scale Sedimentary Architecture of the Upper Part of the Jezero Western Delta Front
[#2953]
Sedimentology of the Jezero western delta shows evidence for progradation of a coarse-grained fan delta into a lake in Jezero crater.
Sedimentology of the Jezero western delta shows evidence for progradation of a coarse-grained fan delta into a lake in Jezero crater.
Golombek M.*
Williams N.
Cacan M.
Grip H.
Lemmon M.
et al.
Mars Helicopter, Ingenuity: Extended Mission Operations and Results
[#2453]
Ingenuity Extended mission flights, airfield selection, ripples, scouting, geologic mapping, dust lifting and flight software updates are described.
Ingenuity Extended mission flights, airfield selection, ripples, scouting, geologic mapping, dust lifting and flight software updates are described.
Beyssac O.*
Chide B.
Cousin A.
Ayoub F.
Bertrand T.
et al.
Coarse-Grained Olivine-Rich Regolith at Jezero Crater, Mars: Nature, Source and Transport
[#1727]
Using SuperCam, we constrain the mineralogy/physical properties of coarse grained regolith and discuss its source and transport.
Using SuperCam, we constrain the mineralogy/physical properties of coarse grained regolith and discuss its source and transport.
Anderson R. B.*
Gabriel T. S.
Forni O.
Manrique J. A.
Gasda P.
et al.
Trace and Minor Element Quantification with SuperCam Laser Induced Breakdown Spectroscopy (LIBS)
[#2182]
We present a summary of the current status of trace- and minor-element quantification with SuperCam LIBS.
We present a summary of the current status of trace- and minor-element quantification with SuperCam LIBS.
Beck P.*
Forni O.
Dehouck E.
Beyssac O.
Benzerara K.
et al.
Secondary Mineralogy of Jezero Delta Rocks from Hydrogen and Carbon Emission Lines in Supercam LIBS Data
[#1241]
Analysis of carbon and hydrogen signal in SuperCam data.
Analysis of carbon and hydrogen signal in SuperCam data.
Shi E. B.*
Liu C. Q.
Ling Z. C.
Hydration States of Ferric Sulfates Identified by Laser Induced Breakdown Spectroscopy
[#2059]
LIBS was used to identify the hydration states of ferric sulfates successfully in the laboratory, which will help to identify the ferric sulfates on Mars.
LIBS was used to identify the hydration states of ferric sulfates successfully in the laboratory, which will help to identify the ferric sulfates on Mars.
Lopez-Reyes G.*
Nachon M.
Veneranda M.
Beyssac O.
Madariaga J. M.
et al.
Anhydrite Detections by Raman Spectroscopy with Supercam at the Jezero Delta, Mars
[#1721]
The SuperCam Raman instrument onboard the Perseverance rover has performed several detections of anhydrite on white veins on the Jezero delta.
The SuperCam Raman instrument onboard the Perseverance rover has performed several detections of anhydrite on white veins on the Jezero delta.
Zalewska N.*
Czechowski L.
Borowska E.
X-Ray Measurements of Terrestrial Concretions as Analogues of Martian Concretions “Blueberries” from Meridiani Planum
[#2932]
We undertook the study of terrestrial analogues of martian concretions discovered by the Opportunity rover in the Meridiani Planum.
We undertook the study of terrestrial analogues of martian concretions discovered by the Opportunity rover in the Meridiani Planum.
Liu J.*
Michalski J.
Gale Crater as an Archive of Redox Processes at the Surface of Early Mars and Early Earth
[#1143]
Gale crater records the evolution of past climate and redox state of surface and atmosphere on early Mars and perhaps other rocky planets.
Gale crater records the evolution of past climate and redox state of surface and atmosphere on early Mars and perhaps other rocky planets.
Szczerba M.*
Rampe E. B.
Peretyazhko T. S.
Bristow T. F.
Morris R. V.
et al.
Hematite Formation and Growth in Gale Crater Seen Through MSL CheMin X-ray Diffraction Data
[#1956]
Hematite crystallites from Gale Crater are of equant shape from 3 to 40 nm, mostly smaller than terrestrial ones. Peak shapes suggest closed-system growth.
Hematite crystallites from Gale Crater are of equant shape from 3 to 40 nm, mostly smaller than terrestrial ones. Peak shapes suggest closed-system growth.
Koeppel A.*
Edwards C. S.
Edgar L. A.
Gullikson A.
Bennett K.
et al.
Surface Temperatures from Mars to Earth and Back: Developing New Interpretations of Thermal Inertia from Ground Truth Experiments
[#1378]
We compiled measurements from Mars and Earth to assess correlation of sediment thermal properties other remotely observable physical and compositional traits.
We compiled measurements from Mars and Earth to assess correlation of sediment thermal properties other remotely observable physical and compositional traits.
Menina S.*
Margerin L.
Kawamura T.
Drilleau M.
Garcia R.
et al.
Stratification of Attenuation Properties in the Crust of Mars from Full Seismogram Envelope Modeling of Near Impacts Detected by InSight
[#1557]
We propose to constrain the attenuation characteristics of heterogeneities in the martian crust from seismogram envelope modeling of near impacts.
We propose to constrain the attenuation characteristics of heterogeneities in the martian crust from seismogram envelope modeling of near impacts.
*presenter