#LPSC2023
#LPSC2023

Program with Links to Abstracts
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Poster Session: Not Headed Downhill Yet: Celebrating 10 Years of Curiosity at Gale Crater
Tuesday, March 14, 2023, 6:30 PM
Town Hall Exhibit Area
Swida O. B.*
Foing B. H.
Vleugels C. A.
Simulation of Mars Curiosity Computer Vision for Low Cost Autonomous Navigation System
[#2654]
Develop a low-cost autonomous navigational algorithm using the images captured by the instruments on Mars Curiosity that is applicable for future missions.
Develop a low-cost autonomous navigational algorithm using the images captured by the instruments on Mars Curiosity that is applicable for future missions.
Gambrill J. A.*
Martínez G. M.
Sebastián E.
Analyses of Thermal Noise in Curiosity's Ground Temperature Measurements
[#2568]
Identification of and analysis on noise present within ground temperature measurements by Curiosity’s REMS instrument.
Identification of and analysis on noise present within ground temperature measurements by Curiosity’s REMS instrument.
Henley T. L. J.*
Schmidt M. E.
Bray S. L.
Zheng J. J.
Marincic I. K.
et al.
Dust Coverages on Horizontal Rock Targets in Gale Crater: Influences of Seasonal Winds, Elevation, and Proximity to Active Dune Fields
[#1547]
Horizontal rock targets recorded throughout MSL have demonstrated how elevation, seasonal winds, and proximity to aeolian dune deposits affect surficial dust abundances.
Horizontal rock targets recorded throughout MSL have demonstrated how elevation, seasonal winds, and proximity to aeolian dune deposits affect surficial dust abundances.
Johnson J. R.*
Bell J. F.
Merusi M.
Joseph J.
Rice M.
et al.
Recent Spectrophotometric Observations Along the MSL and Mars2020 Rover Traverses
[#1387]
The MSL and Mars2020 rovers acquired new multispectral and stereo images at multiple times of sol to enable photometric studies of materials along the traverses.
The MSL and Mars2020 rovers acquired new multispectral and stereo images at multiple times of sol to enable photometric studies of materials along the traverses.
Manelski H. T.*
Sheppard R. Y.
Fraeman A. A.
Wiens R. C.
Johnson J. R.
et al.
Variability in Mt. Sharp Group Bedrock as Seen by ChemCam Passive and Active Spectra
[#1410]
Passive spectra taken by ChemCam in the Mt. Sharp group are examined using multivariate techniques and are compared to LIBS elemental data.
Passive spectra taken by ChemCam in the Mt. Sharp group are examined using multivariate techniques and are compared to LIBS elemental data.
Hoffman M. E.*
Newsom H. E.
Clegg S. M.
Gasda P. J.
Lanza N.
et al.
ChemCam Sulfur Abundances in the Knockfarril Hill Member, Gale Crater, Mars
[#2660]
Using ChemCam data and a multivariate sulfur calibration model developed by Clegg et al. to analyze chemistry from the Knockfarril Hill member of Gale crater.
Using ChemCam data and a multivariate sulfur calibration model developed by Clegg et al. to analyze chemistry from the Knockfarril Hill member of Gale crater.
VanBommel S. J.*
Berger J. A.
Gellert R.
O'Connell-Cooper C. D.
McCraig M. A.
et al.
Analysis of Sub-cm Chemical Endmembers with the Mars Science Laboratory Alpha Particle X-ray Spectrometer: A Demonstrated Improvement in Derived Elemental Stoichiometry
[#1214]
Improved analysis of APXS rasters betters constraints for mineral detections at the subcentimeter level within APXS data.
Improved analysis of APXS rasters betters constraints for mineral detections at the subcentimeter level within APXS data.
Litvak M. L.*
Mitrofanov I. G.
Gellert R.
Djachkova M. V.
Lisa D. I.
et al.
Depth Distribution of Chlorine at the Gale Crater According to DAN and APXS Measurements Onboard the Curiosity
[#1997]
Using Curiosity DAN and APXS data we examine depth distribution of Cl at Gale and revealed two components: surface Cl (concentration>1%) and shallow Cl (<1%).
Using Curiosity DAN and APXS data we examine depth distribution of Cl at Gale and revealed two components: surface Cl (concentration>1%) and shallow Cl (<1%).
Djachkova M. V.*
Nikiforov S. Y.
Mitrofanov I. G.
Litvak M. L.
Lisov D. I.
et al.
Water and Chlorine Abundances Within Distinct Geological Units in Gale Crater
[#2160]
We present the assessment of water equivalent hydrogen and absorption equivalent chlorine data gathered by the dynamic albedo of neutrons for MSL geologic units.
We present the assessment of water equivalent hydrogen and absorption equivalent chlorine data gathered by the dynamic albedo of neutrons for MSL geologic units.
Dibb S. D.*
Hardgrove C. J.
Correlation Between Average Local Relief and Passive Thermal Neutron Count Rates Measured by the Curiosity Rover Dynamic Albedo of Neutrons (DAN) Instrument
[#2427]
We discuss the correlation between thermal neutron count rates measured by Curiosity/DAN and variable topographic relief around the rover.
We discuss the correlation between thermal neutron count rates measured by Curiosity/DAN and variable topographic relief around the rover.
Berner A.*
Czarnecki S.
Hardgrove C.
Gasda P. J.
Mesick K.
Analyzing the Effect of High-Relief Topography on Active Neutron Measurements
[#2686]
We present our analysis of data taken by the DAN instrument onboard the Curiosity rover to understand the effect of topography on thermal neutron counts.
We present our analysis of data taken by the DAN instrument onboard the Curiosity rover to understand the effect of topography on thermal neutron counts.
Czarnecki S.*
Hardgrove C.
Rampe E. B.
Smith R. J.
Gasda P. J.
Constraining the Hydration of X-Ray Amorphous and Clay Mineral Phases in Gale Crater, Mars
[#2768]
Constraining hydrated phases in Gale crater with DAN water and CheMin mineralogy has implications for water/rock ratios and alteration redox, pH, and chemistry.
Constraining hydrated phases in Gale crater with DAN water and CheMin mineralogy has implications for water/rock ratios and alteration redox, pH, and chemistry.
Simpson S. L.*
Achilles C. A.
Rampe E. B.
Bristow T. F.
Blake D. F.
et al.
The Composition of X-Ray Amorphous Materials in Gale Crater, Mars
[#2781]
Here we discuss ongoing efforts to determine the composition and potential origins of the X-ray amorphous materials detected by the CheMin X-ray diffractometer.
Here we discuss ongoing efforts to determine the composition and potential origins of the X-ray amorphous materials detected by the CheMin X-ray diffractometer.
Valdueza J. E.*
Hausrath E. M.
Bristow T. F.
Rampe E. B.
Testing Destruction of Clay Minerals by Silica-Poor Brines in Gale Crater, Mars Using Laboratory and Field Experiments
[#2562]
This study examines the impacts of silica-poor brines on clay mineral alteration in laboratory dissolution experiments with future field experiments planned.
This study examines the impacts of silica-poor brines on clay mineral alteration in laboratory dissolution experiments with future field experiments planned.
Turner S. M. R.
Schwenzer S. P.*
Bridges J. C.
Sutter B.
Thorpe M. T.
et al.
The Role of Olivine in Fe-Carbonate Formation in Gale Crater, Mars
[#2337]
We investigate carbonate formation in Gale crater by using thermochemical modeling to explore the role of olivine and its preferential dissolution in Gale.
We investigate carbonate formation in Gale crater by using thermochemical modeling to explore the role of olivine and its preferential dissolution in Gale.
Haber J. T.*
Horgan B.
Potter-McIntyre S.
Broz A.
Smith R.
Evidence of Increased Surface Exposure and Diagenetic Alteration in Evaporitic Environments on Earth and Mars
[#2577]
Near-shore or deep-lake / How can we tell the difference? / Earth rocks can help us.
Near-shore or deep-lake / How can we tell the difference? / Earth rocks can help us.
*presenter