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Record W4321442870 · doi:10.1029/2022je007433

An Examination of Soil Crusts on the Floor of Jezero Crater, Mars

2023· article· en· W4321442870 on OpenAlexaff
Elisabeth M. Hausrath, C. T. Adcock, Andreas Bechtold, P. Beck, Kathleen C. Benison, A. J. Brown, Emily Cardarelli, Nancy Carman, Baptiste Chide, John R. Christian, B. C. Clark, E. A. Cloutis, A. Cousin, O. Forni, T. S. J. Gabriel, O. Gasnault, M. P. Golombek, Felipe Gómez, M. H. Hecht, T. L. J. Henley, Jennifer Huidobro, J. R. Johnson, Michael W. Jones, P. B. Kelemen, Abigail L. Knight, J. Lasue, Stéphane Le Mouëlic, Juan Manuel Madariaga, J. N. Maki, Lucia Mandon, Germán Martínez, Jesús Martínez‐Frías, T. H. McConnochie, Pierre‐Yves Meslin, María‐Paz Zorzano, H. E. Newsom, Gerhard Paar, Nicolas Randazzo, Clément Royer, Sandra Siljeström, M. E. Schmidt, Susanne Schröder, Mark A. Sephton, R. Sullivan, Nathalie Turenne, Arya Udry, S. J. VanBommel, Alicia Vaughan, R. C. Wiens, N. R. Williams

Bibliographic record

VenueJournal of Geophysical Research Planets · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversity of AlbertaBrock UniversityUniversity of Winnipeg
FundersDeutsches Zentrum für Luft- und RaumfahrtSwedish National Space AgencyNuclear Safety and Security CommissionUK Space AgencyArizona State UniversityNational Aeronautics and Space Administration
KeywordsImpact craterMars Exploration ProgramAstrobiologySoil waterGeologyMartianFrost (temperature)MineralogyGeomorphologySoil science

Abstract

fetched live from OpenAlex

Abstract Martian soils are critically important for understanding the history of Mars, past potentially habitable environments, returned samples, and future human exploration. This study examines soil crusts on the floor of Jezero crater encountered during initial phases of the Mars 2020 mission. Soil surface crusts have been observed on Mars at other locations, starting with the two Viking Lander missions. Rover observations show that soil crusts are also common across the floor of Jezero crater, revealed in 45 of 101 locations where rover wheels disturbed the soil surface, two out of seven helicopter flights that crossed the wheel tracks, and four of eight abrasion/drilling sites. Most soils measured by the SuperCam laser‐induced breakdown spectroscopy (LIBS) instrument show high hydrogen content at the surface, and fine‐grained soils also show a visible/near infrared (VISIR) 1.9 μm H 2 O absorption feature. The Planetary Instrument for X‐ray Lithochemistry (PIXL) and SuperCam observations suggest the presence of salts at the surface of rocks and soils. The correlation of S and Cl contents with H contents in SuperCam LIBS measurements suggests that the salts present are likely hydrated. On the “Naltsos” target, magnesium and sulfur are correlated in PIXL measurements, and Mg is tightly correlated with H at the SuperCam points, suggesting hydrated Mg‐sulfates. Mars Environmental Dynamics Analyzer (MEDA) observations indicate possible frost events and potential changes in the hydration of Mg‐sulfate salts. Jezero crater soil crusts may therefore form by salts that are hydrated by changes in relative humidity and frost events, cementing the soil surface together.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.002
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.874
Threshold uncertainty score0.305

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0020.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.074
GPT teacher head0.345
Teacher spread0.271 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations20
Published2023
Admission routes1
Has abstractyes

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