MétaCan
Menu
Back to cohort
Record W4407225867 · doi:10.1029/2023je008046

Collection and In Situ Analyses of Regolith Samples by the Mars 2020 Rover: Implications for Their Formation and Alteration History

2025· article· en· W4407225867 on OpenAlexafffund
Elisabeth M. Hausrath, R. Sullivan, Y. S. Goreva, María‐Paz Zorzano, Alicia Vaughan, A. Cousin, Sandra Siljeström, Sunanda Sharma, Andrew O. Shumway, T. V. Kizovski, S. J. VanBommel, Michael M. Tice, Abigail L. Knight, Germán Martínez, Á. Vicente‐Retortillo, Lucia Mandon, C. T. Adcock, Juan Manuel Madariaga, Iratxe Población, J. R. Johnson, J. Lasue, O. Gasnault, Nicolas Randazzo, Emily Cardarelli, R. E. Kronyak, Andreas Bechtold, Gerhard Paar, Arya Udry, O. Forni, C. C. Bedford, Nancy Carman, J. F. Bell, Kathleen C. Benison, Tanja Bosak, A. J. Brown, Adrian Broz, F. J. Calef, B. C. Clark, E. A. Cloutis, Andrew D. Czaja, Teresa Fornaro, Thierry Fouchet, M. P. Golombek, Felipe Gómez, C. D. K. Herd, K. E. Herkenhoff, Ryan S. Jakubek, Louise Jandura, Jesús Martínez‐Frías, L. E. Mayhew, Pierre‐Yves Meslin, Claire Newman, Jorge I. Núñez, F. Poulet, Clément Royer, Patrick Russell, Mark A. Sephton, Shiv K. Sharma, David L. Shuster, Justin I. Simon, Iona Tirona, R. C. Wiens, B. P. Weiss, Amy J. Williams, Kenneth H. Williford, Z. U. Wolf

Bibliographic record

VenueJournal of Geophysical Research Planets · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversity of WinnipegUniversity of AlbertaBrock University
FundersCanadian Space AgencySwedish National Space Agency
KeywordsRegolithAstrobiologyMars Exploration ProgramMartianImpact craterContext (archaeology)Martian surfaceEarth scienceGeologyPlanetary surfaceEnvironmental scienceMineralogyPhysicsPaleontology

Abstract

fetched live from OpenAlex

Abstract The Perseverance rover has sampled mm‐size lithic fragments containing olivine likely from at least two source regions from the surface of an inactive megaripple surface, and fine‐grained material from the surface and to a depth of ∼4–6 cm. Some of the mm‐size grains lack a coherent diffraction pattern measured by PIXL, consistent with the presence of poorly ordered secondary phases that have been altered. Analysis of these materials on Earth will allow examination of materials that have experienced aqueous, potentially habitable environments that could contain biosignatures. Fluorescence of three different patterns was detected, consistent with inorganic emissions from silica defects or rare earth elements in certain mineral phases, although organic origin cannot be excluded. Analysis of Autofocus Context Imager and Wide Angle Topographic Sensor for Operations and eNgineering images of the subsurface material and MEDA thermal inertia measurements indicate average grain sizes of ∼125 and ∼150 μm, respectively, for the bulk material within the megaripple. The fine‐grained material in the sampling location indicates chemical compositions similar to previously proposed global components as well as airfall dust. In situ and associated atmospheric measurements provide evidence of recent processes likely including water vapor in soil crust formation. The sampled material will therefore help elucidate the formation of Martian soils; current surface‐atmosphere interactions; the composition, shape, and size distribution of dust grains valuable for studies of past and present Martian climate and for assessing potential health and other risks to human missions; and ancient, aqueously altered environments that could have been habitable, and, if Mars contained life, possibly contain biosignatures.

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)0.000
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 score0.767
Threshold uncertainty score0.124

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
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 head0.080
GPT teacher head0.359
Teacher spread0.278 · 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

Citations4
Published2025
Admission routes2
Has abstractyes

Explore more

Same venueJournal of Geophysical Research PlanetsSame topicPlanetary Science and ExplorationFrench-language works237,207