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Record W1862302739 · doi:10.1029/2012je004151

Mineralogy and morphology of geologic units at Libya Montes, Mars: Ancient aqueously derived outcrops, mafic flows, fluvial features, and impacts

2012· article· en· W1862302739 on OpenAlexaff
J. L. Bishop, Daniela Tirsch, L. L. Tornabene, R. Jaumann, A. S. McEwen, Patrick McGuire, Anouck Ody, F. Poulet, R. N. Clark, M. Parente, N. K. McKeown, John F. Mustard, S. L. Murchie, J. R. C. Voigt, Z. Ogretmen Aydin, Marlene Bamberg, A. Petau, Gregory Michael, F. P. Seelos, C. Hash, Gregg A. Swayze, G. Neukum

Bibliographic record

VenueJournal of Geophysical Research Planets · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsMacEwan UniversityWestern University
FundersNational Aeronautics and Space Administration
KeywordsMaficGeologyNoachianOutcropClay mineralsGeochemistryCarbonateMineralMars Exploration ProgramOlivinePyroxeneMineralogyMartianChemistryAstrobiology

Abstract

fetched live from OpenAlex

Abstract There is ample evidence of both ancient and long‐lasting fluvial activity and chemical alteration in the Libya Montes region south of Isidis Basin. The region hosts Noachian to Amazonian aged surface rocks with extensive outcrops of olivine‐ and pyroxene‐bearing material. Libya Montes also features surface outcrops and/or deposits hosting Fe/Mg‐smectite, Fe/Mg‐smectite mixed with carbonate and/or other Fe/Mg‐rich phyllosilicates, and Al‐smectite. These units likely formed through chemical alteration connected with hydrothermal activity resulting from the formation of the Isidis Basin and/or the pervasive fluvial activity throughout this region. The morphology and stratigraphy of the aqueous and mafic minerals are described using High Resolution Imaging Science Experiment and High Resolution Stereo Camera derived digital terrain models. Analyses of the Compact Reconnaissance Imaging Spectrometer for Mars spectra show variations in the chemistry of the Fe/Mg‐smectite from nontronite‐like exposures with spectral features near 2.29 and 2.4 µm more consistent with Fe 3+ 2 OH groups in the mineral structure, and saponite‐like outcrops with spectral features near 2.31 and 2.38 µm characteristic of Mg 2+ 3 OH groups. These Fe/Mg‐smectite bearing materials also have bands near 1.9 µm due to H 2 O and near 2.5 µm that could be due to the smectite, other phyllosilicates, and carbonates. All regions exhibiting carbonate features near 3.4–3.5 µm also have features consistent with the presence of olivine and Fe/Mg‐smectite, indicating that the carbonate signatures occur in rocks likely containing a mixture of these minerals. The Al‐smectite‐bearing rocks have bands near 1.41, 1.91, and 2.19 µm that are more consistent with beidellite than other Al‐phyllosilicates, indicating a higher‐temperature or diagenetically processed origin for this material. Our interpretation of the geologic history of this region is that ancient Noachian basaltic crustal materials experienced extensive aqueous alteration at the time of the Isidis impact, during which the montes were also formed, followed by emplacement of a rough olivine‐rich lava or melt, and finally the smooth pyroxene‐bearing caprock unit.

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 machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.019
Threshold uncertainty score0.037

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.000

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 head0.044
GPT teacher head0.299
Teacher spread0.255 · 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 source (direct Gemma or distilled Codex), 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

Citations73
Published2012
Admission routes1
Has abstractyes

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