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Record W4414651605 · doi:10.1016/j.icarus.2025.116832

Distal impact-related surface flows associated with the well-preserved Tokmok Crater, Noachis Terra, Mars

2025· article· en· W4414651605 on OpenAlexafffund
J. Burley, L. L. Tornabene, G. R. Osinski

Bibliographic record

VenueIcarus · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsWestern University
FundersMedical Organization for Latino AdvancementNatural Sciences and Engineering Research Council of CanadaCanadian Space AgencyU.S. Geological SurveyUniversité de Lyon
KeywordsEjectaImpact craterMars Exploration ProgramMartianTerrainAmazonianMeteoriteAngle of repose

Abstract

fetched live from OpenAlex

Meteorite impact craters on Mars display a diverse range of ejecta morphologies. A number of studies have suggested the presence of impact ejecta deposits beyond the limit of the canonical proximal continuous ejecta blanket, which on Mars is often marked by a topographic high, or “rampart”. It is currently uncertain how such deposits beyond the rampart form, and under what conditions. With the goal of answering such questions, we identified and characterized extensive surface flow deposits beyond the proximal ejecta blanket of Tokmok Crater, a ~ 9 km-diameter well-preserved crater in central Noachis Terra (29.405°S 351.319°E). We refer to these as Distal Flow Deposits (DFDs). We recognize two types: Type 1 flows develop at the base of source crater facing slopes as fan-like accumulations of smooth surfaced material. Type 2 flows form channel-fill like deposits within confining topography that funnel material from flat-lying regions. Through the identification, morphological mapping, and morphometric analysis of various impact units, the DFDs studied here are interpreted to represent the emplacement of outwardly mobilized ground-hugging flows subject to some form of impact-induced fluidization. DFD slope values are consistently below the dynamic angle of repose (Type 1 average = 6°; Type 2 average = 8.4°). DFDs are shown to accumulate where existing target topography captures more extended ejecta than surrounding flat-lying terrains that are resurfaced or obscured by the same deposits. Such deposits are shown to exist well beyond the proximal continuous ejecta blanket, which has important implications for geomorphological studies across Mars.

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: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.100
Threshold uncertainty score0.438

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 head0.007
GPT teacher head0.222
Teacher spread0.215 · 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

Citations0
Published2025
Admission routes2
Has abstractyes

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