MétaCan
Menu
Back to cohort
Record W2010844585 · doi:10.2113/gssgfbull.178.6.427

The northern ice cap of Mars: an enigmatic evolution compared to the polar environment on Earth

2007· article· en· W2010844585 on OpenAlexaff
Pierre Rognon, Robert Desjardins, Gilles Dawidowicz

Bibliographic record

VenueBulletin de la Société Géologique de France · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsUniversité du Québec à Montréal
FundersNational Aeronautics and Space Administration
KeywordsGeologyMars Exploration ProgramGlacial periodMartianIce streamIce divideIce sheetGeomorphologyFault scarpPolarAntarctic sea iceAstrobiologyGeophysicsPaleontologyCryosphereSea iceOceanography

Abstract

fetched live from OpenAlex

Abstract Would it be possible to interpret the dynamics of the northern polar ice cap of Mars with the same criteria as for terrestrial ice sheets? The aim of this paper is to illustrate the problems posed by such an approach. We present a detailed study of the MOC narrow angle image E01-01773, taken at 83.5°N/241.4°W in the upper part of a 300 km-long depression situated at the edge of the northern polar ice cap. On Mars, every depression resembling a valley is a “chasma”, and as this one has no official name, we suggest to call it “West Olympia Chasma” (WOC). By analyzing the satellite image, we have been able to highlight some unusual features of martian glacial geomorphology and to compare them with topographies and sediments known in terrestrial glacial environments. In particular: – the scarp cutting the edge of the ice cap above the chasma is formed of thin alternations of ice and aerosols and is bordered by numerous small and dissymetrical ridges that run parallel to it. On Earth, these ridges would be interpreted as a succession of terminal moraines; in fact, they consist of gravitational debris accumulated under the nearly motionless ice cliff; – at the edge of the ice, where signs of melt water action would be clearly visible in terrestrial environments, there is practically no evidence of such a process on Mars. However, two intriguing channels, several tens of meters wide and about 1 km-long, suggest the occurrence of temporary water flow; – these channels originate at the base of an ice tongue that appears to have flowed recently over the scarp towards the floor of the chasma, in the same manner as surging glaciers on Earth, whereas Mars ice seems motionless; – the sandy sediments covered by the ice cap do not seem to be ground moraines, as would be the case on Earth, but eolian sand brought by winds when the ice cap did not exist. At present, the most effective erosion agents are the winds channelled into the chasma and the alternations of condensation/sublimation. Their combined action explains the dissymetry between both sides of the chasma. The winds are enhanced by local topography and contribute to the movement of dunes towards the outlet of the chasma.

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)0.001
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 score0.452
Threshold uncertainty score0.263

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
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 head0.006
GPT teacher head0.227
Teacher spread0.220 · 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

Citations1
Published2007
Admission routes1
Has abstractyes

Explore more

Same venueBulletin de la Société Géologique de FranceSame topicPlanetary Science and ExplorationFrench-language works237,207