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Record W4408484255 · doi:10.5194/egusphere-egu25-20468

Hydrated silica in Oxia Planum, Mars

2025· preprint· en· W4408484255 on OpenAlexaff
Joseph D. McNeil, Peter Grindrod, L. L. Tornabene, Peter Fawdon

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsWestern University
Fundersnot available
KeywordsPlanum temporaleMars Exploration ProgramAstrobiologyChemistryPsychologyNeurosciencePhysics

Abstract

fetched live from OpenAlex

Oxia Planum, Mars, is the future landing site of ESA’s ExoMars Rosalind Franklin rover (EMRF, launching 2028), which will search for physical and chemical biosignatures at the surface and subsurface using its analytical suite of instruments, the ‘Pasteur’ payload [1]. Oxia Planum contains detections of deposits containing hydrated silica (SiO2·nH2O; opal [2]). Hydrated silica is important in understanding aqueous processes and habitability on Mars owing to its numerous formation pathways which invariably require liquid water, and its excellent preservation potential for physical and chemical biosignatures that may be present. CRISM data indicate the presence of opal-bearing material (hydrated silica unit; HSU) in two main physiogeographic locations within Oxia Planum. Firstly, HSU is present in a thin (~5 m), bright-toned, blueish-white unit positioned stratigraphically below the sedimentary fan, and above the phyllosilicate-bearing plains. The fan body also contains exposures of meter-scale, laterally-discontinuous outcrops of bright-toned, similarly-colored strata. CaSSIS CBRCs indicate that these outcrops are identical in color to the CRISM detections of HSU in the larger, exposed outcrops. This, as well as their similar relationship to the fan, indicates that they are likely to also be HSU. Outcrops of HSU are also present infilling topographic lows south of the sedimentary fan, at the margins of Pelso Chasma. The position of the 1.4 µm and 2.2 µm BDR values from targeted CRISM cubes indicate that the HSU in Oxia Planum is predominantly amorphous (Opal-A); ten out of fourteen spectra plot within the Opal-A field, three plot within the crystalline opal (Opal-CT) field, and one plots in the overlap region. The mean crystallinity of opal in Oxia Planum is similar to the mean crystallinity of opal in fans elsewhere on Mars. CRC values for the 1.4- and 1.9- micron features both indicate that opal in the HSU is predominantly weathering-derived, instead of hydrothermally-derived. Aqueous alteration of hydrated silica under martian conditions can alter its crystallinity through dissolution and reprecipitation by circulating fluid, over time converting relatively more amorphous opal (Opal-A) into relatively more crystalline opal (Opal-CT; [3]). The observation of Opal-A at Oxia Planum, situated directly above clay-bearing plains that underwent aqueous alteration [4], implies an unconformity exists between the alteration of the clay-rich plains and the deposition of the overlying hydrated silica-bearing unit, and therefore also between the plains and the sedimentary fan. References: [1] Vago et al. (2017) Astrobio. 17, 471-510; [2] Quantin-Nataf et al. (2021) Astrobio. 21, 345-366; [3] Sun & Milliken (2018) GRL. 45, 10,221-10,228; [4] Mandon et al. (2021) Astrobio. 21, 464-48

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 score0.063
Threshold uncertainty score0.124

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0000.000
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 head0.014
GPT teacher head0.241
Teacher spread0.228 · 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".

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Citations0
Published2025
Admission routes1
Has abstractyes

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