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Record W4408422897 · doi:10.5194/egusphere-egu25-2878

The heat flux through the cores of small terrestrial planetary bodies from electrical resistivity measurements of liquid Fe-S-Si at high pressures

2025· preprint· en· W4408422897 on OpenAlexaff
Erin Lenhart, Wenjun Yong, Richard A. Secco

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldEarth and Planetary Sciences
TopicHigh-pressure geophysics and materials
Canadian institutionsWestern University
Fundersnot available
KeywordsElectrical resistivity and conductivityFlux (metallurgy)High heatMaterials scienceHeat fluxAstrobiologyGeologyGeophysicsPhysicsMechanicsHeat transferComposite materialMetallurgy

Abstract

fetched live from OpenAlex

Dynamo action in liquid Fe planetary cores varies according to alloyed light elements such as S and Si. This study experimentally constrains the thermal conductivity of Fe-S-Si alloys at planetary core conditions, which may be used in combination with thermal evolution models to find the total thermal convective force in the core. A sample of Fe alloy with 16wt%S and 2wt%Si was chosen as a predicted composition of the core of Asteroid 4 Vesta, based on studies of HED meteorites [1-2]. This is near the miscibility limit of S and Si in liquid Fe [3].Experiments were performed at 2-5 GPa in a 1000-ton cubic anvil press and at up to 9 GPa in a 3000-ton multi-anvil press. Temperatures as high as 2100 K into the melt of Fe-S-Si. The electrical resistivity of the liquid Fe-S-Si alloy was measured in situ; to find the electronic component of the thermal conductivity, the Wiedemann-Franz Law was used. To confirm the sample composition and homogenization, electron microprobe analysis was performed on samples recovered from various stages of melting, yielding compositional maps of Fe, S, and Si across each sample.The individual effects of S and Si on the electrical resistivity of liquid Fe are seen in the results for the conditions of small planetary cores. Fe-16wt%S-2wt%Si has an electrical resistivity of 300-450 µΩ·cm at the complete melt in the pressure range of 2-7 GPa. Pure Fe at the same pressures is at most half this value [4], meaning that a moderate amount of S greatly decreases thermal conductivity in the liquid core. These results may be used to find the adiabatic heat flux at the top of the core of a given planetary body, with direct application to the formation of a magnetic dynamo in the liquid cores of objects such as Vesta, Ganymede, and Mars.References:[1] Steenstra, E.S., Dankers, D., Berndt, J., Klemme, S., Matveev, S., van Westrenen, W., 2019. Icarus, v. 317, p. 669-681.[2] Pringle, E.A., Savage, P.S., Badro, J., Barrat, J.-A., Moynier, F., 2013. Earth Planet. Sci. Lett., v. 373, p. 75-82.[3] Chabot, N.L., Wollack, E.A., Klima, R.L., Minitti, M.E., 2014. Earth Planet. Sci. Lett., v. 390, p. 199-208.[4] Yong, W., Secco, R.A., Littleton, J.A.H., Silber, R.E., 2019. Geophys. Res. Lett., v. 46, p. 11065-11070.

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: Bench or experimental · Consensus signal: Bench or experimental
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.001
Threshold uncertainty score0.003

Distilled classifier scores by category (both heads)

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)0.0010.000

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 head0.041
GPT teacher head0.239
Teacher spread0.199 · 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 designBench or experimental
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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