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Record W3184973091 · doi:10.1126/science.abf8966

Thickness and structure of the martian crust from InSight seismic data

2021· article· en· W3184973091 on OpenAlexafffund
Brigitte Knapmeyer‐Endrun, M. P. Panning, Felix Bissig, Rakshit Joshi, Amir Khan, Doyeon Kim, V. Lekić, Benoît Tauzin, Saikiran Tharimena, Matthieu Plasman, Nicolas Compaire, R. García, Ludovic Margerin, Martín Schimmel, É. Stutzmann, N. C. Schmerr, E. Bozdağ, Ana‐Catalina Plesa, M. A. Wieczorek, Adrien Broquet, Daniele Antonangeli, S. M. McLennan, Henri Samuel, Chloé Michaut, Lu Pan, S. E. Smrekar, C. L. Johnson, Nienke Brinkman, Anna Mittelholz, Attilio Rivoldini, Paul M. Davis, Philippe Lognonné, Baptiste Pinot, John‐Robert Scholz, Simon C. Stähler, Martin Knapmeyer, Martin van Driel, Domenico Giardini, W. B. Banerdt

Bibliographic record

VenueScience · 2021
Typearticle
Languageen
FieldEarth and Planetary Sciences
TopicHigh-pressure geophysics and materials
Canadian institutionsUniversity of British Columbia
FundersCanadian Space AgencyInstitut Universitaire de FranceCentre National de la Recherche ScientifiqueInstitut de Physique du Globe de ParisMax-Planck-GesellschaftNuclear Safety and Security CommissionEidgenössische Technische Hochschule ZürichH2020 Marie Skłodowska-Curie ActionsSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungDeutsches Zentrum für Luft- und RaumfahrtJet Propulsion LaboratoryCentre National d’Etudes SpatialesBundesministerium für Bildung und ForschungNational Aeronautics and Space AdministrationBranco Weiss Fellowship – Society in ScienceCalifornia Institute of TechnologyEuropean CommissionAgence Nationale de la RechercheBelgian Federal Science Policy OfficeNational Science FoundationEuropean Space AgencyStaatssekretariat für Bildung, Forschung und InnovationDavid and Lucile Packard FoundationUK Space Agency
KeywordsMartianCrustGeologyAstrobiologyGeophysicsEarth scienceMars Exploration ProgramSeismologyPhysics

Abstract

fetched live from OpenAlex

A planet's crust bears witness to the history of planetary formation and evolution, but for Mars, no absolute measurement of crustal thickness has been available. Here, we determine the structure of the crust beneath the InSight landing site on Mars using both marsquake recordings and the ambient wavefield. By analyzing seismic phases that are reflected and converted at subsurface interfaces, we find that the observations are consistent with models with at least two and possibly three interfaces. If the second interface is the boundary of the crust, the thickness is 20 ± 5 kilometers, whereas if the third interface is the boundary, the thickness is 39 ± 8 kilometers. Global maps of gravity and topography allow extrapolation of this point measurement to the whole planet, showing that the average thickness of the martian crust lies between 24 and 72 kilometers. Independent bulk composition and geodynamic constraints show that the thicker model is consistent with the abundances of crustal heat-producing elements observed for the shallow surface, whereas the thinner model requires greater concentration at depth.

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)0.001
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 score0.009
Threshold uncertainty score0.017

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
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 head0.015
GPT teacher head0.212
Teacher spread0.197 · 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

Citations271
Published2021
Admission routes2
Has abstractyes

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