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Record W109370866

Study of Metal Extracted from Tzarev L5 Chondrite by Mössbauer Spectroscopy and Metalography

2006· article· en· W109370866 on OpenAlexaboutno aff
E. V. Zhiganova, М. И. Оштрах

Bibliographic record

VenueMeteoritics and Planetary Science Supplement · 2006
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstro and Planetary Science
Canadian institutionsnot available
Fundersnot available
KeywordsKamaciteTroiliteChondriteMössbauer spectroscopyAnalytical Chemistry (journal)Ordinary chondriteChemistryMetalMaterials scienceMeteoriteCrystallographyMetallurgyPhysics
DOInot available

Abstract

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Introduction: Mossbauer spectra of ordinary chondrites consist of several components related to metal, troilite, olivine, pyroxene, and iron oxides. The area of metal subspectra does not exceed 20% and this value is related to the metal iron content. Usually chondrite metal contains more than one metal phase, but they cannot be resolved in complicated Mossbauer spectrum of chondrite sample [1, 2]. Therefore, metal extraction from meteorite matter is necessary for detailed study by Mossbauer spectroscopy. Methods: A sample of metal extracted from ordinary chondrite Tzarev L5 was prepared as powder and glued on pure aluminum foil. Extraction was performed by several steps: powdering, levigation in acetone followed by the separation in strong and weak magnetic fields, then drying and etching by weak HF, and final selection with binocular loupe from silicates. Mossbauer spectrum was measured at room temperature using spectrometer SM-2201 with high accuracy, stability, and sensitivity in transmission geometry with moving absorber. Sections of Tzarev L5 for metallography were polished with diamond paste and etched by Nital (2 vol% HNO3, balance ethyl alcohol). Chemical composition of metal was obtained by microanalysis EDAX realized on SEM. Results: Mossbauer spectrum of metal from Tsarev L5 was measured with high velocity resolution using 4096 channels and than presented in 1024 channels for fitting. The results of the spectrum better fit demonstrated the presence of three sextets with the hyperfine field values related to kamacite α-Fe(Ni,Co), martensite α2-Fe(Ni,Co) and kamacite α′-Fe(Ni,Co), one doublet related to residue olivine, and one singlet related to taenite γFe(Ni,Co). The result of the metal grains metallography demonstrates the presence of various metal phases: α-Fe(Ni,Co), α2-Fe(Ni,Co), and both α′Fe(Ni,Co) and γ-Fe(Ni,Co) in plessite. Conclusions: Study of extracted metal from Tzarev L5 by Mossbauer spectroscopy permitted us to reveal four different metal phases and determine its hyperfine parameters and relative areas. These results were in good agreement with metallography data. References: [1] E. V. Zhiganova et al. 2005. Meteoritics & Planetary Science 40:A174. [2] E. V. Zhiganova et al. Hyperfine Interactions. Forthcoming. 5144 Si AND C ISOTOPIC RATIOS IN AGB STARS: SiC GRAIN DATA, MODELS, AND THE GALACTIC EVOLUTION OF THE Si ISOTOPES E. Zinner1, L. R. Nittler2, R. Gallino3, 7, A. I. Karakas4, M. Lugaro5, O. Straniero6, and J. C. Lattanzio7. 1Washington University, Saint Louis, Missouri 63130, USA. E-mail: ekz@wustl.edu. 2Carnegie Institution of Washington, NW Washington, D.C. 20015, USA. 3Universita di Torino, Italy. 4McMaster University, Hamilton, Ontario, L8S 4M1, Canada. 5University of Utrecht, 3508 TA Utrecht, The Netherlands. 6INAF, Osservatorio Astronomico di Teramo, Italy. 7Monash University, Victoria 3800, Australia

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 score0.043
Threshold uncertainty score0.997

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)0.0010.000

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 head0.005
GPT teacher head0.215
Teacher spread0.210 · 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".

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Citations0
Published2006
Admission routes1
Has abstractyes

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