Nanoscale\nAnalyses of X‑ray Amorphous Material\nfrom Terrestrial Ultramafic Soils Record Signatures of Environmental\nConditions Useful for Interpreting Past Martian Conditions

The secondary mineral assemblage of martian rocks and\nsediments\nis critical to the interpretation of past conditions on Mars. X-ray\namorphous material that is variably Mg/Fe/Si-rich and Al-poor, and\nthat likely contains secondary alteration products, makes up between\n15 and 73 wt % of Gale crater materials measured by the CheMin instrument\nand is also prevalent on the martian surface in other locations. Despite\nits prevalence, the structure and origin of this material and its\nimplications for past martian environments remains unknown. Here,\nwe employ transmission electron microscopy and synchrotron microprobe\nanalyses of Fe/Si/Mg-rich and Al-poor ultramafic soils from the mediterranean\nclimate Klamath Mountains of California and subarctic climate Tablelands\nof Newfoundland, Canada to help interpret environmental conditions\nduring the formation of chemically similar X-ray amorphous material\nin Gale crater, Mars. X-ray amorphous material includes globular amorphous\nsilica and chemically heterogeneous nanospherical amorphous material\nand nanocrystalline phases. Amorphous silica is present only in soils\nthat undergo extensive periods of cyclic freezing conditions. X-ray\namorphous material from the subarctic Tablelands is significantly\nricher in Mg and Si than material from the warmer Klamath Mountains.\nNanocrystallites in both examined soils are richer in Fe than the\ntruly amorphous material. However, Fe-rich nanocrystallites contain\nsignificantly more Mg and Si in the subarctic Tablelands, whereas\nKlamath Mountains soils contain highly Fe-enriched nanocrystallites\nincorporating little Mg and Si and potentially contain nanocrystalline\nsmectites. These characteristics provide helpful identifiers to interpret\npast environmental conditions during the formation of X-ray amorphous\nmaterial both in situ and in returned samples from Mars.

Publication Details

Journal
Figshare
Published
2024-12-05
DOI
https://doi.org/10.1021/acsearthspacechem.4c00158.s001
Primary Topic
Mycorrhizal Fungi and Plant Interactions
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Nanoscale\nAnalyses of X‑ray Amorphous Material\nfrom Terrestrial Ultramafic Soils Record Signatures of Environmental\nConditions Useful for Interpreting Past Martian Conditions

Figshare
Mycorrhizal Fungi and Plant Interactions
article

Nanoscale\nAnalyses of X‑ray Amorphous Material\nfrom Terrestrial Ultramafic Soils Record Signatures of Environmental\nConditions Useful for Interpreting Past Martian Conditions

article en

Abstract

The secondary mineral assemblage of martian rocks and\nsediments\nis critical to the interpretation of past conditions on Mars. X-ray\namorphous material that is variably Mg/Fe/Si-rich and Al-poor, and\nthat likely contains secondary alteration products, makes up between\n15 and 73 wt % of Gale crater materials measured by the CheMin instrument\nand is also prevalent on the martian surface in other locations. Despite\nits prevalence, the structure and origin of this material and its\nimplications for past martian environments remains unknown. Here,\nwe employ transmission electron microscopy and synchrotron microprobe\nanalyses of Fe/Si/Mg-rich and Al-poor ultramafic soils from the mediterranean\nclimate Klamath Mountains of California and subarctic climate Tablelands\nof Newfoundland, Canada to help interpret environmental conditions\nduring the formation of chemically similar X-ray amorphous material\nin Gale crater, Mars. X-ray amorphous material includes globular amorphous\nsilica and chemically heterogeneous nanospherical amorphous material\nand nanocrystalline phases. Amorphous silica is present only in soils\nthat undergo extensive periods of cyclic freezing conditions. X-ray\namorphous material from the subarctic Tablelands is significantly\nricher in Mg and Si than material from the warmer Klamath Mountains.\nNanocrystallites in both examined soils are richer in Fe than the\ntruly amorphous material. However, Fe-rich nanocrystallites contain\nsignificantly more Mg and Si in the subarctic Tablelands, whereas\nKlamath Mountains soils contain highly Fe-enriched nanocrystallites\nincorporating little Mg and Si and potentially contain nanocrystalline\nsmectites. These characteristics provide helpful identifiers to interpret\npast environmental conditions during the formation of X-ray amorphous\nmaterial both in situ and in returned samples from Mars.

Figshare
Openalex Percentile: Top 57%
Mycorrhizal Fungi and Plant Interactions
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.