lnu.sePublications
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Insights Into Carbonaceous Matter in ∼3.5 Ga Hydrothermal Barites from the Dresser Formation (Pilbara Craton, Australia)
University of Göttingen, Germany.
Linnaeus University, Faculty of Health and Life Sciences, Department of Biology and Environmental Science. University of Göttingen, Germany.
University of Göttingen, Germany.
University of Cologne, Germany.
Show others and affiliations
2023 (English)In: IMOG 2023 / [ed] European Association of Geoscientists & Engineers, 2023, Vol. 2023Conference paper, Oral presentation with published abstract (Refereed)
Abstract [en]

The emergence of life on the juvenile Earth is still poorly understood and remains one of the major questions in geobiological research. Some of our planet´s most ancient rocks contain carbonaceous matter (CM) that may represent a valuable archive to trace earliest life.

However, it is often difficult to prove the origin and syngeneity of such CM. Here we report on CM preserved in ∼3.5 Ga old barites from the Dresser Formation (Pilbara Carton, Western Australia). On outcrop scale, spatial associations between bedded and vein-hosted barites suggest that the bedded barite may have formed from hydrothermal fluids discharging into subaquatic caldera environments [1]. Bedded barites associated with stromatolites contain abundant CM (total organic carbon = 0.3 wt% [2]) whose nature has been investigated further. Three populations of CM were recognized by means of light microscopy and high-resolution Raman mapping: (i) CM flakes at the edges of single growth bands of barite crystals, (ii) CM dispersed within barite crystals, and (iii) CM in 50–300 µm wide secondary quartz veins that cross-cut barite crystals. Raman spectra of the CM indicate peak metamorphic temperatures of approximately 300 ± 50 °C, corresponding to lower greenschist-facies conditions which are consistent with the metamorphic overprint by granitic intrusions in the area ∼3.3 Ga ago [3]. Near edge X-ray absorption fine structure (NEXAFS) and solid-state nuclear magnetic resonance (NMR) measurements revealed a highly aromatic nature of the CM which is in line with relatively high thermal maturity. As all three CM populations experienced the major metamorphic overprint ∼3.3 Ga ago, a syngenetic formation of the CM with the host barite can be assumed or, in case of the vein-hosted secondary CM, an emplacement soon after barite growth.

Place, publisher, year, edition, pages
2023. Vol. 2023
National Category
Geology
Identifiers
URN: urn:nbn:se:lnu:diva-127542DOI: 10.3997/2214-4609.202333167Scopus ID: 2-s2.0-85214691887OAI: oai:DiVA.org:lnu-127542DiVA, id: diva2:1834855
Conference
 IMOG 2023
Available from: 2024-02-05 Created: 2024-02-05 Last updated: 2025-01-22Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full textScopus

Authority records

Reinhardt, ManuelDrake, Henrik

Search in DiVA

By author/editor
Reinhardt, ManuelDrake, Henrik
By organisation
Department of Biology and Environmental Science
Geology

Search outside of DiVA

GoogleGoogle Scholar

doi
urn-nbn

Altmetric score

doi
urn-nbn
Total: 56 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf