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Spherule layers in the 2011 ICDP drilling in the Barberton Mountain Land: Early impact record on Earth

Fachliche Zuordnung Paläontologie
Förderung Förderung von 2013 bis 2017
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 235479303
 
Erstellungsjahr 2018

Zusammenfassung der Projektergebnisse

This project dealt with the characterization of two new drill cores from the Barberton Greenstone Belt (BGB). The ICDP core BARB 5 intersected not less than 5, ca. 4 cm wide spherule layer (SL) beds and 3 further spherule showings, and core CT 3 retrieved 17 SL deposits. The BARB 5 SLs occur at the transition from Fig Tree Group to Onverwacht Group (Barberton Greenstone Belt), and the CT 3 occurrences are likely part of the uppermost Fig Tree Group section or also occur at the transition to the Onverwacht Group. All SLs were petrographically studied and microchemically investigated. As in most other SL occurrences in the BGB, the new SLs and some of the hosting strata have a very large range of Ir concentrations, with many samples displaying super-chondritic values. In this study, the application of a combination of instrumental neutron activation and microchemical techniques resolved the cause of such anomalous enrichments. The work by Mohr-Westheide et al. (2015) based on scanning electron microscopy–energy dispersive X-ray spectrometry at high spatial resolution identified local areas of platinum group element (PGE) enrichment, invariably in the vicinity of Ni-rich chromium spinel (Ni-Cr spinel) clusters. These areas are invariably present in subsamples for which bulk analysis has previously demonstrated enrichment of the Extraterrestrial Component (ETC). By applying high-resolution BSE-EDS scanning microscopy and dedicated feature analysis techniques it was then possible to identify µm to sub-µm sized platinum groups metals (PGMs) and PGE sulfarsenides as carriers of the ETC. The PGMs are considered primary impact-related/generated particles, whereas the sulfarsenides represent the product of secondary alteration with S-rich solutions. Step three in this innovative approach was then to apply TEM techniques to study the textures/structures of the PGMs and obtain sub-µm to nanometer scale chemical compositions. The variability of PGM types indicates that most likely several processes (sublimation from the impact vapor plume, crystallization from impact melt, etc) were responsible for the formation of these particles. Having demonstrated that the excessively high contents of ETC are the result of a PGM micro-nugget effect, the previous hypothesis that measured PGE abundances could be directly converted to sizes of Archean impact projectiles has been shown as not valid. Furthermore, the µ-XRF technique was successfully employed to identify structures and semi-quantitative chemical information on bulk drill core of SL and host rock material. Further dating efforts and stratigraphic refinement of SL positions are required to obtain conclusive evidence on whether these new SL intersections should be linked to previously identified SLs at the transition from Fig Tree to Onverwacht groups.

Projektbezogene Publikationen (Auswahl)

 
 

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