Abstract
Recent evidence for astronomical-induced cycles in banded iron formations (BIFs) hints at the intriguing possibility of developing astrochronological, i.e. precise time-stratigraphic, frameworks for the earliest Proterozoic as also reconstructed for parts of the Mesozoic and Paleozoic. The Kuruman Iron Formation (IF) (Griqualand West Basin, South Africa) and Dales Gorge Member of the Brockman IF (Hamersley Basin, Western Australia) are of special interest in this regard, given their inferred temporal overlap at ca. 2.47 Ga and similar long-period orbital eccentricity imprint. This suggests that these two BIFs may be correlated on the basis of their large-scale cycle patterns and using additional radio-isotopic age constraints. To examine the possibility of establishing such a framework, we generated and analysed several high-resolution proxy records from both drill-core and outcrop, combined with high-precision U-Pb dating of zircon from interbedded shale horizons. Time-series analysis of these records yields a variety of spectral peaks, of which a prominent ~5 m and ~16 m cycle can be linked to the basic stratigraphic alternations and bundling as observed in the field. New and revised 207Pb/206Pb ages calculated from the U-Pb data of the Dales Gorge Member and Kuruman IF, respectively, indicate a comparable average sedimentation rate of 10 to 12 m/Myr for both units. Based on this depositional rate, we attribute the ~5 m cycle to the long (~405 kyr) orbital eccentricity cycle. More tentatively, we interpret the ~16 m cycle as the very long (presently ~2.4-Myr) eccentricity cycle, having a reduced period of ~1.3 Myr due to chaotic behaviour in the solar system. Other identified cycles (~560 kyr, ~700 kyr and ~1.8 Myr) can be explained in terms of weaker orbital eccentricity components and/or as harmonics and combination tones of these cycles resulting from nonlinear responses. An initial attempt to establish cyclostratigraphic correlations between the Kuruman IF and Dales Gorge Member solely based on their characteristic cycle patterns proved unsuccessful, which may be due to a difference in the recording of the astronomical signal between different depositional environments. Next, we used the zircon ages to first constrain correlations at the scale of the ~16 m cycle, followed by a correlation of the basic ~5 m cycles. The resultant framework remains problematic and debatable at the individual ~405 kyr cycle-level, but provides a starting point for future studies. Particularly, our findings highlight the need for further investigations into how Milankovitch forcing influenced BIF sedimentation and paleoenvironmental conditions at a time when the Earth and solar system behaved fundamentally different from today.
| Original language | English |
|---|---|
| Pages (from-to) | 325-358 |
| Number of pages | 34 |
| Journal | South African Journal of Geology |
| Volume | 127 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - Jun 2024 |
Bibliographical note
Publisher Copyright:© 2024 The Authors. Some rights reserved.
Funding
This research was funded by the Dutch National Science Foundation grant NWO ALWOP.190 (FJH, PRDM, MLL) ; the Swiss National Science Foundation grant 200021_169086 (JHFLD) ; the Foundation Stichting Dr. Schuermann grants 2017-126, 2018-136 and 2019-145 (FJH, PRDM, MLL) and the Heising-Simons Foundation grant 2021-2797 (MLL) . We thank the people from Wireline Alliance for the downhole geophysical logging; Michael Wawrick and Lena Hancock from the GSWA for the HyLogger data extractions from cores DGM1 and SGP1; Gregory Jack for help with the drone flying and fieldwork logistics; Marcel van Maarssenveen, Jakob Steiner and Timothy Baars for their advice on the GPS measurements and photogrammetry modelling; Nam Hoang Hoai, Federico Mogavero and Jacques Laskar for their expertise and discussions on chaotic solar system evolution; and David de Vleeschouwer and Matthias Sinnesael for helpful reviews. Our special thanks go to the late Rineke Gieles for her dedicated help with the XRF core scanning and who sadly passed away in 2020, and to Prof. Nic Beukes, for his guidance in the UUBH1 drilling project and who sadly passed away in 2023.
| Funders | Funder number |
|---|---|
| Nederlandse Organisatie voor Wetenschappelijk Onderzoek | |
| Heising-Simons Foundation | 2021-2797 |
| Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung | 2019-145, 2018-136, 2017-126, 200021_169086 |
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