Abstract
Understanding the locus of fluid flow along thrust and splay faults is important to understand the hydraulic properties of accretionary systems and fault mechanics. Here, we use rock magnetic techniques in combination with backscattered electron imaging to depict the locus of enhanced magnetic mineral alteration within the Pāpaku fault, an active splay fault of the subduction interface at the northern Hikurangi Margin. The Pāpaku fault was cored at Site U1518 during Expedition 375 of the International Ocean Discovery Program and we report room temperature magnetic parameters, complemented by first-order reversal and thermomagnetic curves in the depth interval 250–400 m below seafloor (mbsf). The ∼60-m wide Pāpaku fault zone comprises two main slip zones, referred to as the upper main brittle (304–321 mbsf) and lower subsidiary (351–361 mbsf) fault zones, and an intervening zoned, termed the lower ductile deformation zone. Two narrow zones, at the top of the main brittle fault zone, and one in a sand-rich interval above the subsidiary fault zone, experienced enhanced magnetic mineral diagenesis, which resulted in the recrystallization of ferrimagnetic greigite to paramagnetic pyrite. We propose that secondary magnetic mineral diagenesis was driven by anaerobic methane oxidation within these intervals, which occurs in the presence of methane and sulfate. We relate the observed changes to the fault parallel transport of fluids which is restricted to two damage zones. Overlying compacted and clay-rich sediments likely act as a barrier to upward advective flow through the fault zone and into the hanging wall.
Original language | English |
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Article number | e2020JB020671 |
Number of pages | 15 |
Journal | Journal of Geophysical Research: Solid Earth |
Volume | 126 |
Issue number | 2 |
DOIs | |
Publication status | Published - Feb 2021 |
Bibliographical note
Funding Information:This study used samples and data of the International Ocean Discovery Program Expeditions 372 and 375. The authors are grateful to the science party and all technical staff that assisted with the acquisition of samples, data, and contributed in scientific discussions. A.G. acknowledges funding through NWO DeepNL (Grant no. 2018.040), the Korea Institute of Energy Technology Evaluation and Planning (KETEP), and the Ministry of Trade, Industry & Energy (MOTIE) of the Republic of Korea (Grant no. 20168510030830). Lilly Zerbst assisted with early magnetic analyses during tenure of an undergraduate scholarship under the framework of the RISE worldwide program of the German Academic Exchange Service (DAAD). The authors are grateful to Maartje Hamers who assisted with early SEM investigations, Tilly Bouten who produced BSE images on the electron microprobe, Bertwin de Groot who conducted thermomagnetic experiments, Patrick Fulton and Bob Musgrave for reviews on the manuscript.
Funding Information:
This study used samples and data of the International Ocean Discovery Program Expeditions 372 and 375. The authors are grateful to the science party and all technical staff that assisted with the acquisition of samples, data, and contributed in scientific discussions. A.G. acknowledges funding through NWO DeepNL (Grant no. 2018.040), the Korea Institute of Energy Technology Evaluation and Planning (KETEP), and the Ministry of Trade, Industry & Energy (MOTIE) of the Republic of Korea (Grant no. 20168510030830). Lilly Zerbst assisted with early magnetic analyses during tenure of an undergraduate scholarship under the framework of the RISE worldwide program of the German Academic Exchange Service (DAAD). The authors are grateful to Maartje Hamers who assisted with early SEM investigations, Tilly Bouten who produced BSE images on the electron microprobe, Bertwin de Groot who conducted thermomagnetic experiments, Patrick Fulton and Bob Musgrave for reviews on the manuscript.
Publisher Copyright:
© 2021. The Authors.
Keywords
- diagenesis
- fluid flow
- greigite
- rock magnetism
- splay fault
- subduction zone