Detrital remanent magnetization of single-crystal silicates with magnetic inclusions: constraints from deposition experiments

Author:

Chang Liao12,Hong Hoabin1,Bai Fan1,Wang Shishun1,Pei Zhaowen1,Paterson Greig A3ORCID,Heslop David4,Roberts Andrew P4,Huang Baochun1,Tauxe Lisa5ORCID,Muxworthy Adrian R6ORCID

Affiliation:

1. Laboratory of Orogenic Belts and Crustal Evolution, School of Earth and Space Sciences, Peking University, 100871 Beijing, China. E-mail: liao.chang@pku.edu.cn

2. Laboratory for Marine Geology, Qingdao National Laboratory for Marine Science and Technology, 266071 Qingdao, China

3. Department of Earth, Ocean and Ecological Sciences, University of Liverpool, Liverpool, UK

4. Research School of Earth Sciences, Australian National University, Canberra, ACT 2601, Australia

5. Scripps Institution of Oceanography, University of California San Diego, La Jolla, CA 92093-0220, USA

6. Department of Earth Science and Engineering, Imperial College London, London, UK

Abstract

SUMMARY Quasi-linear field-dependence of remanence provides the foundation for sedimentary relative palaeointensity studies that have been widely used to understand past geomagnetic field behaviour and to date sedimentary sequences. Flocculation models are often called upon to explain this field dependence and the lower palaeomagnetic recording efficiency of sediments. Several recent studies have demonstrated that magnetic-mineral inclusions embedded within larger non-magnetic host silicates are abundant in sedimentary records, and that they can potentially provide another simple explanation for the quasi-linear field dependence. In order to understand how magnetic inclusion-rich detrital particles acquire sedimentary remanence, we carried out depositional remanent magnetization (DRM) experiments on controlled magnetic inclusion-bearing silicate particles (10–50 μm in size) prepared from gabbro and mid-ocean ridge basalt samples. Deposition experiments confirm that the studied large silicate host particles with magnetic mineral inclusions can acquire a DRM with accurate recording of declination. We observe a silicate size-dependent inclination shallowing, whereby larger silicate grains exhibit less inclination shallowing. The studied sized silicate samples do not have distinct populations of spherical or platy particles, so the observed size-dependence inclination shallowing could be explained by a ‘rolling ball’ model whereby larger silicate particles rotate less after depositional settling. We also observe non-linear field-dependent DRM acquisition in Earth-like magnetic fields with DRM behaviour depending strongly on silicate particle size, which could be explained by variable magnetic moments and silicate sizes. Our results provide direct evidence for a potentially widespread mechanism that could contribute to the observed variable recording efficiency and inclination shallowing of sedimentary remanences.

Funder

National Natural Science Foundation of China

Royal Society

Australian Research Council

NERC

NSF

Publisher

Oxford University Press (OUP)

Subject

Geochemistry and Petrology,Geophysics

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