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1 - Introduction

from Part I - Essentials of Mineral Magnetism

Published online by Cambridge University Press:  07 January 2026

Andrew P. Roberts
Affiliation:
Australian National University, Canberra

Summary

The question ‘what use is mineral magnetism?’ is addressed in this chapter. Magnetic rock-forming minerals can record magnetic information on timescales that exceed the age of the Earth, which enables paleomagnetism to underpin the global plate tectonic paradigm and provide the geomagnetic polarity timescale that is used to calibrate geological time. Paleomagnetic analysis also enables understanding of terrestrial and extraterrestrial magnetic fields and planetary processes that generate these fields and their variations through time. Environmental magnetism exploits the sensitivity of magnetic minerals to environmental processes at Earth’s surface, which facilitates understanding of the climatic, tectonic, or other driving forces of environmental change. The magnetic properties of nanoparticles are also exploited by organisms, as studied in biomagnetism, and are manipulated by humans in industrial, technological, and medical applications, which makes mineral magnetism useful in an exceptional range of fields. This book serves workers in these fields by providing an introduction to mineral magnetism and in-depth treatments of the magnetic properties of terrestrial magnetic minerals.

Information

Figure 0

Figure 1.1 Geomagnetic polarity timescale (GPTS) for the last 170 Ma, which is defined largely using the marine magnetic anomaly record. Black = normal polarity; white = reversed polarity. Geological epochs are listed to the right of the GPTS; Pleist. = Pleistocene; Plio. = Pliocene. After Ogg (2012).Figure 1.1 long description.

Figure 1

Figure 1.2(a) Simple block model of uniformly magnetized blocks of ocean crust that give rise to measured marine magnetic anomalies.Figure 1.2a long description.

(modified from Fig. 3 of Pitman and Heirtzler (1966))
Figure 2

Figure 1.2(b) More complex crustal magnetization structures with magnetic anomaly profiles from lava emplacement models compared to profiles for the East Pacific Rise. A bimodal emplacement model was used to simulate off-axis thickening of the extrusive layer as inferred from seismic observations. The upper model has smaller volumetric contributions from off-axis flows that are more consistent with the observed anomaly profile. Lava magnetization is proportional to geomagnetic field intensity. Colours correspond to isochrons in extrusives; dykes are indicated in black. Magnetic anomalies were calculated from multiple strips through the model. The anomaly for a constant thickness source (0.5 km) and magnetization proportional to geomagnetic intensity is shown in red.Figure 1.2b long description.

From Fig. 5 of Gee et al. (2000).
Figure 3

Figure 1.3 Age of ocean lithosphere based on marine magnetic anomalies. Light grey = continents; dark grey = continental margins; black lines = plate boundaries.Figure 1.3 long description.

From Fig. 1a of Müller et al. (2008).
Figure 4

Figure 1.4 Illustration of climate forcing of Saharan dust deposition in marine sediments. The eolian hematite record (bottom, black) with band-pass filtered components of the dust record (blue; period bands are in kyr) from Larrasoaña et al. (2003), which reflects an immediate response to insolation-driven African monsoon forcing at all major orbital periods (red) from Laskar et al. (1993); band-pass filtering used the same band as the dust record with normalization by the respective standard deviation. The band-pass-filtered dust signal is scaled identically for all period bands and is multiplied by −1 because of anti-correlated dust production with insolation-driven monsoon response.

Modified from Figs. 4 & 8 of Larrasoaña et al. (2003).
Figure 5

Figure 1.5 Illustration of the diversity of bacteria, chain types, and magnetic mineral morphologies in magnetotactic organisms. Bright-field transmission electron microscope (TEM) images of (a) magnetotactic coccus strain SHHC-1 (Zhang et al., 2017), (b) magnetotactic spirillum MYS-1 (Li et al., 2013), (c) magnetotactic bacterium strain SHHR-1 (Li et al., 2017), and (d) Candidatus Magnetobacterium casensis strain MYR-1 (Li et al., 2015). (e–h) High-resolution TEM images of individual magnetite particles produced by (e) SHHC-1, (f) MYS-1, (g) SHHR-1, and (h) MYR-1, respectively. All particles were imaged along the [011] zone axis of magnetite to illustrate the (e) octahedral, (f) cubo-octahedral, (g) elongated prismatic, and (h) bullet-shaped morphologies of the respective magnetic particles. Bright-field TEM images of a rod-shaped bacterium that produces (i) bullet-shaped magnetite and (j) prismatic greigite in the same cell (Wang et al., 2013). (k) High-angle annular dark-field-scanning TEM (HAADF-STEM) image of two MYR-1 cells and three magnetotactic cocci. (l) HAADF-STEM image with energy-dispersive X-ray elemental mapping of the bacteria in (k) with sulphur-rich granules (green) and polyphosphate inclusions (blue) within magnetotactic bacteria in addition to iron-rich magnetite particles (red) (Li et al., 2015).Figure 1.5 long description.

Original figure with unpublished images provided by Prof. Jinhua Li.
Figure 6

Figure 1.6(a) A colloidal suspension including drug-bearing magnetic nanoparticles is injected into the blood stream and directed to pathological tissue using focussed magnetic fields.Figure 1.6a long description.

Modified from Fig. 5 of Pankhurst et al. (2003).
Figure 7

Figure 1.6(b) Schematic detail of a magnetic nanoparticle designed for drug delivery. Magnetic nanoparticles have high surface area to volume ratios and are reactive, so they are covered with protective coatings, including polymers, silica or gold. Active therapeutic biomolecules are bound to the protective coating with organic linkers. See text for discussion.Figure 1.6b long description.

From Fig. 1 of McBain et al. (2008).

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  • Introduction
  • Andrew P. Roberts, Australian National University, Canberra
  • Book: Mineral Magnetism
  • Online publication: 07 January 2026
  • Chapter DOI: https://doi.org/10.1017/9781108935630.003
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  • Introduction
  • Andrew P. Roberts, Australian National University, Canberra
  • Book: Mineral Magnetism
  • Online publication: 07 January 2026
  • Chapter DOI: https://doi.org/10.1017/9781108935630.003
Available formats
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Save book to Google Drive

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  • Introduction
  • Andrew P. Roberts, Australian National University, Canberra
  • Book: Mineral Magnetism
  • Online publication: 07 January 2026
  • Chapter DOI: https://doi.org/10.1017/9781108935630.003
Available formats
×