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Diagenetic imprints on magnetic mineral assemblages in marine ...

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Chapter 1<br />

2.1.1 Ir<strong>on</strong> (titanium) oxides<br />

4<br />

Magnetically, three naturally occurr<strong>in</strong>g ir<strong>on</strong> oxide <strong>m<strong>in</strong>eral</strong>s are important; magnetite,<br />

hematite and maghemite. Some properties of these <strong>m<strong>in</strong>eral</strong>s and several others are given<br />

<strong>in</strong> table 1. Magnetite is found <strong>in</strong> rocks and sediments and can also be produced by certa<strong>in</strong><br />

types of bacteria, known as magnetotactic bacteria, which use it for navigati<strong>on</strong>al<br />

purposes. Magnetite is characterised a high sp<strong>on</strong>taneous <strong>magnetic</strong> moment and by two<br />

important temperatures, i.e., the Curie po<strong>in</strong>t at 580 o C and the Verwey transiti<strong>on</strong> at about<br />

-150 o C (e.g., Dunlop and Özdemir, 1997). These temperatures and the respective<br />

changes <strong>in</strong> observed magnetisati<strong>on</strong> are frequently used <strong>in</strong> diagnostic tests.<br />

Table 1. Properties of some comm<strong>on</strong> <strong>magnetic</strong> <strong>m<strong>in</strong>eral</strong>s<br />

M<strong>in</strong>eral Formula Ms (kA/m) TC ( o C) <strong>magnetic</strong> structure<br />

Magnetite Fe3O4 480 580 ferri<strong>magnetic</strong><br />

Hematite α-Fe2O3 ~2.5 675 canted antiferro<strong>magnetic</strong><br />

Maghemite γ-Fe2O3 380 590-675 ferri<strong>magnetic</strong><br />

Goethite α-FeOOH ~2 120 antiferro<strong>magnetic</strong><br />

Greigite Fe3S4 ~125 ~330 ferri<strong>magnetic</strong><br />

Pyrrhotite Fe7S8 ~80 320 ferri<strong>magnetic</strong><br />

A more detailed descripti<strong>on</strong> is given by Hunt et al. (1995), Dekkers (1997) and Dunlop and Özdemir (1997).<br />

Hematite is comm<strong>on</strong> <strong>in</strong> soils and sediments, and is the ma<strong>in</strong> carrier of the<br />

magnetisati<strong>on</strong> of ‘red beds’, a major source of <strong>in</strong>formati<strong>on</strong> <strong>in</strong> classic paleomagentism<br />

(Evans and Heller, 2003). The <strong>m<strong>in</strong>eral</strong> is like magnetite characterized by two<br />

temperatures (e.g., Dunlop and Özdemir, 1997), the Néel temperature at 675 o C and the<br />

Mor<strong>in</strong> transiti<strong>on</strong> at approximately -15 o C (Mor<strong>in</strong>, 1950).<br />

Maghemite, the fully oxidised form of magnetite, is also frequently encountered <strong>in</strong><br />

soils. It has a Curie temperature at around 645 o C, that is unfortunately difficult to<br />

measure, there the <strong>m<strong>in</strong>eral</strong> is metastable, i.e. it transforms to hematite with a loss of<br />

magnetisati<strong>on</strong> (e.g., Dunlop and Özdemir, 1997). This so-called <strong>in</strong>versi<strong>on</strong> temperature can<br />

be used <strong>in</strong> identificati<strong>on</strong>, however it is very variable and many different values have been<br />

reported.<br />

In nature vary<strong>in</strong>g compositi<strong>on</strong>s for the above-menti<strong>on</strong>ed <strong>m<strong>in</strong>eral</strong>s are observed, <strong>in</strong><br />

most cases some ir<strong>on</strong> has been replaced by titanium. In Fig. 1 a ternary diagram<br />

illustrates the solid soluti<strong>on</strong> series <strong>in</strong> which ir<strong>on</strong> titanium <strong>m<strong>in</strong>eral</strong>s can occur. Two ma<strong>in</strong>

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