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petrology of ultramafic and related rocks along iraqi zagros thrust zone

petrology of ultramafic and related rocks along iraqi zagros thrust zone

petrology of ultramafic and related rocks along iraqi zagros thrust zone

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Typical ophiolite sequences are composed <strong>of</strong> a thin layer <strong>of</strong> deep-sea<br />

sediments, overlying a sequence <strong>of</strong> basaltic pillow lavas, sheeted dike<br />

complexes, foliated to layered gabbro, <strong>and</strong> finally an <strong>ultramafic</strong> complex,<br />

which can have an exposed thickness <strong>of</strong> up to 7 km. This <strong>ultramafic</strong><br />

section <strong>of</strong> ophiloite can vary in composition, however, it is most commonly<br />

dominated by varieties <strong>of</strong> peridotite typically associated with the mantle<br />

such as harzburgite (olivine <strong>and</strong> orthopyroxene rich), lherzolite (olvine,<br />

orthopyroxene, <strong>and</strong> clinopyroxene rich), <strong>and</strong> wehrlite (olivine <strong>and</strong><br />

clinopyroxene rich), <strong>and</strong> dunite (olivine rich).<br />

1-1-2-3 Replacive <strong>ultramafic</strong>s<br />

Another non-cumulate mechanism for the formation <strong>of</strong> <strong>ultramafic</strong><br />

<strong>rocks</strong> involves the replacement <strong>of</strong> pyroxene minerals with olivine through<br />

chemical reactions between a silica-poor magma <strong>and</strong> a pyroxene-rich host<br />

rock (Kubo, 2002). This replacement occurs as the process that silica-poor<br />

magma rises through the mantle <strong>and</strong> saturates pyroxene-rich mantle<br />

lherzolite or harzburgite during its ascent. As silica-rich minerals<br />

generally have a lower melting temperature than silica-poor minerals, the<br />

pyroxene minerals are partially dissolved by the magma, leaving behind<br />

olivine in place <strong>of</strong> pyroxene (Kubo, 2002).<br />

Because replacive processes have only recently been defined, there are few<br />

studies which focus on the extent to which replacement plays a role in the formation<br />

<strong>of</strong> dunites (Kubo, 2002). At this time, replacive processes are thought to occur most<br />

commonly in the transition <strong>zone</strong> <strong>of</strong> ophiolite sequences, between <strong>ultramafic</strong> tectonite<br />

<strong>and</strong> <strong>ultramafic</strong> cumulate units (Arai, 1994).<br />

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