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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Figure 4 – 6: Compositions <strong>of</strong> chromian spinel cores in dunite <strong>and</strong><br />
harzburgite <strong>of</strong> Mawat peridotite plotted on Cr 3+ - Al 3+ -<br />
Fe 3+ cations diagram. ----------------------------------------------------------------53<br />
Figure 4 – 7: Compositions <strong>of</strong> chromian spinel cores in<br />
dunite,harzburgite <strong>and</strong> lherzolite <strong>of</strong> Pauza peridotite<br />
plotted on Cr 3+ - Al 3+ - Fe 3+ cations diagram. --------------------53<br />
Figure 4 – 8: Compositions <strong>of</strong> pyroxene in Pauza peridotite plotted<br />
on En-Wo-Fs diagram (after Morimoto et al., 1988). -- 54<br />
Figure 5 – 1: Chromian spinel compositions plotted on Cr# vs.<br />
Mg#. Fields aftrer (Raymond, 2002). ---------------------------------61<br />
Figure 5 – 2: Cyclic metamorphism <strong>of</strong> Chromian spinel in<br />
harzburgite. -----------------------------------------------------------------------------------62<br />
Figure 5 – 3: Cr# in spinel vs. Fo content <strong>of</strong> olivine in <strong>ultramafic</strong><br />
<strong>rocks</strong> from IZTZ. Fields for spinels occurring in abyssal<br />
(<strong>and</strong> ocean ridge), oceanic SSZ <strong>and</strong> passivemargin<br />
peridotites are after Dick <strong>and</strong> Bullen (1984) <strong>and</strong><br />
Pearce et al. (2000). OSMA field after Arai (1994). Pink<br />
boxes are Pauza, gray boxes are Mawat, <strong>and</strong> yallow<br />
triangles are Penjwin peridotites. ---------------------------------------63<br />
Figure 5 – 4: Chromian spinel compositions plotted on TiO 2 vs.<br />
Al 2 O 3 tectonic discrimination diagram. Fields for arc<br />
volcanic <strong>rocks</strong>, supra-subduction <strong>zone</strong> (SSZ), ocean<br />
isl<strong>and</strong> basalts (OIB), <strong>and</strong> MORB basalts <strong>and</strong><br />
peridotites after Kamentesky et al. (2001). ---------------------64<br />
Figure 6 – 1: A. Field photograph showing the Albitite pod with<br />
massive serpentinite in the Penjwin igneous complex.<br />
B. Sketch showing different mineral <strong>zone</strong>s in the<br />
metarodingite pod, A = serpentinite host rock, B =<br />
blackwall <strong>zone</strong>, C = grossular – prehnite <strong>zone</strong>, D =<br />
VIII