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TEXTURAL AND MICROANALYSIS OF IGNEOUS ROCKS: TOOLS ...

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The common occurrence of population B crystals in rounded and embayed crys-<br />

tals in Site 1203 Units 3, 14, and 31 and Site 884 Unit 8 basalts is a qualitative<br />

indication that these crystals were commonly out of equilibrium with their host<br />

basalts, which is also consistent with plagioclase accumulation.<br />

Huang et al. [72] specifically noted the significance of plagioclase accumulation<br />

in Unit 14 and 31 lavas from Site 1203 (i.e. Fig. 13 of [72]). My observations<br />

of strongly upward kinked plagioclase CSDs for these two Units (Fig. 3.4e,l) are<br />

consistent with their assertions of plagioclase accumulation. Although I provide<br />

seemingly independent evidence of plagioclase accumulation in these two lavas,<br />

the exact origin of the non-linear CSDs of these lavas is not straightforward. Both<br />

magma mixing and crystal accumulation can produce a non-linear CSDs (Fig. 3.3)<br />

[67]. Higgins [67] discussed a number of explanations for curved CSDs, including<br />

size dependent crystal growth rate, destruction of small crystals (i.e., fines destruc-<br />

tion), changes in cooling rate, or changes in the dominant crystallizing phases.<br />

Cashman and Marsh [20] and Marsh [99] presented sound arguments against size<br />

dependent growth. Fines destruction and changes in cooling rate cannot be ruled<br />

out based upon textural evidence alone. I have noted distinct compositional dif-<br />

ferences between population A and B crystals from Site 1203 Units 14 and Units<br />

31, which is evidence against these processes as noted by Higgins [67]. Huang et<br />

al. [72] suggested a significant role for olivine and plagioclase fractionation during<br />

DSM basalt petrogenesis, and there is little other evidence to indicate there was<br />

a change in the dominant crystallizing phases. Although I cannot rule out minor<br />

roles for any of these processes, I suggest accumulation and/or magma mixing are<br />

responsible for the majority of the CSD curvature I have noted.<br />

Higgins [67] noted that magma mixing would lead to compositional differences<br />

123

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