TEXTURAL AND MICROANALYSIS OF IGNEOUS ROCKS: TOOLS ...
TEXTURAL AND MICROANALYSIS OF IGNEOUS ROCKS: TOOLS ...
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 />
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