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TEXTURAL AND MICROANALYSIS OF IGNEOUS ROCKS: TOOLS ...

TEXTURAL AND MICROANALYSIS OF IGNEOUS ROCKS: TOOLS ...

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3.6.3 Crustal Magma Evolution: Insights from Trace Elements<br />

3.6.3.1 Crystal Population Origins<br />

I use Y as a proxy for the heavy REE (HREE), because Y 3+ has a ionic ra-<br />

dius intermediate between Dy 3+ and Ho 3+ , and REE heavier than Eu are highly<br />

incompatible in plagioclase and thus at or below LA-ICP-MS analytical detection<br />

limits. Ratios of LREE such as La or Ce to Y provide insight into OIB (high<br />

La/Y) vs. MORB (low La/Y) source affinities (see Figs. 3.13, 3.12). Trivalent<br />

La and Ce 3+ have the largest ionic radii of the REE and are the two least com-<br />

patible REE in a crystallizing basaltic assemblage (e.g., plagioclase + olivine ±<br />

clinopyroxene). Lanthanum and Ce are difficult to fractionate from one another by<br />

partial crystallization, and in this sense they provide insight into mantle source<br />

affinity. If Unit 3 population A and B crystals indeed share a common parent<br />

magma, as indicated by their major element similarities, then parent magmas of<br />

these populations should have similar La/Ce and La/Y ratios.<br />

Parent magmas of Unit 3 population A and B crystal cores and Unit 3 whole-<br />

rock data reported by Huang et al. [72] have broadly similar Sr abundances,<br />

La/Ce and La/Y ratios (Figs. 3.12a, 3.13), which supports my initial hypothesis<br />

that population A and B crystals had compositionally similar parent magmas. The<br />

extension of Unit 3 population B parent magmas to slightly higher Sr abundance<br />

can be attributed to crystallization of these older crystals from less fractionated<br />

magmas with a source shared with the population A crystals. The gentle upward<br />

curvature of the plagioclase CSD from the top of Unit 3 supports this notion, as it<br />

provides evidence of minor accumulation of larger (i.e., older) crystals. Accumu-<br />

lation and partial resorption of crystalline debris (i.e., large rounded population<br />

B crystals) was volumetrically minor, such that the resultant bulk-rock compo-<br />

127

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