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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tion driven plumes, or stirring by new magma input [83, 98]. In the case of the<br />
OJP magma chamber system, magma in the chamber interior(s) was the most<br />
eruptible, had Kwaimbaita or Kroenke basalt-like composition(s), and made up<br />
the most significant compositional and textural fractions of basalts erupted to<br />
the surface. Disruption of solidification fronts released evolved material (liquid +<br />
crystals) to mix with the main body of magma e.g., [98]. Mixing small fractions of<br />
evolved material from disrupted solidification fronts into the main magma body<br />
can lead to changes in basalt chemistry (Marsh, 1996). However, if the geometry<br />
of the OJP magma chamber system was such that inputs from disrupted solid-<br />
ification fronts were small relative to the size of the magma body, the input of<br />
more evolved material would have had little affect on the bulk magma chemistry.<br />
Evidence for this process is thus best preserved by allochthonous crystals e.g.,<br />
[37, 98], much like the An65−73 phenocrysts with evolved parent magma composi-<br />
tions and the An80−86 xenolith crystals with primitive magma compositions, which<br />
are all out of equilibrium with the host Kwaimbaita basalt. Parent magma trace<br />
element compositions of An65−73 phenocryst zones, which trend to much more<br />
evolved compositions than whole-rock data, suggest some of these crystals grew<br />
deep within solidification fronts that were eroded and mixed into the main magma<br />
body. Crystals with similarly evolved compositions may also form in dikes and<br />
conduits within the magma chamber system that become readily congested. In<br />
these regions geometry and magma supply rate allow solidification fronts to prop-<br />
agate inward and meet filling the space with a crystal mush that has a network<br />
of interstitial spaces filled with variably evolved melts [98]. Within the interstices<br />
of the crystal mush significant melt differentiation can occur where the mush is<br />
infrequently flushed with new (primitive) melt. I suggest the xenolith crystals and<br />
78