BASALTIC LAVAS OF MOUNT ST. HELENS: EVIDENCE FOR DIVERSE MANTLE SOURCES AND INPUTS FROM MORE EVOLVED MAGMAS
New SEM/EMP studies of MSH basalts document that olivine core compositions span large ranges (up to 23 mole % Fo, with an average of ~13 mole %) within individual samples. Cores with higher Fo contents than predicted from whole-rock Mg# suggest that MSH basalts were likely derived from more primitive LKT and IPBs variants similar to those from nearby Indian Heaven and Battleground lava fields. Some samples contain olivine grains with cores of Fo60-72 (lower than predicted from whole-rock Mg#s). Those grains exhibit embayments, reverse zoning, and/or overgrowth rims of orthopyroxene with Mg#s ~70-65. The diverse olivine populations in some MSH basalts indicate that they received variable and relatively small inputs from more silicic magmas. Another explanation is petrological cannibalism and incorporation of antecrysts derived from previously emplaced magma batches. Despite close proximity of their vents (within a few km of each other) and eruption within a short time interval (< 300 years), we see no evidence of significant mingling or mixing between the LKTs and IPBs. We conclude that they ascended from different magma source regions along narrowly separated, discrete plumbing systems. This conclusion brings into question the existence of a broad region of hybridization in the crust (MASH zone), as well as lateral migration of magma from east of MSH as suggested by geophysical studies (Hill et al., 2009, doi: 10.1038/NGEO661; Kiser et al., 2016, doi: 10.1130/G37591.1).