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Inclusions in Mount St. Helens dacite erupted from 1980 through 1983.

Heliker, C Christina (1995) Inclusions in Mount St. Helens dacite erupted from 1980 through 1983. Journal of Volcanology and Geothermal Research. 66; 1-4, Pages 115-135. 1995.

AuthorsHeliker, C Christina
Year1995
TitleInclusions in Mount St. Helens dacite erupted from 1980 through 1983.
SourceJournal of Volcanology and Geothermal Research. 66; 1-4, Pages 115-135. 1995.
PublisherElsevier. Amsterdam, Netherlands. 1995.
Document typeSerial
ISSN0377-0273
GeoRef1995-068533
KeywordsCascade-Range; chemical-composition; dacites-; eruptions-; gabbronorite-; gabbros-; igneous-rocks; inclusions-; intrusions-; lava-; melting-; mineral-inclusions; Mount-Saint-Helens; phase-equilibria; plutonic-rocks; plutons-; pumice-; pyroclastics-; sampling-; Skamania-County-Washington; United-States; volcanic-rocks; volcanism-; volcanoes-; Washington-
NotesIn memory of Harry Glicken
DOI10.1016/0377-0273(94)00074-Q

Abstract

Inclusions of plutonic, metavolcanic and volcanic rocks are abundant in dacite pumice and lava from the 1980-1986 eruption sequence at Mount St. Helens. Point counts of inclusions exposed in talus blocks from the dome from 1980 through 1983 show that inclusions form approximately 3.5 vol% of the lava. Eighty-five percent of the inclusions are medium-grained gabbros with an average diameter of 6 cm. Additional rock types include quartz diorite, hornfelsic basalt, dacite, andesite and vein quartz. Disaggregated inclusions are common and define shear planes within the dome. These fragmented inclusions may significantly contaminate analyses of the dacite. The gabbroic inclusions are of four distinct types, all with mineral assemblages consistent with crystallization pressures of less than 9 kb. Textures and major-element compositions indicate that most of the gabbroic inclusions are cumulates. The most abundant inclusion type is laminated gabbronorite, which contains up to 9% interstitial glass, derived from partial melting. The presence of quartz veins and hornblende-bearing veins within sheared zones in the laminated gabbronorite indicates that the source of these inclusions was holocrystalline rock that had been penetrated by water-rich fluids. The gabbronorite contained sufficient water to be susceptible to partial melting when the magma that fed the 1980-1986 eruption sequence was emplaced nearby. Various types of gabbroic inclusions, including the laminated gabbronorite, are common in Mount St. Helens lavas of approximately the last 3000 years. This coincides with the interval in which Mount St. Helens first erupted basalt and basaltic andesite lavas. These observations, together with the fact that the gabbroic inclusions are compositionally unlike any of the Tertiary intrusive rocks in the Mount St. Helens area, strongly suggest that the inclusions are related to the introduction of basalt to the Mount St. Helens magmatic system. The source of the gabbros could be a layered mafic pluton formed through crystal accumulation from multiple batches of basaltic magma emplaced at mid- to upper-crustal depths beneath the volcano. The prevalence of explosive eruptions at Mount St. Helens may play a part in bringing the inclusions to the surface. The eruptive products of the cataclysmic eruption of May 18, 1980 contain notably fewer inclusions than the pyroclastic flows and dome lavas erupted subsequently. This suggests that the May 18 eruption shattered conduit wall rock that was subsequently stoped into the magma and carried to the surface later in the eruption series.

73 samples from this reference

SampleRock nameMajorTraceIsotope
s_70381-2MGabbro yes
s_70381-2MGabbro yes
s_70381-1CGabbro yes
s_70381-1CGabbro yes
s_70381-2MGabbro yes
s_70381-1CGabbro yes
s_70381-1CGabbro yes
s_70381-2MGabbro yes
s_70381-1CGabbro yes
s_70381-2MGabbro yes
s_70381-1CGabbro yes
s_70381-2MGabbro yes
s_70381-1CGabbro yes
s_70381-1CGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_41881-77PGabbro yes
s_80381-54JDiorite yes
s_80381-54JDiorite yes
s_80381-54JDiorite yes
s_80381-54JDiorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_41381 76CNorite yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_12481-3AGabbro yes
s_32281-4CGabbro yes
s_70381-1CGabbro yes
s_32181-1KGabbro yes
s_41881-77CGabbro yes
s_41881-80RGabbro yes
s_70381-2MGabbro yes
s_81881-69DGabbro yes
s_1XGabbro yes
s_62AGabbro yes
s_61881-84Gabbro yes
s_72881-30GGabbro yes
s_90881-1Gabbro yes
s_111880Gabbro yes
s_70381-3SGabbro yes
s_81481-1Gabbro yes
s_72881-1Gabbro yes
s_41881-80AGabbro yes
s_41381-76GNorite yes
s_60581-83SNorite yes
s_82281-68HNorite yes
s_41881-77PGabbro yes
s_30981-74GTroctolite yes
s_12581-1ANorite yes
s_41881-77RBasalt yes
s_72481-2Basalt yes
s_80581-2Basalt yes
s_80381-SOEBasalt yes
s_91780-2XBasalt yes
s_70381-4Basalt yes
s_70181-1SBasalt yes
s_82881-73XBasalt yes
s_82282-74TDacite yes
s_11281-62BDacite yes