| Tectonic setting | Cascade eruptions |
| Mount St. Helens | Mount Shasta |
| Related websites | References |
| The Cascade Mountains consist of several active volcanoes (triangles) as well
as many volcanic centers that were active during the Neogene and Quaternary. These
volcanoes are developed above a subduction zone that stretches from northern California to
southern British Columbia. The subduction zone involves the Juan de Fuca and related oceanic
plates that descend beneath the western edge of North America. Unlike typical subduction zones, no trench is present along the continental margin. Instead, terranes and the accretionary wedge have been uplifted to form a series of coast ranges and exotic mountains--Klamath Mountains. Inland from these coastal mountains are a series of valleys--Shasta, Willamette, Puget. These valleys represent old forearc basins, which have been uplifted. Major cities of the region are located in these valleys today--Portland, Seattle and Vancouver. |
The Cascade Mountains include more than a dozen, large volcanoes. Although they share general characteristics, each has unique geological traits and history. The major volcanoes of the Cascades are listed below.
| Volcano | Location | Eruptions | Mt. Garibaldi | British Columbia | none | Mt. Baker | Washington | 1792, 1843-65, 1870, 1880 | Glacier Peak | Washington | 1750 (?) | Mt. Rainier | Washington | 1841, 1843, 1854 | Mt. Adams | Washington | none | Mt. St. Helens | Washington | 1800-57, 1980-84 | |
|---|
| Volcano | Location | Eruptions | Mt. Hood | Oregon | 1854, 1859, 1865-66 | Mt. Jefferson | Oregon | none | Three Sisters | Oregon | 1853 (?) | Newbury Caldera | Oregon | none | Mt. Thielsen | Oregon | none | Crater Lake | Oregon | none | Mt. McLoughlin | Oregon | none | |
|---|
| Volcano | Location | Eruptions | Medicine Lake | California | 1910 | Mt. Shasta | California | 1786, 1855 | Cinder Cone | California | 1850-51 | Lassen Peak | California | 1914-17 | Chaos Crags | California | 1854-57 | |
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| Cascade eruptions |
Magma of the Cascades is generated by partial melting along the subduction zone. The most typical lava of Cascade eruptions is andesite, an intermediate igneous composition which is characteristic for subduction zones around the world. Other lava types span the spectrum of composition from basalt, to dacite and rhyolite. Each major Cascade volcano has a distinct signature in terms of its lava composition; some are quite consistent, whereas others show great variability.
Eruptions of andesite and basalt tend to be relatively calm events dominated by lava flows. Exceptions occur where such magmas encounter substantial groundwater (under snow cover, glaciers), which may create steam-driven explosions of the Strombolian type. Dacite and rhyolite magmas are more viscous and tend to develop higher gas pressures. Such magmas may explode violently in catastrophic eruptions that release immense volumes of tephra, ash, and pumice. Glacier Peak, Mazama (Crater Lake), and Mt. St. Helens have experienced this type of eruption.
Recent eruptions, particularly Mt. St. Helens in 1980, have provided important clues for better understanding of ancient volcanism in the Cascade system. One result of the 1980 eruption was recognition of the importance of landslides and mass movements in the development of volcanic landscapes. A huge section on the northern side of Mt. St. Helens slid away and created a jumbled landslide terrain many miles from the volcano itself. Accompanying pyroclastic flows and mudflows swept across the landscape. Similar events have occurred at Mt. Shasta and other Cascade volcanoes in prehistoric times.
Map of Mt. St. Helens and surroundings showing eruption zones.
Mount St. Helens
Mount St. Helens experienced a violent eruption on May 18th 1980. It was one of the most closely
studied volcanic eruptions on record. The main eruptions displaced 2.7 km³ of rock and
extruded ½ km³ of magma. In comparison to other major
volcanic eruptions, this was not particularly large. For example, the Krakatoa eruption of
1883 was 6 km³, and some prehistoric eruptions have been 100s to 1000s of km³.
Events leading up to the main eruption included several distinct phenomena (Decker and Decker
1981).
The main eruption was set off by an earthquake of 5.1 magnitude at 8:32 am on May 18. The
quake struck under the northern side of the volcano and triggered a massive landslide. The
whole northern side of the volcano began to slide down as a rippling mass. Seconds later a huge
explosion of ash clouds blew out the side of the volcano. This lateral blast was directed over
the terrain to the north. It consisted of superheated steam clouds filled with ash and rock
debris. The lateral blast created three zones of destruction.
Some 550 km² were devastated by the lateral blast, which was finished by 9:00 am. At
that time, a vertical ash cloud began to build up; it reached an altitude of 20 km before
waning in the afternoon. High-altitude ash was blown to the northeast all day across Washington
and Idaho. The landslide, which initiated the eruption, also generated debris-avalanche
deposits that were transported some distance down the North Fork of the Toutle River valley.
This event was the largest such historical landslide, having a volume of 2½-3 km³
and extending 25 km from the source area (Lipman and Mullineaux 1981). In addition, the
landslide generated mudflows, which surged along stream valleys, especially the Toutle River.

© Weyerhaeuser Co. (1988).
| View of Mt. Shasta from the north. Elevation of the summit peak (Hotlum cone to left) is 14,161 feet. Shastina is the slightly lower peak to right. Photo date 5/99; © J.S. Aber. |
Ancestral Mt. Shasta began to develop at least half a million years ago. The exact nature of this volcano is unknown, but it must have been quite large, as it generated a tremendous landslide between 300,000 and 360,000 years ago (Harris 1988). The enormous slide transported chaotic blocks of rocks into Shasta valley. The avalanche deposits extend 45 km northwest of the volcano and represent a volume of about 27 km³--about ten times the volume of the Mt. St. Helens 1980 avalanche deposits.
Mount Shasta vicinity has experienced four main eruptive cycles during the past half million years--Sargeants Ridge, Misery Hill, Shastina, and Hotlum. Hornblende and pyroxene andesite lava flows dominate the eruptive cycles, which each terminate with intrusion of dacite domes (Harris 1988). These domes, being more resistant to erosion, form the summit peaks of Mount Shasta, Shastina, and Black Butte. The Hotlum eruptive center is considered to be active, as the summit dome is still hot. Boiling sulfur springs and steam emissions were seen in the 1850s, but these are reduced now to a single hot spring and small fumaroles.
| Geology professor, Bill Hirt (right), leads a field excursion into a lava-tube cave near Mt. Shasta. Photo date 5/99; © J.S. Aber. |
| Section through a small cinder cone on the Deer Mountain shield volcano, northeast of Mt. Shasta. Compare with cinder cones in Eifel district. Photo date 5/99; © J.S. Aber. |
| Near-vertical dike within the cinder cone on Deer Mountain shield volcano. Photo date 5/99; © J.S. Aber. |
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Related websites
References

GO 326/ES 767 © J.S. Aber (2008).