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Under The Volcano: Gases Yield Clues To Mount St. Helens' Next Eruption

Date:
October 15, 2004
Source:
University Of Bristol
Summary:
Research reported in the journal Science shows that rocks erupted from the Mount St Helens volcano in 1980 preserve a remarkable record of the goings-on beneath the volcano in the period prior to its eruption.

Mount St. Helens dome and uplift with new growth, as seen from the southeast. USGS Photograph taken on 13 October 2004, by Kathy Cashman.
Credit: Photo courtesy of U.S. Geological Survey

Research reported in Science today (14 October 2004) shows that rocks erupted from the Mount St Helens volcano in 1980 preserve a remarkable record of the goings-on beneath the volcano in the period prior to its eruption.

Professor Jon Blundy and his PhD student Kim Berlo from the Earth Sciences Department at Bristol University, UK, demonstrate that monitoring the content of gases being emitted from the volcano right now might predict whether the next eruption will be so catastrophic, and when it might occur.

The team identified a subterranean reservoir full of magma at around 7 km depth that had been steadily shedding gas for at least five years prior to the eruption. Some of this gas then accumulated in a more shallow and short-lived reservoir around 4 km beneath the volcano. It is the expansion of these gas bubbles as they rise up that ultimately drives volcanic eruptions.

Blundy and his team showed that the magma which erupted explosively in May 1980 came largely from both the deep and shallow reservoirs, while subsequent, more gentle eruptions in 1980 came exclusively from magma trapped at shallow levels. Clearly there is a link between the storage depth of the magma and its eruptive style.

Furthermore, using short-lived radioactive isotopes, they demonstrate that the process of gas transfer from deep to shallow reservoirs must have occurred just weeks before the eruption.

Mount St. Helens recently cleared its throat with a series of small steam and ash eruptions. But it is unclear whether this activity will evolve into a more substantial eruption such as the explosion in 1980 which removed 400 metres off the top of the volcano and spewed ash over an area of more than 56,000 square kilometres.

Professor Blundy said: ‘We have shown there is a link between the storage depth of magma and the explosiveness of an eruption. This suggests that monitoring the abundance of short-lived radioactive isotopes above restless volcanoes could be a useful tool for predicting the style of the next eruption. It might also provide clues as to when the next eruption will occur’.

A wide range of print-quality images of Mount St Helens, freely available to the media, can be down-loaded from: http://vulcan.wr.usgs.gov/Volcanoes/MSH/Images/MSH04/


Story Source:

The above story is based on materials provided by University Of Bristol. Note: Materials may be edited for content and length.


Cite This Page:

University Of Bristol. "Under The Volcano: Gases Yield Clues To Mount St. Helens' Next Eruption." ScienceDaily. ScienceDaily, 15 October 2004. <www.sciencedaily.com/releases/2004/10/041015101945.htm>.
University Of Bristol. (2004, October 15). Under The Volcano: Gases Yield Clues To Mount St. Helens' Next Eruption. ScienceDaily. Retrieved September 23, 2014 from www.sciencedaily.com/releases/2004/10/041015101945.htm
University Of Bristol. "Under The Volcano: Gases Yield Clues To Mount St. Helens' Next Eruption." ScienceDaily. www.sciencedaily.com/releases/2004/10/041015101945.htm (accessed September 23, 2014).

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