27 August 2010
Montserrat and the Soufriere Hills volcano
Posted by Jessica Ball
This summer I was lucky enough to take an absolutely amazing field trip on the island of Montserrat, where my advisor spent two weeks showing us around her old stomping grounds. And let me tell you, I would have no problem doing volcanology on a Caribbean island for a while…
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From http://travel.state.gov/travel/cis_pa_tw/cis/cis_974.html |
Montserrat is part of the Lesser Antilles volcanic arc, which is formed by the subduction of the Atlantic tectonic plate below the Caribbean plate. Most of the islands in the arc have andesitic volcanoes, which tend to produce explosive eruptions and lava domes. Montserrat itself is composed of three different volcanic centers: the Silver Hills in the north (the oldest, where the rocks date to ~11-25 million years), the Centre Hills in the center (9.5 – 5.5 million years), and the Soufriere / South Soufriere Hills in the south (at least 1.7 million years to the present). (For more information on the argon-argon dates that produced these ages, see the Harford et al. reference below.)
The island is very densely vegetated, with most towns clustered around the coast; this also means that the best (old) rock exposures are in sea cliffs. (Hence we spent a lot of mapping time on beaches. Not a bad deal, eh?)
Montserrat from the north, with the Silver Hills in the foreground and the Centre Hills just visible below the clouds. |
When seismic activity (namely earthquake swarms) started happening in 1992, the island was still trying to recover from the damage caused by Hurricane Hugo in 1989. In 1995, phreatic explosions (involving heated groundwater, but no lava eruption) began opening vents in English’s Crater. Ash from larger explosions prompted the evacuation of southern Montserrat in August of 1995, and by November a lava dome began growing in the crater. Since then there have been a number of periods of dome growth and collapse, during which the volcano has built the original lava dome into a large edifice that completely covers the old crater. Dome growth has been accompanied by pyroclastic flows, lahars, and ash venting; occasional periods of explosive eruptions and phreatic activity have occurred.
Dome collapses at Montserrat are impressive, often accompanied by explosions, and can involve anywhere from tens of thousands to millions of cubic meters of material. The most recent occurred in February of this year; you can see video (thermal and normal) at the Montserrat Volcano Observatory website, and I’ll be showing photos of our field trip to the collapse deposits in a later post.
We had the opportunity to spend some time at the Montserrat Volcano Observatory, where the scientists graciously spend time showing us the ropes (and taking us on some great field trips).
The Montserrat Volcano Observatory perched above the Belham Valley. Swanky! |
Examining friction marks on a boulder in the February 2010 deposits. |
In return, we gave lunchtime presentations on subjects relevant to andesitic dome eruptions, and helped map some of the older deposits on the west side of the island. In Smith et al. (2007) – mentioned above – the authors mapped cliffs on the east (old airport) side, but presumably got distracted by the new eruption before they could get to the rest of the island. As part of our class requirement (yes, we got credit for this trip!), we did a survey of sea cliffs on the west side of the island, which meant many long and grueling hours spent on beaches and in boats.
As field locations go, you really can’t beat one that’s steps away from the beach (and the beach bar). |
How could anyone work in these conditions? |
It was a fantastic trip, with great opportunities for seeing old and new products of explosive volcanism (sometimes side by side). The staff at the MVO were very gracious, as was everyone we met on the island. (Perhaps the only downside of the trip was the state of my legs after two weeks of being munched on by tropical mosquitoes; apparently I’m tastier than the majority of the folks who went on the trip.) More discussion to come of the February 2010 collapse, the older volcanics, and how to distinguish different kinds of deposits!
Fascinating!Can I ask, the mentioned friction marks on the boulder, are they intended as caused by a pyroclastic flow overflowing the boulder, or generated trough "grain" impacts during the flow.And if I'm not divagating to much, what are the main distinctions between pyroclastic flow and lahar deposits in the field, are there posibilities to use remote sensing technologies?
David,If I'm remembering correctly, the friction marks are from boulders impacting each other while moving in a pyroclastic flow – they look very similar to slickensides. PF and lahar deposits are actually quite tricky to tell apart sometimes; one of the tells for a lahar deposit is that you can sometimes find "preserved" bubbles (i.e., spherical void spaces) in the matrix where air was trapped during flow. PFs also tend to have only one rock type involved, but that's not a given. I'll do a post later on about the differences (at least for Montserrat; they won't apply everywhere). I'm not sure about whether there would be differences in satellite/aerial data – but that would be a neat thing to look into!
Gee, rough summer.
and i copy your pictureExamining friction marks on a boulder in the February 2010 depositsdont have a zoom one?
the ballistic model of the ejecta create friction marks at all scale's i s'pose that are analysis of the friction of the sliding particleslike the impact marks of eolic grains in sands of sand dunes
Yes, it was a terrible summer :)ODEUSQUERI, I do have close-up photos of the friction marks that I will be putting up in another post – they will be fairly high resolution. Please remember that I've asked people to contact me before using my photos, however!
Please remember that I've asked people to contact me before using my photos, however….only for personal use's …..dont worry..word verification -trapsgeological ones?
How do these recent flows respond to hurricanes (like the one passing through at the moment)?
I suspect with lahars; there was a lot of sediment in the ocean near the February flows, and there were quite a few drainages developing in the deposits.
Jessica,Very fascinating. I am doing research to create a dance to "Vesuvius" by Frank Ticheli. Was wondering if you were aware of any tradition's/ceremonies that were held at the base of Mount Vesuvius. Trying to get inspiration that is authentic and costuming too. Any help would be greatly appreciated.ThanksMillene [email protected]
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Im doing a project of this volcano and Im interested because Im from Puerto Rico nand thats the most nearest volcano,keep up a good work Jessica Ball