Cornwall: tin, pasties and the world

The county of Cornwall is like England’s foot, stretching out languorously into the warm waters of the Gulf Stream1. Now a relatively poor area, best known for fishing and tourism, it has a proud industrial past based on mining, notably of tin. Once the most important thing about Britain, Cornish tin is now distributed across the world. The up and downs of mining also scattered Cornish miners globally. If you look in the right places in the right ways, traces of both can still be found.

If you took a chunk of rock and analysed it, atom by atom, you’d find most elements inside it somewhere. In order to have a rock that is an ore, of interest to miners, it must contain enough of what you want so that it can be extracted commerciallyTherefore the formation of ore deposits is often associated with processes that take specific elements from large volumes of rock and put them into much smaller volumes. Granites, which are common in Cornwall, are good at doing this. As granite intrusions cool, water that was within the magma, or from the surrounding rocks, is heated and flows widely. Hot water is good at dissolving and transporting certain elements. At some point this hot water cools and the elements dissolved within it are precipitated out, often into fractures called veins. In places around the Cornish granites there are veins rich in cassiterite – tin oxide.

South Crofty Tin mine in Cornwall. Phone from exnottsminer under CC

South Crofty Tin mine in Cornwall. Photo from exnottsminer under CC

Cornwall’s tin travels far

The Bronze Age (in Europe 3000 BC to 500 BC) saw extensive trade networks develop across Europe. The technology of smelting copper and tin to form a durable alloy is first seen around the copper deposits of Cyprus. The warm Mediterranean world had few tin deposits, forcing them to trade with cold barbarian lands to the North. We know that from 2000 BC tin mining started in Cornwall, initially focusing on alluvial deposits (river gravels containing ore).

The Phoenicians, a now vanished pre-Roman civilisation in North Africa, traded directly with Cornwall. The name “Britain” comes from the Phoenician name “Baratanac”, meaning “Land of Tin”. The Greek historian Herodotus, who is the source for much of the little we know about the ancient world, describes how tin comes from the Cassiterides, ‘lands of tin’ that sat beyond Gaul (France). It’s thought that the Phoenicians, who managed the trade, might have been a little cagey about the exact whereabouts of this economically valuable land.

When great military powers invade far-off lands, there are always people who say that their true motivation was to get access to valuable natural resources. We don’t know of any ancient Romans waving banners saying ‘No Blood for Tin’ when Julius Caesar invaded Britain, but modern historians have suggested Cornwall’s tin deposits were a motive.

Given the lack of documentary sources for these ancient periods of history, its obvious that archaeology has a role to play. A recent paper used the black arts of isotope chemistry to study ancient tin. The isotopes within metals can be used to uniquely characterise where they came from2: the different geological settings leave a distinctive isotopic signature. Despite having an impressive 10 different isotopes it’s proved relatively difficult to do this with tin, but the authors have shown that a Bronze Age artifact in central Europe (the “Himmelsscheibe von Nebra” or sky disc of Nebra) contains tin  from Cornwall.

Bronze Age metal disc from Germany, containing Cornish tin. Image from Wikipedia

Bronze Age metal disc from Germany, containing Cornish tin. Image from Wikipedia

Another recent scientific study looks at Cornish bogs. By studying metal concentrations in layers within the bog, they can trace when mining was active. Local smelting would spread tin through the environment to be captured in the bogs. From this evidence they suggest that there was only a little mining before the Roman period and that the arrival of the Romans, with their Southern European work ethic and trading mindset3 greatly increased the rate of mining.

To get this direct evidence of the ancient movements of Cornish tin takes big machines run by dedicated scholars. Evidence of the movement of Cornish miners in the Nineteenth Century is easier to find, and tastier too.

Pasties – a world tour

The Cornish pasty, now protected by the full might of European Law, is a folded and crimped pastry circle containing beef, potato, onion and swede. It was popular with the tin miners, as it was a convenient meal that could be eaten with dirty hands.

Cornish pasty. Image from  Hammer 51012 under CC as I couldn't be bothered to take my own picture of one.

Cornish pasty. Image from Hammer 51012 under CC as I couldn’t be bothered to take my own picture of one.

The potato reminds us that this is not a Bronze Age dish. In many ways the pasties heyday was the Nineteenth Century, which was also a big time for Cornish mining. By this time all the surface ore had been found and miners were digging down deep, following the veins into the earth. Mining in Cornwall had its peak in the early 19th Century. The Royal Geological Society of Cornwall was founded in 1814 and is the second oldest in the world. Mining terms such as vug and gossan are Cornish in origin.

The mid-Nineteenth Century saw Cornish mining start on a slow but terminal decline as massive deposits were opened up in Bolivia and East Asia. As work dried up, tens of thousands of Cornish miners emigrated to new mining districts across the world, where their skills were in great demand. A Cornish saying of the time said that “a mine is a hole anywhere in the world with at least one Cornishman at the bottom of it!”4

Some went to America. The Californian gold rush of 1850s attracted many Cornishmen and Cornish Pasties are still found for sale in the Sierra Nevada to this day. Others went to the iron and copper districts of northern Michigan and also left pasties behind5.

They reached South Africa and Australia, but also non-English speaking countries such as Mexico and Brazil. They are credited with bringing football (“soccer”) to Mexico and also the ubiquitous pasty. Mexicans may add hot chili sauce to theirs, which would be frowned on in Penzance, but they did open the world’s first Cornish Pasty museum in 2011.

The business of mining and the shipping of raw materials is not glamorous, but it is important. Our civilisation depends on technology that needs particular materials, whether the tin in a Bronze Age sword or the rare metals in your mobile phone. Written histories, often created by politicians or the winners of wars, sometimes overlook the importance of such lowly matters. The study of objects, whether metallic or cultural, can help redress the balance a little.

Categories: England, geochemistry, History

The Grampian / Taconic orogeny in Ireland – when arcs attack

Ever since the plate tectonic paradigm-shift of the 1960s, geologists have strived to understand ancient rocks in terms of the movements of plates. The geology of north-western Ireland can be explained by what happened when a subduction zone ran out of oceanic crust back in the Ordovician. Let me take you back to before that happened.

Imagine you are floating in the sea. In 480 million years time the crust below will be in Ireland. The sea is warm – CO2 levels are high and you are fewer than 30° south of the equator. Apart from cheeky trilobites nibbling your toes, it is an idyllic place to be. You are near a large land-mass. It’s barren looking  - plants are just about to learn how to survive outside the sea 1 so there is little to soften the landscape. The tumbler of gin and tonic2 you clumsily dropped has sunk into sediment that will one day be part of the Dalradian Supergroup.

Your mood has soured. Not only has your drink gone, but you’re getting creeped out by the cloud on the horizon out to sea. It’s not a fluffy, friendly one but a dark spreading plume of volcanic ash. Far out to sea, there is a line of volcanoes and they spell D-O-O-M for the peaceful spot you’ve found. Every year the volcanic arc gets a little bit nearer. Eventually it will smash into the continent behind you, grinding over the top. The peaceful sand and mud washing around below your feet will be sediment no more. The collision between the volcanic arc and the continent will transform the Dalradian sediments into the contorted metamorphic rocks that today make up much of NW Ireland.

An accident waiting to happen

Here’s a diagram showing a section through the land below. Black is oceanic crust, yellow stippled is sediment3.

x-section 1 geo labels

Let’s start from the left. Notice that the edge of the continent is thin and tapering – it was stretched out when the ocean basin formed. The oceanic crust attached to the continent is being stuffed down back into the deep earth. As it sinks, it is squashed and heated, starting a complex process that ends with molten rock reaching the surface. Over time this magma has formed a volcanic arc, a small piece of thickened crust.

This situation can’t last for ever. Once all of the oceanic crust of the lower plate has run out, normal subduction comes to an end. The upper plate slides over the thinned continental margin and ends up lying on top of the continent – a process called obduction. The island arc and forearc basin are squashed against the continent. Like a bulldozer hitting a pile of sand, the arc collision compresses and thickens the crust. The Dalradian sediments become thoroughly deformed and heated and are now a wildly complex set of schists and marbles.  This process creates a mountain belt, an event known as the Grampian orogeny.

As shown in the diagram below 4, the orogeny does not stop plate convergence. The old subduction zone has been destroyed, but another one is created in the opposite direction. This process, called ‘subduction flip’ changed the tectonic stress regime; it’s believed to have led to a process of ‘orogenic collapse’ whereby the thickened crust extends and thins, bringing metamorphism to an end. The overall tectonic event was remarkably quick, around 15 million years.

x-section 2 base

Where are they now?

This type of orogeny can be recognised as it leaves distinctive rock types behind. Ophiolites, pieces of oceanic crust within continents are found in several places in Ireland; the largest example is the Tyrone ophiolite, but traces of oceanic crust can also be found in Mayo, near Westport, in the Clew Bay and Deerpark Complexes. The story goes that there are no snakes in Ireland because Saint Patrick, while fasting on top of Croagh Patrick, threw them down into Clew Bay. That the sea-facing side of the mountain contains a lot of green serpentinite suggests the origins of the story have a geological angle5.

ireland grampian map

Map of NW Ireland. Red – continental basement, Yellow-Dalradian, Blue – lower-mid Ordovician volcanics, Brown – Ordovician sediments, purple serpentinite & melange. Data from Geological Survey of Ireland, displayed using Google Earth

Parts of the volcanic arc can now be found around Lough Nafooey, just to the south of the South Mayo trough, which corresponds to the fore-arc basin. The Dalradian sediments and underlying older crust make up most of the land to the north west of these rocks.
Let’s revisit the cross-sections, labelling the modern day equivalents. Before the collision:

x-section 1 geograph labels

and immediately afterwards:

cross section of Grampian orogeny

A wider context

Ireland was only a small section of a continental margin that stretched from rocks now in Greenland down into the eastern US and Canada. The Grampian orogeny also affected Scotland and the same arc-collision event is found in eastern Northern America where it is known as the Taconic orogeny. 

Figure 1 from Hollis et al. 2012

Figure 1 from Hollis et al. 2012

Recognising the connection across the Atlantic helped geologists understand the causes of these complicated patterns in the rocks – different sections show different parts of the orogeny and synthesising research across a wider area leads to a richer understanding. The patterns are complex – more so than I’ve shown above. There were probably multiple ‘accretion events’ where different arcs collided at different times. The pattern of plates in modern day SE Asia is seen as an analogy here – they may have been multiple subduction zones and arcs within the wider ocean.

Geological is 4-dimensional, and the Grampian/Taconic orogeny reminds us of this. The timing of the various accretion events varies because the edge of the continent was not straight. Promontories (sticky-out bits) were hit by the arc sooner than parts where there was more oceanic crust to be consumed. Another complication is that continents don’t break cleanly: fragments of continental crust can end up far from the main continent (for example Rockall in the Atlantic). The arc whose collision caused the Grampian orogeny in Scotland (now found buried in the Midland Valley) is thought to sit on continental crust.

These 15 million years were a very important time for the crust of the northern half of Ireland, but are only a small part of the wider geological history of Ireland. I’ll leave the story unfinished here and tell you what happened when the new subduction zone ran out of oceanic crust in future posts.

References

RYAN, P., & DEWEY, J. (1991). A geological and tectonic cross-section of the Caledonides of western Ireland Journal of the Geological Society, 148 (1), 173-180 DOI: 10.1144/gsjgs.148.1.0173
Hollis, S., Roberts, S., Cooper, M., Earls, G., Herrington, R., Condon, D., Cooper, M., Archibald, S., & Piercey, S. (2012). Episodic arc-ophiolite emplacement and the growth of continental margins: Late accretion in the Northern Irish sector of the Grampian-Taconic orogeny Geological Society of America Bulletin, 124 (11-12), 1702-1723 DOI: 10.1130/B30619.1
Bird, A., Thirlwall, M., Strachan, R., & Manning, C. (2013). Lu-Hf and Sm-Nd dating of metamorphic garnet: evidence for multiple accretion events during the Caledonian orogeny in Scotland Journal of the Geological Society, 170 (2), 301-317 DOI: 10.1144/jgs2012-083

Categories: Ireland, metamorphism, mountains, subduction, tectonics

Scandinavian crust now in Alaska!

The face of the earth is ever changing. Plate tectonics is slowly but surely rearranging the locations and inter-connections of continents. However knowing this in the abstract doesn’t prepare you for the awed surprise of discovering that a section of crust formed in Scandinavia is now found in Alaska.

The evidence for this comes from a massive accretion of data from geologists across the world. Build up a geological history, underpinned by accurate dating, for enough parts of the world and you can start correlating ancient events. Other tools area palaeomagnetic studies that can tell the you the latitude of a piece of crust at a given time and suites of fossils that trace small areas where organisms with local characteristics were found.

The latest research (Beranek et al. 2013) uses most of these techniques to nail down the link between a portion of Alaska and rocks now in Northern Scandinavia. It’s long been known that Alaska and Pacific Canada is made up of portions of crust (terranes) that formed elsewhere. The portion in question, the Alexander terrane is not small, covering 100000 km2 from British Columbia up into Alaska. Here’s where they reckon this crust was half a billion years ago:

Figure 12 from Beranek et al. 2013

Figure 12 from Beranek et al. 2013

The area labelled Laurentia corresponds to North America today, Baltica to Scandinavia. Arctic Alaska and Farewell are other terranes now found a long way from home. If you’ve read my post about rotating continents, you’ll have spotted the way Baltica dramatically swings round.

How did these terranes get round to the other side of Laurentia/North America?

Figure 11 from Colpron & Nelson 2009.

Figure 11 from Colpron & Nelson 2011. AX = Alexander terrane

This figure from Colpron & Nelson (2009) shows how. We are 50 million years further on from above. Baltica and Laurentia are now fused together, the ‘Caledonides’ – a strip of fascinatingly deformed rocks – mark where they collided. The  narrow subduction zone to the north of this area will over time pull itself forward, dragging the continental fragments over the top of Laurentia. A similar process is going on today in the Caribbean, where the Caribbean Arc is moving east, pulling ‘Pacific’ rocks further towards the Atlantic Ocean.

Ultimately these fragments end up plastered onto western Northern America in the area known as the Cordillera, waiting for cunning geologists to spot their true origins. I don’t know about you, but my flabber is well and truly gasted by this, by both the fact that it happened and that we can work out that it did so.

Colpron, M., & Nelson, J. (2009). A Palaeozoic Northwest Passage: incursion of Caledonian, Baltican and Siberian terranes into eastern Panthalassa, and the early evolution of the North American Cordillera Geological Society, London, Special Publications, 318 (1), 273-307 DOI: 10.1144/SP318.10
Beranek, L., van Staal, C., McClelland, W., Israel, S., & Mihalynuk, M. (2013). Baltican crustal provenance for Cambrian-Ordovician sandstones of the Alexander terrane, North American Cordillera: evidence from detrital zircon U-Pb geochronology and Hf isotope geochemistry Journal of the Geological Society, 170 (1), 7-18 DOI: 10.1144/jgs2012-028

Categories: mountains, tectonics

When continents rotate

The earth’s surface is not fixed. Oceans come and go and continents are constantly moving, breaking up and reforming like blobs of oil on the surface of a stock-pot.

Since tectonic plates are not flat (they collectively form the surface of the not-flat earth), their movement over the surface of the earth is best described as a rotation. Just as maps are distortions of the global globe-like reality, so most diagrams of plate tectonics ignore the rotational possibilities. Nonetheless, the complicated reality of plate movements over hundreds of millions of years has created some startling examples of spinning continents.

Sutherland in Scotland is a fabulous place, and has long been a geological nursery for budding geologists. Its name means ‘South-land’ in Norse, as the Viking influence  was strong. Appropriately there are strong links with the geology of Sutherland and that of Scandinavia. The phase of deformation that formed the classic Moine Thrust is linked with the Scandian orogeny, the phase of mountain building that dominates the geology of Norway.

A recent open-source paper (Bergh et al. 2012) makes a more striking connection – between the ancient Lewisian Gneiss and basement rocks of similar age from near Tromsø in Arctic Norway. I went there recently and, believe me, it’s a long way from Scotland. The paper lists surveys the geological history of both areas and finds many similarities. It suggests that were part of the same orogenic belt 1.83 billion years ago, as shown in this diagram.

fig 22 Bergh et al

As is usual in such figures, the lines of modern day coasts are used to allow correlation with modern day geography. The rocks of modern-day NW Scotland correspond to the area labelled LEWISIAN, whereas the LOFOTEN and WTBC rocks are now in Arctic Norway. The outline of Scandinavia is close to its modern-day orientation, whereas Greenland and Atlantic Canada (“Laurentia”) are upside down, to our eyes.

How did we get from there to our modern-day situation?

Let’s jump forward a billion years or so.

Cocks&Torsvik2006-550

Firstly, we are now in the southern hemisphere. Secondly, Laurentia is in a more ‘normal’ configuration – the shape of Greenland is easier to pick out. The ‘Scandinavian block’ has rotated around 180° in the same way. An ocean, called Iapetus has formed between  our Norwegian rocks (marked with a little red T) and our Scottish ones (an L).

By the late Ordovician, the Iapetus ocean was closing again and Baltica is returning to collide again with Laurentia, only by now it has rotated by 180°. Again.

Ordovician plate configuration

 

Soon Iapetus closes, causing the Scandian orogeny which glues together the rocks of Baltica and Laurentia. Our Scottish and Arctic rocks become fixed back into a single continent. The rotation of Baltica while it wandered off means that entire length of Norway now separates two areas of crust that once were next to each other.

The Atlantic ocean has formed since then, of course, but along a line slightly different to that of Iapetus, so now the ‘Laurentian’ rocks of North west Scotland (and Ireland) are separated from similar rocks in Canada and Greenland. Will they be reunited in the future or will future continental rotations keep them apart? Only time will tell.

References

The last two diagrams are figure 2 and figure 7 from Cocks and Torsvik (2006)

Steffen G. Bergh, Fernando Corfu, Per Inge Myhre, Kåre Kullerud, Paul E.B. Armitage, Klaas B. Zwaan, Erling K. Ravna, Robert E. Holdsworth, & Anupam Chattopadhya (2012). Was the Precambrian Basement of Western Troms and Lofoten-Vesterålen in Northern Norway Linked to the Lewisian of Scotland? A Comparison of Crustal Components, Tectonic Evolution and Amalgamation History Tectonics – Recent Advances, Prof. Evgenii Sharkov (Ed.), ISBN: 978-953-51-0675-3 DOI: 10.5772/48257

Cocks, L., & Torsvik, T. (2006). European geography in a global context from the Vendian to the end of the Palaeozoic Geological Society, London, Memoirs, 32 (1), 83-95 DOI: 10.1144/GSL.MEM.2006.032.01.05

Categories: Uncategorized