Looking from the sky at diamonds

When a geologist looks at Google Maps images, we usually filter out any human activity. But in the case of mines, that would be a mistake – the holes humans dig can tell us about the geology.

What’s this? A big circular hole in the ground and large piles of bluish mine waste. The shadows are on the northern side, showing we are in the Southern hemisphere. This is the Letlhakane mine in Botswana.

And here’s another one, in the northern hemisphere. The hole here is half a kilometre deep (it’s an older mine, the Mirny mine in Siberia. They used jet engines to melt the soil so they could dig).

And again, the Diavik mine in Canada. Note that the hole is considerably deeper than the lake it sits in. They really wanted to dig that hole and yet most of the its contents are sitting in those big blue piles.

Finally the oldest example in the world, the Big Hole in Kimberley. The piles of dirt were put back in the hole, or covered in houses. Mining underneath here reached a kilometre depth.

We’ve been looking at some famous diamond mines. Diamonds form deep in the earth and those worth digging holes for only reach the surface via weird fizzy molten rock called kimberlite. This magma zips up from 100km depth to the surface in only hours. Travelling at depth along a narrow crack (or dyke in geo-speak1) when the magma reaches the surface it forms a carrot-shaped pipe. The magma solidifies, peppered with diamonds that formed at depth and were pulled up inside it.

The pipe is circular in cross-section, so as the miners dig out the kimberlite they leave a circular hole. The vast majority of what is dug out is waste – only the precious diamonds are extracted. Kimberlite is bluish in colour, as you can see from the piles of it above.

The Big Hole in Kimberley was the first kimberlite pipe ever identified2, in the 19th Century. Diamonds found before then were from placer deposits, river gravels that contain diamonds eroded out of kimberlite pipes. Diamond placer deposits were first discovered in India and then Brazil. But the biggest area for modern mining is on Namibia’s Skeleton Coast.

Southern Africa’s Orange river rises on the Kapvaal Craton, an area rich in kimberlite pipes. For 100 million years it has flowed across the continent into the Atlantic ocean, leaving thick placer deposits. These have since been pushed around since by wind and ocean waves to cover a wide area.

Starting at the beginning of the Twentieth Century, German settlers found diamonds and the government designated a huge area of land as Sperrgebiet – forbidden territory. This whole area remains closed, but active mining is concentrated the southern end, on the coast, where the diamonds are concentrated in ancient beach sands.

The mine here looks very different from the others, no round hole or blue kimberlite (but look for the regular patterns on the spoil heaps). Like the other mines, this one was caused by the desire for the beauty and strength of diamonds.

Categories: diamonds, Great Geology in Google earth

Great Geology in Google Maps: mapping from above

In most cases, geological maps are made by piecing together observations of hundreds of individual outcrops. Boundaries between types of rock are covered in grass and sheep1 and have to be traced on the map later as a line between rock outcrops, like a inverted game of dot-to-dot. In areas like Himalayas the same boundaries may be visible in an instant on a vast wall of rock. Quickly mapping vast areas of country by tracing features by eye across expanses of bare rock is a great way to do geological mapping.

It turns out you can have a go at this ‘Himalayan-style’ mapping at home. Make a cup of tea (add salted butter, or spiced sweet milk for authenticity) and fire up Google Maps. It works outside the Himalayas too – deserts are great for this.

This is an area of Namibia in SW Africa. Immediately you can see different areas of rock – the image itself is like a geological map, only without labels. Himalayan geologists would identify the different areas of rock by getting samples, but we’ll stick with Googling the geology of the area.

Let me take you through the geological components and their history.

First off, the orange lines that look like rivers. Ignore them: they are rivers and we are geologists, not geographers. Mentally filter them out of the image.

damaraNext look at the stripy area top left – we’ll call them the Damara sediments. They formed in the long-vanished Khomas ocean between the Congo craton (ancient piece of crust) and the Kalahari craton. The area is stripy because the sedimentary layers are not flat. They are now on edge and form ridges on the surface.
dgraniteThe light orange area far right is made of Damara granites (and modern sand, again filter it out, if you can). These formed when the Khomas ocean closed and Congo and Kalahari got stuck together as part of Gondwanaland. This happened about half a billion years ago.

KarooBottom left, the rusty brown area is sediments and volcanic rocks that are part of the Karoo Supergroup. These formed on Gondwanaland between the Carboniferous and the Jurassic when geological conditions in this part of Africa were relatively calm.

Brandburg3

The really obvious round thing that I’ve perversely left until last is a circular granite intrusion called Brandberg that formed a little later, as Gondwanaland was ripped apart and the South Atlantic opened.

 

I’ve given you the relative ages of the different rock packages, but we could have worked this out from Google Maps. The observations I’ll show you are exactly the same as those used by field geologists. What follows are a sequence of close-ups. Some are outside of the original area, but none are far away.

Unconformity

We’ve got two areas of sediments, the Damara and the Karoo. How do we know one is older than the other?

Here we see the red-brown Karoo sitting in a blob in the middle, with stripy purple-brown Damara to the NE. Look carefully (zooooming helps) and you can see circular lines in the Karoo. Note that the rivers go round this blob.

We are looking at a hill of Karoo sediments. The lines are the edges of different beds and they are tracing contours around the hill. These are flat layers of underformed sandstone2.

Try tracing the lines in the Damara – these are also the edges of sediment beds but they have been tilted. Note that they are cut by the edge of the Karoo. The surface between the two rock packages is an unconformity. It represents the time when the Damara sediments were pushed into a mountain belt and then eroded into a flat surface.

Folding and cross-cutting granites


This is a view of the contact between the Damara granites and the Damara sediments, which have some zig-zaggedy folding here. The boundary between the two is fairly abrupt and cuts the folded bedding planes. Using the principle of cross-cutting relationships the granite is younger than the sediments and the folding (although the folding may be related to the emplacment of the granite). There are some fine white lines crossing the folded sediments that may be veins of magma that came out of the main granite – further evidence of what came first.

Scoot around a bit and you can see that there is an unconformity between this older Damara granite and the Karoo, which gives us the relative ages of the three.

Three-way contact


This is a view of three of our rock packages. There’s a prominent river forming a yellow bar across the picture. Apart from that, from left to right we have: Damara sediments; Karoo sediments, sitting above the unconformity; the Brandberg granite. The boundary between the Karoo and the Brandberg is straight and cuts across bedding, suggesting the intrusion is later.

Another possibility to consider is that this is an older granite and the edge is just the edge of a hill. Well, look a the patterns of the streams – they are flowing down from the centre of the granite (it actually forms the biggest mountain in Namibia). For it to be higher now than the flat Karoo sediments, it must be younger than them.

The boundary between the Brandberg and the Karoo is quite interesting3, with tilting of the Karoo and a zone where the sediments and granite are mixed. Apart from the small zone that is Karoo coloured but without clear bedding, I can’t make this out.

The geological history I started with is based on many things, including precise dating of events and detailed field work. However, the basic age-relationships between the rocks can be worked out using simple geological rules and good photographs.

These same principles are being used on other planets where geologists have never been. We know a lot about the geological history of Mars by mapping from space using just these techniques.

Damara granite next to folded Damara

Categories: Great Geology in Google earth, sediments

Hot spot volcanoes: no plumes required?

It’s a simple and well-known picture. Volcanoes form either at plate boundaries due to subduction or inside plates due to mantle plumes. Invoking plumes – columns of hot rock rising from deep in the mantle – is an awfully useful way of explaining oddly-placed volcanoes, both ancient and modern.

Too useful, many people think. The concept has been abused. See Erik Lundin’s excellent critique in “52 things you should know about Geology“: “A concept that is granted the freedom of perpetual ad hoc amendments has the ability to  explain anything … But such a concept can neither be falsified not used predictively. In the long run it may be wiser to ask  yourself ‘Is there an alternative explanation?’ rather than simply shrugging, ‘Plumes do that’.

mt-noora-16

Layers of volcanic debris and ash from the Newer Volcanics Province, Australia. Spot the bombs. With permission from Stephanie Sykora

How else to melt the mantle?

The best place to find alternative explanations is mantleplumes.org a site dedicated to “discussing the origin of “hotspot” volcanism”. The site lists many mechanisms, but I’m going to focus on just two: edge-driven convection and shear-driven upwelling.

It’s not that hard to melt the mantle. It’s everywhere fairly close to its melting point and it gets hotter the deeper you go. A key point to understand is that most of it only stays solid because of the intense pressure it is under. As mantle quickly rises up beneath mid-ocean ridges it melts because it stays hot as the pressure reduces. All the atoms that were squeezed tightly together in solid crystal lattices manage to break free into a liquid state,  once the earth’s grip lessens a little.

Almost all matter behaves like this, but it doesn’t feel like common sense because we are most familiar with the freezing and melting of water, which is weird and works the opposite way round (which is why ice floats). I labour the point because both of today’s mechanisms are ways of creating upwellings1 – areas where hot mantle material rises up and so is prone to melting.

Edge-driven convection (EDC) is flow caused around the edges of continents. Continents have deep cold roots to them, like icebergs2. A convection cell is set up with a zone of upwelling about 600km from the craton edge. It wouldn’t be surprising if you find some volcanic rocks above here.

EDGEFig2_500

Diagram showing edge-driven convection. Reproduced with permission from mantleplumes.org

The above model assumes nothing is moving, but we know that there will often be flow of the mantle relative to the plates. If there is mantle flow across an edge (for example a craton edge) then material will flow up. This is one way of producing shear-driven upwellings (SDU)3

SCUFig1_600

Diagram showing mechanisms of shear-driven upwelling. I discuss the left-hand example. Taken with permission from mantleplumes.org.

So far, so theoretical. Let’s go to Australia and look at some rocks.

Welling-up down-under

The Newer Volcanics Province is an active (but dormant) volcanic area in Victoria, Australia. To get a great overview of its many great volcanic features, check out this post (from which the photos here come). The lava is basaltic in composition – just what you’d expect from melting of mantle, but we are a long way from a plate boundary.

A recent paper in Geology studies what’s going on deep beneath the lava. Rhodri Davies and Nicholas Rawlinson of ANU, Canberra and Aberdeen universities start off with a spot of 3-D seismic tomography. Previous workers through they could dimly see a plume beneath, but armed with a new seismic data set from the (wonderfully-named) WOMBAT project they show there is no plume. Instead they show a shallow low-velocity anomaly underneath the NVP, consistent with region of hotter mantle, perhaps containing a small proportion of magma.

"Volcanic bomb with a olivine-rich xenoliths from the mantle at Mt. Noorat – Victoria, Australia" Courtesy of Stephanie Sykora

A piece of mantle that flowed upwards and melted: “Volcanic bomb with a olivine-rich xenoliths from the mantle at Mt. Noorat – Victoria, Australia” Courtesy of Stephanie Sykora

Having made the plume vanish, they turn to modelling of the mantle flow, based on their new improved knowledge of what is down there.

This area of Australia sits outside of the deep cratonic root. It’s like a thin ledge sticking out from the side of the iceberg. Therefore the edge of the deep root, that might cause EDC is to the north, allowing the upward return flow to sit directly beneath the NVP. Their models also include relative plate motion  (how the plate is moving relative to the mantle beneath). This allows them to model the effects of SDU as well.

The modelling results produce a region of upwelling with velocities between 1 and 2 cm a year – fast moving for mantle – sitting directly underneath the NVP. This neatly explains the NVP, without any need to invoke plumes.

The mechanism is neat, but begs the question as to why there isn’t a line of volcanoes all around cratonic roots. Addressing this question, they point out the interaction of SDU and EDC. Under the NVP the two effects are complimentary – upwelling is increased where the mantle is flowing away from step. Also the edge here isn’t straight – 3D effects are important. Finally, mantle composition varies. So-called ‘fertile’ mantle may melt under conditions where mantle that’s already had melt extracted would not.

Are plumes dead?

There’s a compelling model here for explaining many volcanic hot-spots around the world with no need for plumes. Do we need plumes at all? Gillian Foulger, the force behind mantleplumes.org certainly doesn’t think so. Also Don Anderson of Caltech who recently had the posthumous last word at the AGU annual meeting last year.

Their views may prevail in time, but for the moment most of us still believe in plumes. Explaining how small-scale convection causes a minor volcanic field in one place doesn’t explain continental flood basalts like the Deccan or Siberian Traps. You know, the ones that cause mass extinctions and thickly cover vast areas.

But clearly plumes and not the only game in town. To progress, ideas involving plumes need to be anchored in our understanding of the deep earth, to be falsifiable and have predictive power. Recent research aims to do just that. Watch this space.

References

Davies D.R. (2014). On the origin of recent intraplate volcanism in Australia, Geology, 42 (12) 1031-1034. DOI: http://dx.doi.org/10.1130/g36093.1

Categories: Deep earth

Great Geology in Google Maps: dunes

Google Maps is a great resource, particularly in satellite view. My favourite way to enjoy it is via the Chrome extension “Earth View from Google Maps“. This pops up a gorgeous image in every new tab. Many show human landscapes, but every now and then one appears that catches this geologist’s eye. This post is the first in a series exploring and celebrating these images.

This view is of the Rub’ al Khali or ‘Empty Quarter’ of the Arabian Peninsula – the largest sand desert in the world.

In dry environments sand is moved not by water but by wind. The characteristic landform is the sand dune. Common in deserts on earth, they are also found on Mars and even comets.
The shapes of dunes depends on the supply of sand, but above all the wind. Wind strength and direction, averaged over the year, will determine the shape of a dune. Various types of dune are recognised. The ones in this image are complex. Further east of here the dunes are clearly linear features, but here the lines are broken up into loops reminiscent of arabic script.

Look carefully and you’ll see that there are dunes upon dunes. The surface of the large sand bodies are covered in ridges and patterns with a wide variety of shapes. These themselves may have small ripples on, only visible if you visit in person.
 

This image is from the ‘Grand Erg Oriental’ in the Sahara desert in Algeria. It shows star dunes, which form when the wind is variable and simply piles the sand up into mounds 100s metres tall.

Both these areas of sand (by chance) sit above oil-fields, the oil-bearing rocks sitting deep under the ground. Ancient desert sands are of interest to oil geologists as the grains are very round and form sandstones that can contain a lot of liquid.
Ancient ‘aeolian sandstones’ are basically fossilised sand dunes and are often red. The ‘red sandstones’ of the UK, much Triassic sandstone in Europe and the classic Navajo Sandstone in the US are of this type.

Next time you see a red sandstone with big swooping cross bedding, think of these pictures.

Categories: Great Geology in Google earth, sediments