While minor diamond discoveries were made among alluvial gold in New South
Wales starting in 1851, a discovery in 1979 on the Kimberley Plateau of
Western Australia enabled the country to be the world's most prolific
diamond producer. Based on ancient bedrock, diamond exploration began in
1972, with a kimberlite pipe discovery coming in 1976 in the Ellendale
area. In 1979, a large lamproite pipe was found and named the Argyle mine;
by 1992 over 200 million carats had been mined there. Only 5% of the
production is gem quality. A unique feature of the Argyle mine, though, is
a small but consistent supply of valuable pink to red or purple diamonds.
The Argyle mine on the Kimberley plateau of Western Australia.
Australian Production
Total: 428 million carats Annual: 35-40 million carats
Experiments and the high density of diamonds tell us that they crystallize
at very high pressures. In nature this means that diamonds are created by
geologic processes at great depth within Earth, generally more than 150
kilometers down, in a region beneath the crust known as the mantle. Other
processes, bring diamonds to where people can find them.
The upper mantle is slightly plastic, which allows it to circulate slowly
in a creeping, convective flow that helps drive the surface motion of
Earth known as "plate tectonics." The cross section shown here provides a
closer look at Earth's crust and underlying mantle. The crust can be
divided into ocean basins, underlain by a thin layer of dense, basaltic
rock, and continents, formed of a much thicker but less-dense layer of
granitic rocks. Just below the crust is the portion of the mantle called
the lithosphere, which is rigid and acts like rock. Below this is the
asthenosphere, a more plastic, flowing region that enables the overlying
crustal plates to move in what is known as plate tectonics.
The plot of pressure and temperature shows the conditions at which either
diamond or graphite exist. The general conditions present in the Earth are
described by curved lines called geotherms. Note that there are two
geotherms: Because the continental crust is old and thick, conditions are
somewhat colder in and beneath it than beneath the much younger ocean
basins. Diamonds can form at depths as shallow as 150 kilometers beneath
the continental crust, while beneath oceans they need depths of at least
200 kilometers, as shown by the diamond boundary on the cross-section.
Diamond is amazingly dense. At 3.51 grams per cubic centimeter, it is
vastly more dense than graphite -- the more common form of the light
element carbon -- at 2.20 grams per cubic centimeter. This comparison
offers an important clue to diamond's origin: The fact that diamond is
"squeezed" much denser than graphite, which forms near Earth's surface,
implies formation at high pressure. As shown on the graph, this concept
was corroborated by experimental synthesis of diamond at high pressure and
temperature.
This simplified diagram shows the conditions of pressure and temperature
where diamond and graphite will be the stable forms of carbon. The points
show the conditions at which diamonds were first grown by the companies
ASEA and General Electric in the early 1950s. Temperatures are in Kelvin;
subtract 273 to convert to degrees Celsius. This magnitude of high
pressure is difficult to comprehend. For example, the pressure of 55,000
atmospheres necessary to make a diamond at 1400 degreesC (orange hot)
would require:
The Eiffel Tower (7000 metric tons) resting on a 5 inch plate;
10 Anighito meteorites (10 X 20 metric tons) resting on a 5 cent piece.
Diamonds ascend to Earth's surface in rare molten rock, or magma, that
originates at great depths. Carrying diamonds and other samples from
Earth's mantle, this magma rises and erupts in small but violent
volcanoes. Just beneath such volcanoes is a carrot-shaped "pipe" filled
with volcanic rock, mantle fragments, and some embedded diamonds. The rock
is called kimberlite after the city of Kimberley, South Africa, where the
pipes were first discovered in the 1870s. Another rock that provides
diamonds is lamproite.
The volcano that carries diamond to the surface emanates from deep cracks
and fissures called dikes. It develops its carrot shape near the surface,
when gases separate from the magma, perhaps accompanied by the boiling of
ground water, and a violent supersonic eruption follows. The volcanic cone
formed above the kimberlite pipe is very small in comparison with
volcanoes like Mount St. Helens, but the magma originates at depths at
least 3 times as great. These deep roots enable kimberlite to tap the
source of diamonds.
Magmas are the elevators that bring diamonds to Earth's surface.
Most diamonds consist of primeval carbon from Earth's mantle, but those
from eclogites probably contain carbon recycled from the ocean crust by
plate tectonics -- the carbon of microorganisms. How do we know? Carbon
atoms occur in three different masses, or isotopes. Unlike
high-temperature processes in deep Earth, low- temperature, biological
processes, such as photosynthesis, are sensitive to the differences in
mass, and actively sort different carbon isotopes. Thus, the ratios of
carbon isotopes in organic materials -- plants, animals, and shells --
vary, and also differ from those in the carbon dioxide of the atmosphere
and the oceans. Geochemists "read" the carbon isotopes in samples to
interpret nature's record.
Virtually all carbon atoms, the ones in a diamond or a tree or you, came
from the stars. Particularly at Earth's surface the proportions of 12C and
13C (the carbon isotopes of mass 12 and 13) get redistributed. Expressed
as simple numbers in 13C notation -- in which larger numbers mean more 13C
-- organic carbon has large negative values, average Earth has a mildly
negative value, and the carbon in shells is near zero.
The narrow range of 13C values for harzburgitic diamonds in the histogram
on the top resembles the range of average Earth, indicating that the
mantle is the likely carbon source. The large range for eclogites suggests
mixing of organic carbon (the strongly negative numbers), mantle carbon
(mildly negative numbers), and shell-like carbon (values near zero).
These data support recycling of once-living carbon from Earth's surface
deep into the mantle to form diamond.
When ocean floor slides into the mantle, the basaltic rock becomes
eclogite, and organic carbon in sediments may become diamond.
The search for diamonds has determined that most are derived from
kimberlite pipes in the oldest, nuclear portions of the continents, where
the basement rocks are older than 1.5 billion years.
The oldest parts of continents are called cratons, and can be divided into
two terranes: Archean-age archons, which are older than 2,500 million
years, and Proterozoic-age protons, which are 1,600 -- 2,500 million years
old. The distribution of these terranes is shown on the map.
Kimberlite pipes occur in many parts of the continental crust, but most
diamond-rich ones are found in archons. This fact suggests that most
diamonds were formed and stored deep below the cratons, in the area shown
in the lower figure, and were later transported to the surface by
kimberlite and lamproite magmas that extracted them and other samples from
the mantle.
Kimberlite and Lamprolite
The complex volcanic magmas that solidify into kimberlite and lamproite
are not the source of diamonds, only the elevators that bring them with
other minerals and mantle rocks to Earth's surface. Although rising from
much greater depths than other magmas,
these pipes and volcanic cones are relatively small and rare, but they
erupt in extraordinary supersonic explosions.
Kimberlite and lamproite are similar mixtures of rock material. Their
important constituents include fragments of rock from Earth's mantle,
large crystals, and the crystallized magma that glues the mixture
together. The magmas are very rich in magnesium and volatile compounds
such as water and carbon dioxide. As the volatiles dissolved in the magma
change to gas near Earth's surface, explosive eruptions create the
characteristic carrot- or bowl-shaped pipes.
Kimberlite magma rises through Earth's crust in networks of cracks or
dikes. The pipes only form near Earth's surface. This cross-section of a
kimberlite pipe shows the carrot-shaped profile produced by explosive
eruption. The root zone starts in fissures, where gases are released from
the rising magma and drive the eruption; they blow out the fragment-laden
kimberlite to form the volcano's tuff ring and fill the pipe.
Depth measurements show the level of erosion for various kimberlite pipes
in South Africa. Adapted from Hawthorne (1975).
These drawings illustrate the formation and filling of the typical
champagne-glass shape of a lamproite pipe. The initial stage of the
eruption, powered by gases either from the lamproite magma or from boiling
ground water, corrodes the hosting rock to form the champagne-glass shape
(top). The eruption then produces particles of ash, lapilli, and pumice
that partially fill the crater and form a tuff ring (middle). Finally, the
crater fills with a lava pond from the degassed lamproite magma (bottom).
Adapted from a sketch by Barbara Scott-Smith
Kimberlites are generally much younger than the diamonds they bring to
Earth's surface. Kimberlites and lamproites have been dated between 50 and
1,600 million years old. Diamonds associated with harzburgites are about
3.3 billion years old -- more than two thirds the age of Earth itself, and
those from eclogites generally range from 3 billion to less than 1 billion
years old. These age differences help clarify a picture of diamonds having
crystallized and been stored beneath the ancient continental cratons and
only later being lifted to Earth's surface by kimberlites.
Since inclusion minerals crystallized simultaneously with their diamond
host, the age of the inclusions gives the age of the diamond. The ancient
age of peridotite diamonds suggests that the formation of ancient Archean
continental cores (archons) included diamond crystallization in the
underlying mantle lithosphere. A relatively cool, rigid, deep keel beneath
these continental nuclei provided a stable environment in which diamonds
crystallized and were stored. Subsequently, oceanic crust diving into the
mantle was metamorphosed into eclogite and pasted onto this keel. Much
later passage of kimberlite magmas through the keel dislodged diamonds
from both peridotite and eclogite and sent them to Earth's surface.
This cross-section of continental crust shows the 200-km-thick cool keel
(part of the mantle lithosphere) that provided a stable environment for
diamond crystallization and preservation.
Kimberlites centered over the keel are likely to yield harzburgite-hosted
diamonds from the storage zone (marked with diamonds).
Kimberlites near the edge of the keel are more likely to contain
eclogite-hosted diamonds, while those off the keel are likely to be barren
of diamonds.
Geologic processes create two basic types of diamond deposits, referred to
as primary and secondary sources. Primary sources are the kimberlite and
lamproite pipes that raise diamonds from Earth's mantle, where they
originate. Secondary sources, created by erosion, include such deposits as
surface scatterings around a pipe, concentrations in river channels, and
fluxes from rivers moved by wave action along ocean coasts, past and
present. Mining of these deposits depends upon sufficient concentration
and quality of diamonds.
The diagram here shows the trail of diamonds left by geological processes.
The primary deposits, or diamond pipes, are the vertical portion. The
flared top of the pipes can yield substantial quantities of diamonds, but
following the narrowing pipe downward eventually becomes unprofitable.
Note how erosion of the landscape moves surface minerals -- including the
diamonds -- from the pipes down hills, streams, and rivers to their
ultimate destination, the ocean.
Because diamonds are dense they concentrate at the bottom of active zones
of moving sand and gravel. These secondary deposits are eluvial Ð above a
pipe, colluvial -- adjacent to a pipe, alluvial Ð stream and river
transported, and marine -- along beaches that can wind up onshore or
offshore with changing sea level. Secondary deposits may be found far from
active means of transport, in the fossilized channels of now-vanished
rivers or under fossil beaches.
The diamond octahedron has the shape that we describe as a diamond. While
it is the most common shape for a diamond crystal, cubes, dodecahedra, and
combinations of these three shapes are common. All are highly symmetrical,
with equal dimensions in three perpendicular directions, and all are
manifestations of the cubic crystal system to which the mineral diamond
belongs.
Exceptions are the flat form called a macle, which is a twin, or composite
crystal, as if mirrored across the middle, and etched crystals, with
rounded surfaces and, sometimes, elongated shapes. The shapes of diamond
crystals can be very intriguing.
These triangles result from subtle changes in height on a diamond's
octahedron face and are called trigons. The trigons shown here are
indentations, probably produced by natural etching of the crystal. The
image was created with Nomarski differential interference contrast
microscopy and is 0.29 mm across.
Xenoliths - hitchikers from the center of the
earth
Kimberlite magmas carry foreign rocks -- xenoliths -- from Earth's mantle
to the surface. Xenoliths are geologists' only samples from the deep
Earth, and carry information about diamond growth conditions.
The 2 most common types of xenoliths are peridotites and eclogites. Peridotite is the main constituent of the mantle beneath the crust
and consists primarily of olivine -- the gem variety is peridot. Eclogite, consisting primarily of garnet and a green pyroxene, is
formed by plate tectonics when basalt of the ocean crust founders into the
mantle. Certain kinds of xenoliths contain diamonds.
These diagrams show the compositions of mantle xenoliths. Lherzolite is a variety of peridotite thought to form most of the
upper mantle.
Harzburgite is another kind of peridotite with less clinopyroxene.
Garnet harzburgites contain red garnet and, occasionally, diamonds.
Eclogite, a very different rock, consists of garnet and sodium-rich
pyroxene; some also contains diamonds.
Diamond inclusions
Diamonds with inclusions are like little space capsules from the mantle:
pristine mineral samples are protected by the diamond's indomitable
embrace and transported to the surface by a volcanic rocket.
Inclusions capture a picture of the rock and environment in which diamonds
grow and indicate that garnet harzburgite (a type of peridotite) and
eclogite are the most common rocks in which diamonds have grown.
A single mineral inclusion rarely defines a specific rock, but two or more
minerals may enable interpretation of rock associations and origin. Some
inclusion minerals are virtually unique to diamond sources and are thus
sought in the exploration for diamonds.
A purple pyrope garnet, an indicator of garnet harzburgite, in a brownish
diamond octahedron from the Udachnaya pipe, Sakha Republic, Russia (about
0.8 mm across).
Certain minerals are present in the rocks from the upper mantle that occur
with diamonds in kimberlite and lamproite pipes, as seen in nearby cases
of xenoliths and diamond inclusions. Some of these minerals, being
resistant to weathering and denser than quartz sand, concentrate in
channel bottoms. Because they occur in far greater abundance than diamond,
exploration geologists look for these "indicators" among the gravel of
regions they suspect may host diamond-bearing pipes.
Indicator minerals for diamond include, in order of decreasing
significance: garnet, chromite, ilmenite, clinopyroxene, olivine, and
zircon. But the order of persistence in streams is zircon, ilmenite,
chromite, garnet, chromian diopside, and olivine. Diamond itself is
obviously a most important indicator.
Most indicator minerals have a distinctive color. Seen here are red pyrope
garnets, green chromian clinopyroxene, black ilmenite and chromite, and
yellowish-green olivine.
Mining of a diamond-bearing pipe starts with the excavation of a pit into
the pipe. In this process, called "open-pit" or "open-cast" mining, the
initially loose and eventually hard ore material is removed with large
hydraulic shovels and ore trucks. Hard rock is drilled and blasted with
explosives so the broken material can be removed. When deep, rich ore
warrants it, the mining goes underground with vertical shafts descending
to horizontal drifts, or passageways that enter the pipe.
A cross section of the underground workings at the Dutoitspan mine,
Kimberley, South Africa. Adapted from De Beers
In bedrock adjacent to the pipe, shafts are sunk and drifts are tunneled
into the pipe. The highly mechanized and efficient method known as block
caving is shown in the adjacent model. Concrete-lined tunnels are
excavated under a large vertical section, perhaps 140 to 180 meters (400
to 600 feet) of kimberlite.
Along the tunnels are draw points, or openings in the concrete casing
where kimberlite is drilled and blasted to cave in a section above the
tunnel. Broken kimberlite falls through the draw points and is scraped out
of the tunnel with a drag or scraper bucket attached to a cable and winch,
working much like a clothes line on a pulley.
The kimberlite above the tunnels falls under its own weight and leads to a
slow, continuous caving of ground that is removed through the draw points.
The scraped kimberlite rubble is loaded into cars on a lower level and
moved to a crusher underground. The crushed ore is then conveyed to skips
that carry the ore up the vertical shaft for processing.
In the last 20 years scientists have discovered new sources of diamond.
Continental collisions -- a result of plate tectonics -- can subject
slices of a crust to immense burial and uplift. In Kazakhstan, for
example, diamonds formed in buried crust that returned to Earth's surface.
Meteor impacts produce immense pressures, and diamonds can be formed and
sprayed among the impact debris. Meteorites also experience impacts
themselves and can contain diamonds. And the most ancient meteorite
material contains star dust, the remnants of the death of stars. Some of
this star dust is extremely tiny bits of diamond, just big enough to be
crystals and older than the solar system itself.
Very small "microdiamonds," averaging only 12 micrometers across,
were discovered during diamond exploration in a region called the
Kokchetav Massif, in northern Kazakhstan, in large slices of metamorphic
rock that must have been pushed at least 120 kilometers deep into Earth
and returned.
Discovery of this process, termed ultrahigh pressure (UHP) metamorphism,
has revolutionized ideas about and interest in what can happen to Earth's
crust. Recently scientists have found traces of diamond around meteor
impacts.
Cartoon of the formation of a UHP terrane that can yield diamonds. At top,
the down-going subducted ocean crust (green) has a thin covering of
sediment (gray) that is sheared off and driven upward (inset), apparently
caused by the continental collision (middle) that squeezes the
diamond-bearing metamorphic rocks back into the crust (bottom).
At the 35-million-year-old Popigai crater in Siberia, graphite transformed
into microdiamond aggregates up to 1 centimeter across. It is now
suspected that diamonds form in most major impacts, becoming a new
indicator of ancient cosmic collisions. In 1987, microscopically small
fragments of diamond, called "nanodiamonds," were recovered from
meteorites that predate the solar system. New studies indicate that they
formed more than 5 billion years ago in flashes of radiation from dying
red-giant stars into surrounding clouds of methane-rich gas. The process
is essentially the same as the new process for growing synthetic diamond
called CVD -- chemical vapor deposition.
Most of the diamond deposits first discovered were alluvial --
concentrations in streambed or riverbed sand and gravel. They are still
actively exploited in many ways, from the most primitive to the highly
sophisticated. The goal is relatively simple: to find a location where
moving water has deposited diamonds in the bottom of a channel, possibly
in a pocket or cleft. Because rivers meander and drainage can change,
fossilizing a once active river, the search for alluvial diamonds requires
some geological knowledge and a lot of luck. The process involves removing
the overlying barren ground, digging up the bearing ground, extracting the
diamonds, and, nowadays, restoring the landscape when finished.
In the most basic, individual operations, such as in Sierra Leone or
Angola, the technology involves shovel and pan, with some hand sloshing to
gravitate diamond to the bottom of the pan; the eye is the ultimate
sorting device. Mom-and-pop operations in South Africa involve a small
claim and utilize limited technology -- shovels, buckets, jury-rigged
cranes powered by small vehicles, and the like -- to load a small washing
pan. The concentrate is then sieved into several size ranges, and each
fraction is dumped onto a picking table, where someone checks by eye for
diamonds. In the bigger operations, as shown in the model, large
earth-moving equipment transports the alluvium, and the processing
approaches that of the primary mines -- coarse sieving, then rotary
sieving in a trommel, before loading into a large washing pan. Final
processing includes concentrate sieving, a picking table, and usually a
grease table. Of course, no crushing is required, as nature has already
released the diamonds from the pipe rock.
Once a mining operation yields ore, the diamonds must be sorted from the
other materials. This process relies primarily on diamond's high density.
An old but effective method is to use a washing pan, which forces heavy
minerals like diamond to the bottom and waste to the top. Cones and
cyclones use swirling heavy fluids mixed with crushed ore to achieve
density separations. With 99 percent of the waste in the ore removed,
further separations may use either a grease table or an x-ray separator.
Final separation and sorting is done by eye.
Crushed ore is mixed with a muddy water suspension, called puddle,
and all is stirred by angled rotating blades in the circular washing pan.
Heavier minerals settle to the bottom and are pushed toward an exit point,
while lighter waste rises to the top and overflows as a separate stream of
material.
A working grease table at Longlands, Cape Province, South Africa. The
surface of diamond is highly unusual in that it resists being wetted by
water but sticks readily to grease. Here, wet gravel washes across 3
inclined surfaces covered with beeswax and paraffin. Diamonds stick to the
grease while wetted waste minerals flow past. The operator routinely
scrapes the material that adheres to the table into a grease pot, using a
trowel. The grease in the pot is melted and the diamonds are removed in a
strainer. More automated systems use a rotating grease belt and scraper.
Cones (left) and cyclones (right) use heavy-media separation.
Diamond-bearing concentrate is mixed with a fluid near the density of
diamond. Separation occurs in cones and cyclones by swirling the mixture
at low and high velocities respectively.In the cone, rotational mixing
permits lighter minerals to float to the top and run out as overflow,
while diamonds and dense minerals sink to the bottom and are sucked out
with a compressed air siphon.
In the cyclone, fast rotation of the suspension drives heavy minerals to
the conical wall, where they sink to the bottom and are extracted, while
float waste minerals are sucked from the center of the vortex. Cyclones
are about 99.999% efficient at concentrating diamonds and similarly dense
minerals from the original ore. Adapted from Bruton (1978)
The x-ray separator system acts on a thin stream of particles from the
concentrate accelerated off a moving belt into the air, where they
encounter an intense beam of x-rays. Any diamond fluoresces in the x-rays,
activating a photomultiplier that triggers a jet of air, deflecting the
diamonds (blue) into a collector bin. Adapted from Bruton (1978)
There are two aspects of moving diamonds from mine to dealer. The first is
the fairly straightforward but important task of separating diamonds into
gem-quality, near gem-quality, and industrial-grade diamonds. The second
is the more intriguing aspect: the primary diamond marketing, which has
been and still is largely controlled by De Beers Consolidated Mines, Ltd.
through its majority control of the Central Selling Organization (CSO).
The CSO sells a large percentage of mine production to diamond dealers;
independent mines sell by closed bids and through private transactions.
Sorting small diamonds in a Botswanan operation.
Sorting occurs at every level of the market, from the mine to the jeweler.
At the mine, the sorting depends on the sophistication of the operation
and the size of production, but it is always based on grouping stones of
like type. Diamonds are grouped into "sizes" -- more than one carat;
"smalls" -- between 1 carat and 1/10th carat; and "sand," -- less than
1/10th carat, with some leeway for market pressures.
Diamonds larger than about 15 carats are handled individually. Shape
groups comprise "stones," "shapes," "cleavages," "macles," and "flats,"
describing characteristics familiar to the market. The ultimate purpose of
sorting is to estimate an asking price for the rough diamonds.
After great swings in diamond prices, the Diamond Trading
Corporation (DTC) was set up by De Beers in 1934 to handle the actual
sales of diamonds. The DTC and the Diamond Producers' Association (the
mine operators) form the nucleus of the Central Selling Organization. The
CSO stabilizes prices in hard times and raises them in accord with
inflation and demand during good times. It needs considerable wealth and
stockpiles of diamonds to maintain this position, but this "single channel
marketing" system has been an effective cartel. In the United States
cartels are illegal, so De Beers cannot operate here. However, the
company's interests are represented by a public relations office, the
Diamond Information Center, and indirectly by the diamond dealers and
jewelers who sell the gems.
Marine deposits are a variation on alluvial deposits. They result from the
wave action of the ocean, which has concentrated diamonds at the base of
the surf zone. Waves arriving at an angle to the coast tend to push the
diamonds along the coast, causing the diamonds to stream out from where
rivers deposited them at the coastline. Moreover, changes in climate have
led to great variations in sea level -- hence movement of diamond
concentrations to both old beaches well up on land and others now more
than 100 meters below sea level.
There are 3 types of marine mining operations. In one, sand is moved
from 10 meters below sea level to as far inland as the sea may have risen,
in order to reveal the concentrations on the bedrock. In another, divers
and boats work in the surf zone to perhaps 20 meters of water and use
suction pipes to remove gravel and diamonds from the ocean floor. In the
third, deep-sea marine vessels use remote underwater tractors or large
underwater excavators to remove overlying sediments and extract the
diamond-bearing sand and gravel. Processing is done on land in the first 2
cases and shipboard on the large mining vessels.
Wave refraction maps like this one for concession 2(b) along the
South African coast are used to assist in locating concentrations of
diamonds. The map shows where the wave force is maximized, and thus where
diamonds will have been concentrated by wave action. Wave power is
transformed into the visible spectrum, so that blue represents weak and
red strong power.
With much of Canada underlain by ancient bedrock, the existence of
diamond-bearing kimberlite has been considered very likely, particularly
with tantalizing diamonds found in Wisconsin in deposits swept down by
glaciers from up north. Now the country is home to the latest major
diamond discovery.
Intermittent exploration for kimberlites by major companies was
unsuccessful through the 1980s. But Chuck Fipke, head of Dia Met Minerals,
persevered and in April 1990 located a kimberlite under Point Lake.
Eventually, his company, with partner BHP Minerals, found more than 100
kimberlites on their claims; 42 contain diamonds. Five small pipes, to be
operated as if they were one mine, are scheduled to start production in
the second half of 1998.
The first kimberlite pipe discovered in the Northwest Territories is under
Point Lake. The top of the kimberlite lies about 50 m below the surface of
the lake, which is 600 m wide.