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| SEM
of volcanic opal |
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| unusual
layering |
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| great
artesian basin |
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FORMATION OF
OPAL |
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Sedimentary
opal fields |
| Opal encountered in the
sedimentary opal fields, especially of the
type occurring in Australia, is clearly
formed by colloidal processes. Precious
opal itself is a special case of this process,
and comprises only a very small fraction
of the opal in these areas. The microstructure
of small spheres is now well known,
especially the regular stacking of uniform
particles in the gemstone.
The key factor in these cases is the ultimate
origin of the silica itself. In Australia,
the opal deposits occur in soft siliceous
claystones of Cretaceous age which are overlain
by further siliceous deposits which have
undergone intensive weathering. The mobilisation
of silica is evidenced by the formation
of silicified duricrusts and hard siliceous
bands at various levels beneath the surface.
It is believed that in times of higher rainfall,
the silica, both in true solution and as
finely dispersed colloid, was carried downwards
through the porous beds by percolating water.
At a certain point the water encountered
beds composed mainly of clay minerals which
were much less permeable, especially to
colloid particles.
This gave time for the primary particles
of silica, perhaps 10-20 nm diameter, to
coagulate or grow to larger sizes. Additional
silica in solution would also be polymerised
with the help of the abundant electrolytes,
especially calcium and aluminium sulphates,
which were also present in this environment.
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Any cavities,
open veins, or gaps caused by minor
faulting (called 'slides' in the mines)
would gradually be filled by the growing
silica spheres; they would, in effect,
be filtered out by the semi-permeable
membrane formed by clay layers.
The spheres would themselves settle
very slowly, and, under quiescent
conditions, form horizontal layers.
The water level will be determined
by surface precipitation, and, from
time to time, may dry out underground.
This may favour the development of
potch by accelerating the deposition
of the colloidal silica. The layering
could also be disturbed by minor pressure
movements in the sediments. Partially
filled cavities appear to be uncommon
in the opal-bearing horizons, but
they do occasionally occur.
This is illustrated in a
specimen from the conglomerate
layer opal level of Andamooka. A cavity
is partly filled with opal, the lower
part showing diffraction colours.
The surface of the opal is white and
opaque, and shows cracking due to
more rapid drying of the opaline material
at the surface. The surface of the
opal was horizontal when the specimen
was in situ.
In most cases, irregular growth rates,
ground movement, changing concentrations
of silica and other factors would
result in variable sphere size, and
random accumulation. Most of the material
deposited would therefore form the
typical potch opal found on all opal
fields. |
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Under the most favourable conditions of
accumulation uniform spheres form and settle
into a regular packed structure. Six sets
of conditions would be necessary to achieve
this:
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Quiescent
conditions |
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Uniform
concentration of silica in the form
of the primary colloid particles. |
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Slow
and uniform aggregation of these particles. |
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Aggregation
to a size suitable for optical diffraction
effects to occur when solidified. |
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Slow
settling of the spheres under conditions
to allow them to pack in a regular
fashion. |
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Slow
removal of water, in the first place
by absorption by underlying clay,
and finally by slow drying. |
It is clear that a combination of such
sets of conditions would be rare; this is
certainly confirmed by the limited occurrence
of gem quality opal in the opal fields.
Nevertheless, such conditions do occur occasionally
over vast areas of country, especially that
covering the Cretaceous beds of the Great
Artesian Basin of Australia.
These basic conditions must also hold in
other areas where precious opal deposits
are found in what are essentially sedimentary
environments. The important opal fields
of the Pedro Secundo area of Piaui State
in northeastern Brazil appear to have similar
environmental conditions for the formation
and deposition of opal.
While the actual host rocks are of volcanic
origin, they are, in fact, brecciated and
precede the formation of the opal. They
have evidently been subject to later leaching,
the silica having then been carried downwards
and deposited in a similar manner to the
opal in the Australian fields. This no doubt
also applies to the American deposits at
Rainbow Ridge, Nevada.
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