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concretion of opal
volcanic rocks
minute platy crystals
'lepispheres'
FORMATION OF OPAL

Common Opal

The glassy or semi-glassy form of opal with conchoidal fracture, which is so commonly encountered in nature, for example,, is usually found by XRD analysis to be opal-CT. It occurs under a wide variety of conditions, ranging from nodules formed in cavities in volcanic rocks, probably at a later stage in the cooling process, to concretions in unconsolidated sedimentary beds clearly formed close to the surface. In addition, friable opal-CT is formed in large quantities by diagenesis, especially in deep sea deposits of biogenic silica.

As has been indicated earlier, opal-CT is a crystalline material, albeit with a highly disordered structure. This was first described last century by Mallard (R1589) using optical microscopy. He noted that certain types of what were apparently opal showed a birefringent fibrous structure when viewed in thin section between crossed polarisers; he termed this material 'lussatite', a term which is again being recognised as useful. This phenomenon has been noted frequently in various forms since then.

More recently actual crystals of what appears to be the same material were encountered in cavities in solid common opal. These can just be seen by optical microscopy, but scanning electron microscopy shows that they take the form of minute platelets coating the surfaces of the cavities.

Similar coatings of crystallites were even encountered in the lumina of silicified woods (Scurfield and the author, R0658). The same types of crystals were identified later as a common constituent of deep sea siliceous sediments, where they developed more or less spherical accumulations of these platelets; these have been termed 'lepispheres'.

Lepispheres are well illustrated by Weaver and Wise (R1368), who referred to them as cristobalite. Oehler (R0919) was able to reproduce these lepispheres in the laboratory, but partly in view of their habit, favoured a structural interpretation similar to that proposed by Jones and the author (R0242), i.e., disordered interlayering of cristobalite and tridymite structures (opal-CT).

The widespread marine deposits of opaline silica have been extensively studied in recent years by means of deep sea drilling from ocean-going vessels. Silica deposits ranging from diatoms and radiolarian oozes composed largely of opal-A, through opal-CT to porcelanites and cherts have been encountered.

The primary deposition of these deposits is largely due to biogenic processes. Minute marine organisms such as those mentioned, as well as sponges and other creatures, have siliceous skeletons, which, when the animal dies, can settle to the bottom of the ocean. The actual situation, however, is more complex.

Numerous studies have been made on the deposition of silica on the ocean floors, based in part on the origin of the silica itself. These studies are summarised by Oehler (R0919). Diatoms alone are estimated to extract some 2.5 x 1016 grams of silica annually from near surface waters, but only some 3% - 5% of this reaches the ocean floor by settling of the skeletons of the organisms. Most of the silica is redissolved and rendered available in a virtually closed cycle for these organisms.

Larger particles, such as those formed in sponges, are more likely to be preserved, but will ultimately be subjected to the diagenetic processes taking place in the sea floor deposits. Oehler considers, on the basis of experimental and observational evidence on the formation of opal lepispheres, that:

"it appears that the conversion of biogenic silica (opal-A) to opal-CT occurs principally, if not exclusively, through a solution-reprecipitation mechanism."

A further factor which appears to have an influence on the genesis of the opal-CT is the chemical environment under which diagenesis takes place. The pore water in the sediments is essentially saturated with silica, and thus plays an important intermediate part in the development of new phases. It is suggested that the inhibition of pore water movement in clay-rich sediments may favour the formation of opal-CT rather than quartz.

Lancelot (R1639) and Greenwood (R0205) found that silica tended to form opal-CT in clayey sediments, but in carbonate sediments, where, presumably pore water is saturated in calcium carbonate, quartz appears to be the favoured form.

In general, the transformations found in deep sea siliceous sediments tend to follow the diagenetic sequence:

opal-A --> opal-CT --> quartz