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Radiolarite is a , comparatively hard, fine-grained, -like, and homogeneous that is composed predominantly of the microscopic remains of . This term is also used for and sometimes as a synonym of radiolarian earth. However, radiolarian earth is typically regarded by Earth scientists to be the unconsolidated equivalent of a radiolarite. A radiolarian chert is well-bedded, microcrystalline radiolarite that has a well-developed siliceous cement or groundmass.Neuendorf, K.K.E., J.P. Mehl, Jr., and J.A. Jackson, J.A., eds. (2005) Glossary of Geology (5th ed.). Alexandria, Virginia, American Geological Institute. 779 pp.


Mineralogy and petrology
Radiolarites are biogenic, marine, finely layered sedimentary rocks. The layers reveal an interchange of clastic grains, radiolarian tests, carbonates and organic . are usually not abundant. Radiolarites deposited in relatively shallow depths can interleave with carbonate layers. Yet most often radiolarites are pelagic, deep water sediments.

Radiolarites are very brittle rocks and hard to split. They break conchoidally with sharp edges. During weathering they decompose into small, rectangular pieces. The colors range from light (whitish) to dark (black) via red, green and brown hues.

Radiolarites are composed mainly of radiolarian tests and their fragments. The skeletal material consists of amorphous silica (). Radiolarians are marine, with an inner skeleton. Their sizes range from 0.1 to 0.5 millimeters. Amongst their major orders , , the spherical and the hood-shaped can be distinguished.


Sedimentation
According to Takahashi (1983) radiolarians stay for 2 to 6 weeks in the (productive surface layer to 200 meters water depth) before they start sinking.Takahashi, K. and Honjo, S.(1983). Radiolarian skeletons: size, weight, sinking speed, and residence time in tropical pelagic oceans. Deep-Sea Research, 30, p. 543–568 Their descent through 5000 meters of ocean water can take from two weeks to as long as 14 months.Takahashi, K.(1981). Vertical flux, ecology and dissolution of Radiolaria in tropical oceans: implications for the silica cycle. Unpublished Ph.D. Thesis, Woods Hole Oceanographic Institution and Massachusetts Institute of Technology

As soon as the protist dies and starts decaying, silica dissolution affects the skeleton. The dissolution of silica in the oceans parallels the temperature/depth curve and is most effective in the uppermost 750 meters of the , farther below it rapidly diminishes. Upon reaching the sediment/water interface the dissolution drastically increases again. Several centimeters below this interface the dissolution continues also within the sediment, but at a much reduced rate.

It is in fact astonishing that any radiolarian tests survive at all. It is estimated that only as little as one percent of the original skeletal material is preserved in radiolarian oozes. According to Dunbar & Berger (1981)Dunbar, R. B. and W. H. Berger (1981) Fecal pellet flux to modern bottom sediment of Santa Barbara Basin (California) based on sediment trapping,Bulletin of the Geological Society of America, v. 92, pp. 212–218 even this minimal preservation of one percent is merely due to the fact that radiolarians form colonies and that they are occasionally embedded in fecal pellets and other organic aggregates. The organic wrappings act as a protection for the tests (Casey et al. 1979) and spare them from dissolution, but of course speed up the sinking time by a factor of 10.


Diagenesis, compaction and sedimentation rates
After deposition processes start affecting the freshly laid down sediment. The silica skeletons are etched and the original opal A slowly commences to transform into opal CT (opal with crystallites of and ). With increasing temperature and pressure the transformation proceeds to and finally to stable, cryptocrystalline . These phase changes are accompanied by a decrease in of the ooze which becomes manifest as a compaction of the sediment.

The compaction of radiolarites is dependent on their chemical composition and correlates positively with the original SiO2-content. The compaction factor varies generally between 3.2 and 5, which means that 1 meter of consolidated sediment is equivalent to 3.2 to 5 meters of ooze. The alpine radiolarites of the Upper Jurassic for instance show of 7 to 15.5 meters/million years (or 0.007 to 0.0155 millimeters/year), which after compaction is equivalent to 2.2 to 3.1 meters/million years. As a comparison the radiolarites of the Mountains in Greece yield a comparable value of 1.8 to 2.0 meters/million years, whereas the radiolarites of the Eastern Alps have a rather small sedimentation rate of 0.71 meters/million years.Garrison, R. E., and Fischer, A. G., 1969. Deep-Water limestones and radiolarites of the Alpine Jurassic. In Friedman, G. M. (Ed.) Depositional environments in carbonate rocks. Soc. Econ. Palentol. Mineral. Spec. Pübl. 14. 20 According to Iljima et al. 1978 the Triassic radiolarites of central reveal an exceptionally high sedimentation rate of 27 to 34 meters/million years.

non-consolidated radiolarian oozes have sedimentation rates of 1 to 5 meters/million years.De Wever, P., and I. Origlia-Devos; 1982, Datations novelles par les Radiolarites de la serie des Radiolarites s. l. du Pinde-Olonos, (Greece), C. R. Acad. Sc. Paris., 294, p. 399–404 In radiolarian oozes deposited in the equatorial Eastern Atlantic 11.5 meters/million years have been measured. In areas like off the coast extremely high values of 100 meters/million years were reported.


Depth of deposition
The view that radiolarites are strictly deposited under (deep water) conditions cannot be asserted any longer. Layers enriched in radiolarians have been found in shallow water , for example the Solnhofen limestone and the Werkkalk Formation of . What seems to be important for the preservation of radiolarian oozes is that they are deposited well below the storm wave base and below the jets of erosive surface currents.

Radiolarites without any carbonates have most likely been sedimented below the carbonate compensation depth (CCD). Note that due to changing atmospheric CO2 concentrations the CCD has not been stationary in the geological past and is also a function of . At present, the CCD reaches a maximum depth of about 5000 meters near the while being as shallow as 4200 meters in the north Pacific.Berger, W. H. & Winterer, E. L. (1974). Plate stratigraphy and the fluctuating carbonate line. Editors: Hsü, K. J. & Jenkyns, H. C., Spec. Publ. Int. Ass. Sediment. Pelagic sediments: on Land and under the Sea, p. 11–48


Banding and ribbons
The characteristic banding and ribbon-like often observed in radiolarites is primarily due to changing sediment influx, which is secondarily enhanced by diagenetic effects. In the simple two component system clay/silica with constant clay supply the rhythmically changing radiolarian blooms are responsible for creating a clay-chert interlayering. These purely sedimentary differences become enhanced during diagenesis as the silica leaves the clayey layers and migrates towards the opal-rich horizons. Two situations occur: with high silica input and constant clay background sedimentation thick chert layers form. On the other hand, when the silica input is constant and the clay signal varies rhythmically fairly thick clay bands interrupted by thin chert bands accumulate. By adding carbonates as a third component complicated successions can be created, because silica is not only incompatible with clays but also with carbonates. During diagenesis the silica within the carbonate-rich layers starts pinching and coagulates into ribbons, nodules and other irregular concretions. Resulting are complex layering relationships that depend on the initial clay/silica/carbonate ratio and the temporal variations of the single components during sedimentation.


Occurrence in time and space

Paleozoic
The oldest known radiolarites come from the of .Tatiana J. Tolmacheva, Taniel Danelian & Leonid E. Popov. Evidence for 15 m.y. of continuous deep-sea biogenic siliceous sedimentation in early Paleozoic oceans Radiolarian ooze was sedimented here over a time span of 15 million years into the . The deep water sediments were deposited near the paleoequator and are associated with remnants of . The dating has been done with . In more lime-rich sections four radiolarian faunal associations were identified. The oldest, rather impoverished dates back well into the second stage of the Ordovician (Arenigian). The youngest fauna consists already of 15 different taxa and belongs to the fifth stage (Lower Caradocian).Taniel Danelian, Leonid Popov (2003). La biodiversité des radiolaires ordoviciens: regard à partir des données nouvelles et révisées provenant du Kazakhstan. Bulletin de la Société Géologique de France, 174, Nº. 4, p. 325–335, ISSN 0037-9409

During the Middle Ordovician (Upper ) radiolarites were formed near in . Here radiolarian cherts overlie and volcanic rocks. Radiolarites are also found in the nearby where they are associated with .

The Scottish radiolarites are followed by deposits in Newfoundland from the Middle and Upper Ordovician. The red Strong Island Chert for instance rests on .

At the / boundary black cherts (locally called lydites or flinty slates) developed from radiolarians mainly in the Franconian Forest region and in the in .

Of great importance are the from , and which were deposited at the close of the Devonian. The novaculites are milky-white, thinly-bedded cherts of great hardness; they underwent a low-grade metamorphism during the . Their mineralogy consists of with a grain-size of 5 to 35 μm. The microquartz is derived from the sclerae of and the tests of radiolarians.

During the Mississippian black lydites were sedimented in the in Germany.Schwarz, A. (1928). Die Natur des culmischen Kieselschiefers. Abh. senckenberg. naturf. Ges., 41, p. 191–241 The of hosts radiolarites in limestone ,Catalano, R. et al. (1991). Permian circumpacific deep-water faunas from the western Tethys (Sicily, Italy) – New evidences for the position of the Permian Tethys. Palaeogeogr. Palaeocli. Palaeoeco., 87, p. 75–108 at the same period radiolarites have been reported from northwestern ( of the ). Radiolarites from the of date back to the . & Krahl, J. (1987). Erster Nachweis von Radiolarien im tethyalen Perm Europas. N. Jb. Geol. Paläontol. Abh., 174, p. 357–372 The radiolarites from the in closed the end of the Permian.De Wever, P. et al. (1988). Permian age of the radiolarites from the Hawasina nappes. Oman Mountains. Geology, 16, p. 912–914 Towards the end of the radiolarites formed also along the southern margin of near in .Ruttner, A.E. (1991). The southern borderland of Laurasia in NE Iran. Editors: European Union of Geosciences, Strasbourg. Terra Abstracts, 3, p. 256-257


Mesozoic
During the ( and ) cherty, platy limestones are deposited in the , an example being the Hornsteinplattenkalk of the Frauenkogel Formation in the southern of .Lein, R. et al. (1995). Neue Daten zur Geologie des Karawanken-Strassentunnels. Geol. Paläontol. Mitt. Innsbruck, 20, p. 371–387 They are composed of interlayered cherts and separated by irregular, non-planar bedding surfaces. The cherty horizons have originated from radiolarian-rich limestone layers which subsequently underwent silicification. Similar sediments in Greece incorporate layers with calcareous . On local horsts and farther upslope these sediments undergo a change to red, radiolarian-rich, ammonite-bearing limestones.Bosselini, A. & Winterer, E.L. (1975). Pelagic limestone and radiolarite of the Tethyan Mesozoic: A generic model. Geology, 3, p. 279–282 In central Japan clay-rich radiolarites were laid down as bedded cherts in the Upper Triassic. Their depositional environment was a shallow marginal sea with rather high accumulation rates of 30 meters/million years. Besides radiolarians sponge spicules are very prominent in these sediments.Iljima, A. et al. (1978). Shallow-sea, organic origin of the Triassic bedded chert in central Japan. J. of the Faculty of Sci., Univ. of Tokyo, Sec. 2, Vol. XIX, 5, p. 369-400

From the () onwards radiolarites accumulated in the . The onset of the sedimentation was but the end in the rather abrupt. These alpine radiolarites belong to the Ruhpolding Radiolarite Group ( RRG) and are found in the Northern Calcareous Alps and in the of and (Graubünden). Associated are the radiolarites of . The radiolarites of the appear somewhat later towards the end of the Jurassic.

From the Middle Jurassic onwards radiolarites also formed in the domain along the West Coast of , an example being the Franciscan complex. The radiolarites of the Great Valley Sequence are younger and have an Upper Jurassic age.

The radiolarites of are paralleled by radiolarite sedimentation in the equatorial Western Pacific east of the . The accumulation of radiolarian ooze on Jurassic oceanic crust was continuous here from the onward and lasted till the end of the .Ogg, J. G. et al. (1992). 32. Jurassic through early Cretaceous sedimentation history of the central equatorial Pacific and of sites 800 and 801. Proceedings of the Ocean Drilling Program, Scientific Results, 129 The Windalia radiolarite is a () formation in Western Australia. The formation contains abundant , and nanoplankton D. W. Haig, et. al. Mid-Cretaceous calcareous and siliceous microfossils from the basal Gearle Siltstone, Giralia Anticline, Southern Carnarvon Basin, , Volume 20, Issue 1, 1996, pages 41–68 Locally the varicolored to radiolarite is mined and used as an ornamental stone termed mookaite. Mookaite at mindat.org At the same time radiolarites were deposited at the near .

Radiolarites from the Upper Cretaceous can be found in the and in the Troodos Mountains on (). The radiolarites of are very similar to the occurrences on Cyprus and probably have the same age. Red radiolarian clays associated with manganese nodules are reported from , , and .Margolis, S. V. et al. (1978). Fossil manganese nodules from Timor: geochemical and radiochemical evidence for deep-sea origin. Chem. Geol., 21, p. 185-198


Cenozoic
A good example for radiolarites are radiolarian clays from found within the . The group was deposited in the time range till on oceanic crust which is subducting now under the of the .Speed, R. C. & Larue, D. K. (1982). Barbados architecture and implications for accretion. J. geophys. Res., 87, p. 3633–3643 Younger radiolarites are not known – probably because younger radiolarian oozes did not have sufficient time to consolidate.


Use
Radiolarite is a very hard rock and therefore was extensively used in prehistoric technology and has been called the "iron of the Paleolithic". , , and scrapers were manufactured from it. The cutting edges of these tools, however, are somewhat less sharp than .


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