Radiolarite is a Siliceous ooze, comparatively hard, fine-grained, chert-like, and homogeneous sedimentary rock that is composed predominantly of the microscopic remains of radiolarians. This term is also used for Friability 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.
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 (opal). Radiolarians are marine, protists with an inner skeleton. Their sizes range from 0.1 to 0.5 millimeters. Amongst their major orders albaillellaria, ectinaria, the spherical spumellaria and the hood-shaped nassellaria can be distinguished.
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 water column, 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.
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 sedimentary rock 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 Pindos 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 Japan reveal an exceptionally high sedimentation rate of 27 to 34 meters/million years.
Holocene 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 upwelling areas like off the coast extremely high values of 100 meters/million years were reported.
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 latitude. At present, the CCD reaches a maximum depth of about 5000 meters near the equator 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
During the Middle Ordovician (Upper Darriwilian) radiolarites were formed near Ballantrae in Scotland. Here radiolarian cherts overlie and volcanic rocks. Radiolarites are also found in the nearby Southern Uplands where they are associated with pillow lava.
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 Silurian/Devonian boundary black cherts (locally called lydites or flinty slates) developed from radiolarians mainly in the Franconian Forest region and in the Vogtland in Germany.
Of great importance are the from Arkansas, Oklahoma and Texas 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 Ouachita orogeny. Their mineralogy consists of quartz with a grain-size of 5 to 35 μm. The microquartz is derived from the sclerae of sponges and the tests of radiolarians.
During the Mississippian black lydites were sedimented in the Rhenish Massif in Germany.Schwarz, A. (1928). Die Natur des culmischen Kieselschiefers. Abh. senckenberg. naturf. Ges., 41, p. 191–241 The Permian of Sicily 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 Turkey (Karakaya complex of the Pontic Mountains). Radiolarites from the Phyllite of Crete date back to the Guadalupian.Heinz Kozur & Krahl, J. (1987). Erster Nachweis von Radiolarien im tethyalen Perm Europas. N. Jb. Geol. Paläontol. Abh., 174, p. 357–372 The radiolarites from the Hawasina nappes in Oman 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 Paleozoic radiolarites formed also along the southern margin of Laurasia near Mashad in Iran.Ruttner, A.E. (1991). The southern borderland of Laurasia in NE Iran. Editors: European Union of Geosciences, Strasbourg. Terra Abstracts, 3, p. 256-257
From the Bajocian (Jurassic) onwards radiolarites accumulated in the Alps. The onset of the sedimentation was diachronous but the end in the Tithonian rather abrupt. These alpine radiolarites belong to the Ruhpolding Radiolarite Group ( RRG) and are found in the Northern Calcareous Alps and in the Penninic of France and Switzerland (Graubünden). Associated are the radiolarites of Corsica. The radiolarites of the Apennines appear somewhat later towards the end of the Jurassic.
From the Middle Jurassic onwards radiolarites also formed in the Pacific domain along the West Coast of North America, an example being the Franciscan complex. The radiolarites of the Great Valley Sequence are younger and have an Upper Jurassic age.
The radiolarites of California are paralleled by radiolarite sedimentation in the equatorial Western Pacific east of the Mariana Trench. The accumulation of radiolarian ooze on Jurassic oceanic crust was continuous here from the Callovian onward and lasted till the end of the Valanginian.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 Cretaceous (Aptian) formation in Western Australia. The formation contains abundant foraminifera, radiolaria and calcareous 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 Chalcedony radiolarite is mined and used as an ornamental stone termed mookaite. Mookaite at mindat.org At the same time radiolarites were deposited at the Marin Headlands near San Francisco.
Radiolarites from the Upper Cretaceous can be found in the Zagros Mountains and in the Troodos Mountains on Cyprus (Campanian). The radiolarites of Syria are very similar to the occurrences on Cyprus and probably have the same age. Red radiolarian clays associated with manganese nodules are reported from Borneo, Roti, Seram and Timor.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
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Paleozoic
Mesozoic
Cenozoic
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