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illite (1)
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isotopes
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metal ores
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GeoRef Categories
Era and Period
Epoch and Age
Book Series
Date
Availability
Origin and diagenesis of lacustrine sediments, upper Oligocene Creede Formation, southwestern Colorado Available to Purchase
Magnesium-rich clays of the meerschaum mines in the Amboseli Basin, Tanzania and Kenya Available to Purchase
Hydrogeologic control on zeolitic diagenesis of the White River sequence Available to Purchase
Clay mineral diagenesis in core KM-3 of Searles Lake, California Available to Purchase
Globule ignimbrite of Mount Suswa, Kenya Available to Purchase
The uppermost of the globule ignimbrite sheets of Mount Suswa in Kenya covers an area of about 300 km 2 and ranges in thickness from 25 cm to 2.5 m. It is welded and devitrified and exhibits gas-phase crystallization to an extent that is unusual for a sheet as thin as this. Most of the ignimbrite is composed of rounded ash particles, and the fine-ash fraction consists largely of ovoid and spherical globules. In the basal vitrophyric zone the globules are mostly nonvesicular and 20 to 75 μm in diameter, but in the devitrified part of the sheet they are inflated to form bubbles. Lapilli in the vitrophyric zone are chiefly of obsidian, which is inflated to form pumice in the devitrified zone. Most of the obsidian is characterized by a wavy banding, some of which is a relict welded tuff texture. We have no satisfactory explanation for the banded globules, which originated neither from melting of cuspate shards, nor condensation from vaporized magma, nor in a spray or fountaining of magma. Many of the globules exhibit undeformed banding similar to that in the obsidian, indicating that they originated in essentially their present shape either from larger particles such as lapilli or from a partially remelted welded tuff that yielded both lapilli and ash. Welded-tuff textures in the obsidian lapilli are also difficult to explain and seem to indicate a complex eruptive or emplacement process, which could possibly involve discharge of molten agglutinate from an earlier eruption.
Nature and Origin of Palagonite Tuffs of the Honolulu Group on Oahu, Hawaii Available to Purchase
Tephra deposits of the Honolulu Group on Oahu are middle to late Pleistocene and range from alkali basalt to melilite nephelinite. Some of the deposits are fresh, but most of them are zeolitic palagonite tuff. Where the most complete thicknesses of pyroclastic deposits are preserved, they are generally zoned from clayey soil 3 to 8 feet thick, down into relatively fresh tuff from 15 to 40 feet thick, which is underlain by palagonite tuffs as much as, or more than, 60 feet thick. The contact between fresh and palagonite tuff of Koko Crater roughly parallels the present deeply gullied land surface and indicates that the palagonite was formed long after the cone. The amount of authigenic minerals in tuffs is generally proportional to the amount of palagonite and indicates that minerals are related to the palagonitization process. The principal authigenic minerals were deposited in the following sequence, from first to last: phillipsite, chabazite, thomsonite, gonnardite, natrolite, analcime, montmorillonite together with opal, and calcite. Chemical analyses of sideromelane and associated palagonite by the electron microprobe show that about a third of the SiO2, half of the A12O3, and three quarters or more of the CaO, Na 2 O, and K 2 O are lost when sideromelane is converted to an equal volume of palagonite. A substantial proportion of these components lost from the sideromelane are precipitated nearby as zeolite, montmorillonite, opal, or calcite cement. Reaction of sideromelane with cold percolating ground water accounts for the vertical zoning from a surface layer of relatively fresh tuffs down into palagonite tuffs. The p H and ionic strength of percolating water probably increases with depth by solution and hydrolysis of glass, and where the p H and ionic strength become sufficiently high, the glass reacts to form palagonite and zeolites. A high p H probably accounts for the mobility of aluminum as reflected in its loss from palagonitized glass and its precipitation in zeolites. As support for a p H control of aluminum mobility, aluminum has remained immobile in palagonitic alteration of sideromelane pumice of the Pahala Ash on Hawaii. This pumice is presently weathering to palagonite in the soil profile, which contains water having a p H of 5 to 6. The sharp interface between unaltered sideromelane and palagonite suggests that palagonite was formed by a microsolution-precipitation mechanism rather than by simple hydration and devitrification. Rainfall, grain size, permeability, and original composition are important factors in determining the degree of palagonitic alteration, nature of the authigenic mineral assemblages, and crystal habit of phillipsite on Oahu.