Jökull


Jökull - 01.12.1989, Side 81

Jökull - 01.12.1989, Side 81
extrusive origin of the silicic Rocks of the kækjuskörð Rhyolitic volcano The extension of the silicic lavas of the Kækju- skörð volcano is shown in Fig. 4. Contrary to the view of Dearnley (1954) who regarded most of the silicic rocks of the Loðmundarfjörður area as intrusive, there are several reasons to believe that the silicic rocks have formed as subaerial lava flows: a. The silicic flows show a zonal structure with an upper, central and basal zone. b- Autobrecciation on top and on the flow fronts is common. c- Updoming of the surrounding basaltic lava flows is nowhere visible at the contact to the rhyolite. Fig. 5a shows a schematic section through a rhy- olitic lava flow, displaying its lithologies. Fig. 5b shows a cross section through the Rocche Rosse obsidian coulée on Lipari Island, southem Italy (Cas andWright, 1987). In the basal zone of a rhyolite flow the rock becomes áutobrecciated under the slowly moving and quickly cooling lava. The central zone is characterized by mostly crystallized rhyolite, so- called "stony rhyolite" (Cas and Wright, 1987). The uPper zone of the rhyolite flow can be the one with the most complicated structure. It is often divided tnto different layers and is intensely folded and brec- ciated. Due to emission of gas from the cooling lava below it often has a pumiceous structure. Autobrec- ciation is typical of the surface, base and front of the highly viscous lava flows. Surface ridges on many rhyolitic lava flows, so- called ogives, are most likely surface manifestations of an intemal ramp structure as shown in Fig. 5b. The layering has been folded in the direction of the flow in concave forms °f amplitudes of 10 to 50 metres (Loney, 1968; MacDonald, 1972; Fink, 1980; Cas and Wright, 1987). Many of the features named above occur in the rhyolitic lavas of the Kækjuskörð volcano. Auto- brecciation is common (Fig. 6), especially on top of the flow and on its front. These upper parts of the lavas are more prone to weathering and erosion than the more solid lower parts and are thus not well preserved. Outcrops of the basal layer are rarely found, because it is usually covered by scree depo- sits. The brecciated areas consist partly of fragments of the stony rhyolite from undemeath and partly of perlitic pieces, pumice and obsidian. The size of the components in the autobrecciated rhyolites is com- monly in the centimetre range. The components are dispersed loosely in a finer matrix, but dense pack- ing without any matrix also occurs. The matrix con- sists of pumiceous puffed up glass, quartz and secon- dary chalcedony. The central part of the lava flows, being the most solid part of a rhyolite flow, often forms prominent cliffs. At Orustukambur, on the southem margin of the Kækjuskörð volcano, good sections through rhyolite lavas are exposed. The sili- cic rocks here form prominent cliffs and ramp struc- tures are clearly visible. The layering of the flow foliation is frequently folded. The size of the folds ranges from several millimetres (Fig. 7) up to tens of metres (Fig. 8) in amplitude. STRUCTURE AND DEVELOPMENT OF THE KÆKJUSKÖRÐ RHYOLITIC VOLCANO The structure of the silicic rocks, as shown above, strongly suggests the existence of a small rhyolitic volcano with its centre in the Kækjuskörð area. This volcano could have had its own magma chamber, but the possibility of its formation as a parasitic cone of either the Dyrfjöll central volcano or the Breiðavík central volcano should also be con- sidered. The extrusive silicic rocks of the volcano can be subdivided into at least four different lava flows and two ignimbrites. The total thickness of the exposed lava pile of the volcano, including a few basaltic lava flows, measures at least 600 m and the volcano covers an area of about 13 km2. Quartz tholeiites and the Orustukambur Ignimbrite I form the base of the Kækjuskörð volcano. In the south this base lies about 350 m above sea-level, in the north about 500 m. Regional variations in the under- lying landscape are probably responsible for this height difference, because there are no signs of a tilt- ing of the complex as a whole to the southwest. JÖKULL, No. 39, 1989 79
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