The Ancient Volcanoes of Great Britain, Volume 2 (of 2)Geikie, Archibald
Science
The Ancient Volcanoes of Great Britain, Volume 2 (of 2)
Geikie, Archibald
Volcanoes -- Great Britain
The most instructive example of the process of devitrification which
has come under my observation occurs in the Eskdale dyke. The central
"cores" already referred to present a true glass, which in thin
sections is perfectly transparent and almost colourless, but by streaks
and curving lines of darker tint shows beautiful flow-structure. The
devitrification of this glass has been accomplished by the development
of crystallites and crystals, which increase in number until all
the vitreous part of the rock disappears. What seems under a low
power to be a structureless or slightly dusty glass can be resolved
with a higher objective into an aggregate of minute globules or
granules (globulites), which average perhaps 1/20,000 of an inch in
diameter. Some of these bodies are elongated and even dichotomous at
the ends. These granules are especially crowded upon clear yellow
dart-shaped rods, which in turn are especially prominent upon crystals
and crystalline grains of augite that bristle with them, while the
immediately surrounding glass has become clear. There can be little
doubt that these rudimentary bodies are stages in the arrested
development of augite crystals. There occur also opaque grains, rods
and trichites, which no doubt consist in whole of magnetite (or other
iron oxide), or are crusted over with that mineral.
At least two broad types of microscopic structure may be recognized
among the basic and intermediate dykes. (1) Holocrystalline, or with
only a trifling proportion of interstitial matter. This type includes
the dolerites and basalts, as well as rocks which German petrographers
would class as diabases or diabase-porphyrites. The rocks are very
generally characterized by ophitic structure, where the lath-shaped
felspars penetrate the augite, and are therefore of an earlier
consolidation. In such cases there is a general absence of any true
interstitial matter. The rocks of this type are often rich in olivine,
and appear to be on the whole considerably more basic than those of
the second group. It is observable that they increase in numbers from
the centre of Scotland westwards, and throughout the region of the
basalt-plateaux they form the prevailing type. (2) In this type there
is a marked proportion of interstitial substance, which is inserted in
wedge-shaped portions among the crystallised constituents ("intersertal
structure" of Rosenbusch). The ophitic structure appears to be absent,
and olivine is either extremely rare or does not occur at all. The
rocks of this group are obviously less basic than those of the other.
They form the large dykes that rise so conspicuously through the South
of Scotland and North of England, and their general characters are well
described by Mr. Teall in the paper already cited. In some instances
they enclose abundant porphyritic felspars of earlier consolidation,
and then present most of the characters of andesites. Professor
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