SERPENTINE.
Gebel Korabkansi.
NATURAL SIZE.
Fig. 31.—Olivine-gabbro, Gebel Um Bisilla [11,514], × 10. pl, plagioclase felspar (labradorite); d, altered diallage; o, olivine, altered in places to serpentine (s), with separation of granules of iron oxide.
The main portion of Gebel Um Bisilla is formed of a gabbro [11,514] containing a relatively small proportion of pyroxene and a considerable amount of olivine. In the mass, it is a hard tough rock, consisting of a mixture of white to greenish felspars, showing plagioclastic twinning with the lens, with dull dark minerals, some of a greenish colour and others of a rusty-brown appearance (see [Plate XXIV]). The sp. gr. of the rock is 2·8. The labradorite, which forms about two-thirds of the whole, is very fresh, but is here and there decomposed with formation of calcite along cracks. The pyroxenic constituent is now mostly represented by dusty looking very pale greenish-brown straggling crystals interstitial to the felspars; it appears to have been originally diallage, but is in an advanced stage of alteration, polarising as a confused fibrous mass of hornblende and chlorite, with irregular banding in a direction inclined at about 30° to the general direction of the fibres. The olivine is in large rounded grains, nearly colourless where unaltered, showing the usual irregular cracks; some of the grains are altered to yellowish-green serpentine, with separation of granules of iron oxide.
Fig. 32.—Olivine-gabbro, Gebel Atut [10,365], × 17. o, olivine; a, augite; h, hornblende; f, felspar (labradorite).
Of the fine-grained olivine-gabbros, one of the principal types is the rock of Gebel Atut and Madaret Um Gamil [10,365]. It is a dark heavy rock, weathering into angular blocks with a thin rusty skin, of great hardness and ringing under the hammer. On a fresh fracture, it is seen to be made up of white glassy felspars and dark brownish minerals, some of which have a platey structure with cleavage surfaces which flash as the specimen is turned about in the sunlight. The sp. gr. is 3·01. Microscopic examination shows the rock to be a holocrystalline aggregate of plagioclase (labradorite), augite, hornblende and olivine, with a very little magnetite. The labradorite, which forms about half the rock, is very clear and fresh, in large crystals which frequently show a tendency to idiomorphism. Smaller crystals of labradorite are frequently included in the augite and hornblende. Augite, the next most abundant constituent after the felspar, is present in irregular almost colourless grains with well marked cleavage and numerous irregular cracks, and sometimes slightly clouded. The extinction angles measure up to 36°. The hornblende is in some crystals of a rather pale greenish-brown colour not showing very strong pleochroism, while in others it is more strongly coloured, varying from a rather deep reddish-brown to very pale yellowish-brown when turned over the nicol. The hornblende and augite are frequently associated in such a manner as to suggest that much of the hornblende in the rock originated from alteration of augite. The olivine is fairly abundant in large rounded grains, with the usual blackened irregular cracks; it is mostly fresh, but here and there are patches converted into nearly colourless serpentine with separation of numerous granules of iron oxide.
Fig. 33.—Olivine-gabbro, from a hill eleven kilometres east of Gebel Selaia [10,412], × 17. pl, plagioclase felspar (labradorite); a, augite; hy, hypersthene; o, olivine, with irregular cracks marked by separated magnetite; h, hornblende, enclosing the other minerals and forming a pseudocelephytic border round the olivine and augite. The rock typically contains a somewhat greater proportion of hornblende than appears in the figure.