Some petrographic Anomalies with relations to the Silca strewnfield Norbert
Brügge, Germany 1. Silica glass components in breccias from the Qaret-el-Hanash structure (Kimberlite pipe)
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"There
is a very strange exposure of megascopic breccia observed during the expedition
of November/December 1996, at latitude 25� 22�51″ N and longitude 25� 27�
34″ E. The exposure is of about 2-m high above the surrounding level. The
exposure represents remnant of an eroded section. To the north, this rock
has been replaced by ferruginous breccia and iron deposit. The petrographical and mineralogical studies carried out on the breccia indicate that it represents impact breccia. In addition to the brecciation of the quartz grains some of these grains show PFs and PDFs. The zircon of this breccia shows evidence of deformation as represented by the fragmented nature of some the studied grains and by non-stoichiometric contents of ZrO2 and SiO2". The detection of glass and graphite is accounted also for the impact origin of this breccia. |
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4.
Magnetite spherules MAGNETIC COSMIC (?)
SPHERULES FROM THE GREAT SAND SEA (WESTERN DESERT, EGYPT) Comment: The spherules are certainly not micrometeorites, but aeolian or fluvial reprocessed material from subvolcanic hotspots with iron and magnetite deposits in the Great Sand Sea. |
5. Magnetite float Flickering flames over the Libyan Desert ? |
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6. Magnetic Ferro-Basalt |
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Detected augite ferrobasalt
at northeastern site auf Kemal-el-Din plateau It was found a porphyritic, fine-grained igneous rock dominated by phenocrysts of olivine (30 vol% pheno) and augite in a groundmass of augite, abundant magnetite, minor plagioclase and nepheline. Olivine phenocrysts form colourless, euhedral crystals up to 2 mm in size and are partly altered to red brown iddingsite. Augite phenocrysts are euhedral crystals up to 1 mm in size and often contain magnetite inclusions. The groundmass consists of subhedral brown augite, small laths of plagioclase and euhedral magnetite. Nepheline occurs as areas of nepheline. Specimen is a primitive basalt dominated by olivine and pyroxene with very little plagioclase. Minor amounts of nepheline indicate this is a silica undersaturated alkali basalt. Enough magnetite is present in the sample to make it highly magnetic. Rock Library, Imperial College London, Author: Matt Genge (2017) |
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7. The unusual meteorite GSS-020 5420 grams of a supposed meteorite found in 2000. But only 396 grams of it were examined and classified as Chondrite (H). After studying of the published mineral chemistry, I come to the conclusion that the chondrite GSS-020 is none. The matrix is clearly a remelted mix of material from the Earth' mantle. The Fe-Mg silicate matrix with the mineral relics and metal inclusions are not a criterion to postulate an extra-terrestrial origin. Fe-Mg silicates occur in a mixed series (enstatite and ferrosilicate) and are for example part of peridotite. |
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"The GSS-020 chondrite is an unusual non-brecciated melt rock. On a <1 cm scale the melt portion is texturally homogenous and extends throughout the whole meteorite. GSS-020 is a fine-grained rock composed of about 66 vol% melt rock matrix, 16 vol% relictic silicate objects, 9.5 vol% opaques (mainly mm to submm-sized metal/sulfide grains), and 8.5 vol% numerous homogeneously distributed voids (on average < 0.3 mm in size). Microscopically, the major part of the silicate fraction is matrix material that clearly shows the texture of a quenched melt consisting of about 57 vol% Fe-Mg silicates and 9 vol% glass. Relictic olivine and low-Ca pyroxene (16 vol%) are present as isolated grains in the quenched melt matrix and as unmelted remnants in �ghost� chondrules. The latter have circular shapes and are composed of relictic olivine or/and pyroxene with interstitial melts. The melt rock fraction consists of short-prismatic olivine with grain sizes <30 �m, <50 im-sized augite and interstitial glass. Large olivine grains in melt rocks are zoned with Fe increasing towards the surface. No shock effects are present in either olivines nor pyroxenes. Glasses in melt rock portions are inclusion-free but locally contain crystallites of Fe-Mg silicates. Relictic olivines and pyroxenes are both <0.3 mm in size and contain tiny troilite and metal blebs. In addition, features like planar fractures, mosaicism and mechanical twining indicate shock alteration of the relictic silicates. Metal and troilite mainly occur as nodules (average size < 0.5 mm) of irregular to rounded shapes. Some troilite nodules include large droplets of metal consisting of Ni (kamacite and taenite). Micrometer - sized metal and troilite globules and particles are dispersed throughout the melt. Regions enriched in such globules resemble shock veins or melt pockets. Relictic chromite occurs as fractured single grains with subhedral to anhedral shape, whereas newly formed chromite forms clusters of small euhedral to subhedral crystals." |
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