Gebel Kamil, Egypt Iron Meteorite, Crater Maker, Small Individual

$12.00
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In 2009, a research time located and documented a meteorite impact crater in the Egyptian Sahara. Thousands of iron shrapnels were found scattered around a large eroded crater approx. 45m in diameter. The specimens have organic ripped shapes similar to Sikhote Alin sharpnels and most have a natural dark patina. Samples were analyzed and officially classified as a rare ungrouped iron type (plessitic).

The specimens being offered here are early recovery examples that weigh approx. 3 grams each. I have a total of 10 available pieces and this offer is for one (1) specimen selected from the larger lot shown in the photos. 

Refer to the photos. The black centimeter cube is shown for scale and is not included. You are purchasing one (1) of the meteorites shown. You will get the largest remaining specimen available. Your purchase will include a labeled gemjar.

From the Meteoritical Bulletin entry on Gebel Kamil :

Gebel Kamil 22°01'06"N, 26°05'16"E

East Uweinat Desert, Egypt

Found: 19 February 2009

Classification: Iron meteorite (ungrouped)

History: A total of about 1600 kg of iron meteorite shrapnel (thousands of pieces), ranging in mass from < 1 to 35,000 g, plus a single 83 kg individual completely covered with well developed regmaglypts, was found in and around the 45 m diameter Kamil impact crater by an Italian-Egyptian geophysical team in February 2009 and February 2010. Approximately 800 kg of the total mass observed in the field (the regmaglypted individual inclusive) was recovered. The Kamil crater was identified by V. De Michele, former curator of the Natural History Museum in Milan, Italy. The geophysical survey was carried out within the framework of the "2009 Italian-Egyptian Year of Science and Technology".

Physical characteristics: A 634 g type specimen, measuring 88 × 70 × 55 mm, is flattened and jagged shrapnel with a rough, dark-brown external surface. The surface originally sitting in the desert soil shows some oxy-hydroxides due to terrestrial weathering.

Petrography: (M. D’Orazio, DST-PI; Luigi Folco, MNA-SI) Etched sections show an ataxitic structure interrupted on a cm-scale by crystals of schreibersite, troilite and daubreelite enveloped in swathing kamacite. Kamacite spindles (20 ± 5 μm wide) nucleated on tiny schreibersite crystals. The spindles form small aligned clusters and are rimmed by taenite. The matrix is a duplex plessite made of approximately the same proportion of kamacite and taenite lamellae (1-5 μm in thickness) arranged in a micro-Widmanstätten pattern. Many sections show, particularly close to the external surface, shear dislocations offsetting the plessitic matrix and the crystals of the accessory phases by several millimeters.

Geochemistry: Composition of the metal (ICP-MS; D’Orazio and Folco, 2003) is Co = 0.75, Ni = 19.8 (both in wt%), Cu = 464, Ga = 49, Ge = 121, As = 15.6, Mo = 9.1, Ru = 2.11, Rh = 0.75, Pd = 4.8, Sn = 2.49, Sb = 0.26, W = 0.66, Re = 0.04, Ir = 0.39, Pt = 3.5, Au = 1.57 (all in ppm).

Classification: (M. D’Orazio, DST-PI; Luigi Folco, MNA-SI) Iron meteorite (ungrouped), Ni-rich ataxite, extensive shear deformation and low weathering.