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Anvil shaped chondrite with five crusted and one broken surface. Two surfaces show deep and distinct regmaglypts up to 4 cm wide. The fusion crust is thick and well preserved with a webbing of contraction cracks. Flow lines are visible on several portions, particularly in and around the deepest regmaglypts. Not much is known about the find situation other that the strewn field is supposed to be located near the border of Morocco and the Western Sahara. At least three masses (33.25, 10.10 and 4.3 kg respectively) have appeared from this fall since 2006, but it is highly probable that many more have been sold without reference to each other.

Cuboid cut section with five cut surfaces and one surface showing weathered fusion rind. Polished cut surfaces show a dense array of well defined chondrules in various sizes and crystallization patterns up to 10 mm in diameter. Large portions of the unequilibrated meteorite are shock blackened. This particular specimen was cut from the 34 kg main mass of the Santa Vitorio do Palmar meteorite, which was previously considered lost and which was rediscovered after the owner passed away in 2009. The pictured thin section slide measures 48 x 28 mm.

Unequilibrated chondrite with densely packed chondrules and a comparably low matrix ammount. The cut surface which shows a plentiful variation of chondrules opens a window into the aggregation history of protoplanetary material, as it condensed in the presolar cloud 4.56 billion years ago. The pictured fragment was found mid September 2010 from the back of a camel by S. Larabas in the vicinity of Sidi Ahmed Laaroussi, Western Sahara. An additional search did not turn up any further fragments of this peculiar meteorite.

Prism-shaped and moderately weathered ordinary chondrite. The meteorite features two surfaces with well preserved primary and one with secondary fusion crust. An additional fractured surface shows only traces of fusion. The NiFe aggregates visible on the broken surface developed small rust halos, but no patina has formed on this surface. After cutting of the sample, a megachondrule measuring 6 mm in diameter became visible. The lower photo shows the meteorite in situ. Bou Kra 003 was actually the 5th find in the new dense concentration area Bou Kra which was discovered by the Meteorite Recon team in 2010. Additional finds from the 2012 search campaign in the Bou Kra DCA are currently pending classification.

Oriented shield-shaped mass with single regmaglypts and remnant flow-lines. The meteorite has developed a distinct desert patina as well as few stress cracks due to terrestrial weathering. The matrix as well is darkened as an effect of chemical weathering. Most iron aggregates show progressed oxidation. The upper photo was taken with the meteorite still in its find Position. Note the difference in color due to different lighting and cackground contrast, compared to the studio photo. Bou Kra 002 was actually the 4th find in the new dense concentration area Bou Kra which was discovered by the Meteorite Recon team in 2010.