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# AURE 125 NWA 5951 AURE (prov) Rare UREILITE Achondrite MAIN MASS !
US $ 3,400.00 FREE SHIPPING !
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# AURE 122 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 720.00
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# AURE 123.1 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 195.00
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# AURE 123.2 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 165.00 RESERVED
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# AURE 123.3 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 95.00 RESERVED
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# AURE 123.4 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 35.00 RESERVED
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# AURE 123.5 NWA 5951 AURE (prov) Rare UREILITE Achondrite
US $ 35.00
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# AURE 123.7 NWA 5951 AURE (prov) Rare UREILITE Achondrite
SOLD
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Composition: A technical name for ureilite would be olivine-pigeonite achondrite. Ureilites are noted for containing microscopic nano-diamonds only a few microns in diameter. Compared to most other meteorites, ureilites tend to have a high percentage of carbon (up to 2% by weight) in the form of nano-diamonds and graphite.[1] The diamonds are probably the result of high pressure shockwaves produced by collisions of the ureilite parent body with other asteroids. Ureilites can be divided into two subcategories: monomict and polymict. Monomict ureilites are coarse grained olivine with minor pyroxene traces. Polymict ureilites are a mixture of clasts of dissimilar composition.
A typical ureilite contains olivine and pyroxene (pigeonite, augite, or orthopyroxene) crystals, up to several millimeter across, embedded in a dark carbon-rich matrix of graphite and tiny diamond, low-nickel iron metal, troilite (iron sulfide), and iron carbide.
Origin: Unknown. Some groups of meteorites come from a single object (ie. Mars, Moon, 4 Vesta), but there has been no parent body found as yet for the ureilites. It is probable that their origin is a C-type asteroid. It remains unclear whether ureilites originated on different parent bodies or in different regions of a single body. They could even have originated within the Solar Nebula, which would make them the most primitive Achondrites.The presence of diamonds, which can form from graphite as a result of severe shock metamorphism, hints at a violent impact history.
One single stone of 302 g was purchased in June 2009 in Agadir, Morocco, probably found near the Algerian border in the Sahara Desert. The stone showed intact fusion crust and desert varnish. A probe of 20.09 g for a type mass and another one of 2.86g for thin sections were sent for analysis and classification to the Bathurst Observatory Research Facility, NSW . Further samples were cut from the original stone for resale. The remaining Main Mass of 228.7 g is held by Norbert Kammel of ROCKS ON FIRE, in Noble Park Nth., Victoria, Australia.
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