These Moon Dust display boxes contain genuine moon dust from the cutting of Lunar Meteorite NWA12593. The Moon Dust is securely preserved in a plastic container inside each display box.

Each display box contains 250mg of NWA 12593 lunar meteorite dust displayed in a black plastic glass top display box. These displays make wonderful gifts and come packed in a silver foil gift box.

Please visit our site to see our Libyan Desert Glass. Libyan Desert Glass is generally yellow in color but can be very clear or milky and bubbly light yellow. Some fragments have dark bands and swirls of brownish material. It is in these dark areas that some of the melted comic body is believed by some to be preserved. Libyan Desert Glass was used in ancient times as a gem stone for the Pharaohs and remains a highly prized impact glass for collectors today.

We still have a supply of Mars Rock Martian Meteorites for sale on our website.These quality martian meteorite display boxes make nice additions to your meteorite collections as well as wonderful and unique gift items. Each display box contains a genuine specimen of Mars Meteorite.

NWA 14729 lunar meteorite was purchased from a Moroccan dealer in 2021. The total recovered weight of this lunar meteorite is 2.3 kilograms.  NWA 14729 has been classified as a Lunar (polymict anorthositic troctolite melt breccia). Only nine meteorites have been classified as Lunar Melt Breccias.

The NWA 14729 Lunar Meteorite was found as a single stone. The meteorite has a dark green-brown color. It is a highly shocked meteorite as might be expected as a melt type meteorite. The fine grained light colored host rock is set in a darker vesicular melt rock matrix. Some of the element content in the olivine and plagioclase of NWA 14729 is consistent with that of returned samples of Moon rock from the manned Apollo missions.

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Zagami is considered to be the typical Shergottite; and it was the first Martian meteorite available to collectors. Shergottites are thought to result from magma erupting from a fissure in the Martian crust and then moving in a shallow flow across the surface where it quickly cools. This typical slice shows how solidified pyroxene crystals are oriented in the somewhat general direction of flow. Tiny cracks in the rock are visible as plagioclase shock melt glass veins, as seen on the right side of this slice. Any cracks in contact with the Martian surface when the meteorite's ejection impact occurred will have Mars atmosphere preserved within shock melt glass vein bubbles!

1.07 gram partial slice; 11mm x 23mm x 1.5mm:  $2,170

NWA 11474 broke into many small fragments without fusion crust as it entered Earth's atmosphere. This is one of those fragments that has not been wire brushed, polished, or cut. It has been left just as it appeared when it fell to Earth. At least two dozen 1-3mm anorthosite clasts are easily visible with the naked eye, and shock melt glass surrounds many of these clasts. This fragment was still quite hot when it landed in the Sahara Desert sand, and some of the brown or tan desert sand melted and fused onto the meteorite's surface. If you came upon this meteorite in the desert, picked it up, and wiped it clean; this is exactly what you would be holding in your hand.

1.57 gram individual; 12mm x 15mm x 7mm:  $540

NWA 13366 is an incredibly rare Martian meteorite. Only four Peridotitic Shergottites are recognized, and NWA 13366 is one of them! Shergottites contain 0-15% olivine, but the Peridotitic Shergottites contain 50-60% olivine. NWA 13366 contains 60% olivine! Besides being extremely rare, Peridotitic Shergottites are important because they present additional evidence that the accretion of Mars did not produce a homogenous liquid mantle as occurred with the accretion of Earth. Instead, the Peridotitic Shergottites provide more evidence that the accretion of Mars produced a heterogeneous semi-liquid mantle with multiple zones containing many different mineral mixtures.

3.15 gram partial slice; 33mm x 27mm x1.5mm:  $2,475

NWA 8682 is an absolute joy to examine with a simple magnifying glass! It is officially a feldspathic breccia, but it could be classified as a regolith breccia because almost all the clasts it contains are themselves breccias. The obvious 4mm white anorthosite clast contains gray olivine and black pyroxene clasts within it. Several smaller anorthosite clasts with olivine and pyroxene clasts within them are very easy to see with a magnifying glass. A magnifying glass also reveals at least a dozen 0.5-1mm olivine clasts containing pyroxene clasts within them. A large number of clasts that are actually breccias within a breccia definitely indicates an origin very near the surface of the Moon.

0.42g partial slice; 10mm x 15mm x 1.5mm:  $725