Welcome to our Meteorite Store. We have a large inventory of meteorites for sale including Moon and Mars rocks. We also have tektites, impactites, unique gifts, meteorite rings, and jewelry.
We have been selling meteorites on the internet since 1996 and we guarantee the authenticity of every stone we sell. Our catalog is updated frequently so please check back often. Please signup for our meteorite sales newsletter to receive notices about special offers and discounts. Our newsletter will be sent out a maximum of four times per year. Thank you for visiting!
Moldavites contain more silica than any other type of tektite which produces their green color. Bohemian moldavite types have a greater SiO2 content than the Moravian moldavite types. Bohemian moldavites are mostly variations of green from pale to a rich bottle green color.
Gao officially named
Gao-Guenie was a witnessed fall on March 5 1960. There was initially
some confusion as to whether there had been two distinct falls a month
apart in Burkina Faso, but specimens collected using both names are
exactly the same material. It is now officially considered to be one
fall and has the combined name. Thousands of stones have been found and
continue to be recovered from the area. It is an H5 chondrite. Some
specimens are oriented and many have interesting shapes.
Grapevine Mesa stones have a rusty exterior with some remaining
patches of fusion crust. Slices made from Grapevine Mesa show rounded to
angular silicate inclusions accompanied by rounded to anhedral metal
grains. The metal of Grapevine Mesa closely resembles the meteorite
Bencubbin. Grapevine Mesa has been placed in the subgroup A (CBa) of the
Bencubbin-like Carbonaceous Chondrites. Bencubbin-like Carbonaceous
Chondrites are very expensive and these small fragments make this rare
classification of meteorite much more affordable.
Achondrite meteorites are meteorites without the round chondrule structures. Eucrites are one of the many types of achondrites. Thought to form on larger bodies in space where the rocks can differientiate they have more igneous type compositions. When a meteorite is made up of angular bits of rock it is called a breccia. If it is made of bits from several sources it is called a polymict breccia. This stone is a polymict eucrite breccia. It has not free metal, but is rich in light and dark mineral clasts with a beautiful honey color matrix.
Touat 005 lunar meteorite is composed of
white plagioclase megacrysts up to 2 cm in size and anorthosite
crystals which may be euhedral set in a dark glassy matrix. Touat 005
has shock veins and vesicles evidence of the high stock stage the
meteorite has. Toaut 005 is only moderately weathered.
This is a very
attractive meteorite with a different mixture of clast than many other
feldspathic breccias. The sliced pieces offered here are highly polished
on one side.
Aiquile is an H group ordinary chondrite with abundant visible nickel-iron grains. The stones have a well developed black fusion crust. Aiquile is a type 5 stone based on its chondritic texture and most pieces show no brecciation. However many pieces do contain darker clasts with the same makeup as the rest of the stone. These darker patches can be seen in many of the pieces offered here. Aiquile is moderately shocked and received an S3 stage when classified. As a witnessed fall it is a W0 in weathering which is the stage for the specimens we have for sale which are from a stone found quickly after the fall. Some of the Aiquile stones show isolated small dark inclusions and melt pockets some of these features are also seen among our pieces. Approximately 50 kgs of material were recovered from the fall.
NWA 12594 is a fresh stone with a green-gray color commonly seen in Martian shergottites. It takes a high polish and is a relatively stable meteorite that was not too crumbly during cutting. The slices we are offering have been made into nice affordable pieces that still show off the meteorite well.
As an impact melt meteorite Chico is fascinating to look at. The metal in parts of the meteorite is now tiny blebs of microscopic size that give areas of the stone a silvery metallic sheen. The mineral portion of the meteorite has been melted so much that it runs through the stone as swirling and twisted bands of glassy rock. There are areas bordering the melt that have preserved in them a more normal chondritic appearance. The specimens we are selling were cut from large slices that had been polished on one side already. We have kept them the way they are with one side finished to polish and the other as laboratory cut. The unpolished side actually shows features of the stone that are concealed when polished.
These slices of Imilac Pallasite are polished on all sides and show the wonderful mix of metal and golden olivines. Some of the slices have interesting inclusions of troilite and other meteorite minerals often bordering the bright nickel iron. Imilac is rarely seen for sale as affordable sized polished part slices.
Nice small iron meteorite specimen of Taza (NWA 859) from Northwest Africa.
Latest Meteorite Catalog Updates
Our inventory is updated frequently. Please click to see our latest updates.
Types Of Meteorite For Sale
Iron Meteorites come from the broken metal cores of destroyed asteroids. Iron meteorites are made almost entirely of solid nickel-iron metal and display beautiful internal structures when polished and etched. A couple of excellent examples are Canyon Diablo and Sihote-Alin meteorites.
Chondrite Meteorites are often called Ordinary Chondrites to distinguish them from other stone meteorites. Chondrite meteorites form the largest family of meteorites and come in many varieties. All chondrites share the fact that they have small spherical structures called chondrules as can be seen in most of the meteorite slices. Our meteorite beads are handmade from ordinary chondrite.
Carbonaceous Chondrite Meteorites have chondrules but also have the element carbon in their composition. Some Carbonaceous Chondrites contain organic compounds and primitive protein molecules. This class of meteorites is especially important to research scientists. Carbonaceous meteorites are among the rarest types of space rocks with the most well known being the Allende meteorite.
Achondrites are meteorites without chondrules. Achondrite meteorites come from larger asteroids where minerals melted by pressure within the asteroid or where surface collisions resulted in the melting of asteroid material. The giant asteroid Vesta is believed to be the parent body for many achondrites of the Howardite, Eucrite, and Diogenite families of meteorites.
Lunar and Martian Meteorites are stones that arrived on Earth from asteroid impacts on the Moon and Mars. Their lunar and Martian origins have been confirmed through intensive analysis in laboratories using amongst other evidence, the Apollo Moon Rocks, and Martian atmospheric isotopes as references. The origins of Lunar Meteorites and Martian Meteorites are well confirmed today. NWA 11474 lunar meteorite and NWA 12269 Martian meteorite are very nice representative specimen. New for 2021 we created our Moon Dust display boxes for sale.
Stony-Iron Meteorites are the family of meteorites represented by the Pallasites and the Mesosiderites. Stony-Iron Meteorites contain approximately half nickel-iron metal. In the case of the Pallasites, the other portion is olivine crystals, the same mineral as peridot the semiprecious gemstone. Pallasites are beautiful extraterrestrial jewels once sliced to expose their crystals. Mesosiderites contain silicate minerals in addition to the one-half nickel-iron. Mesosiderites often have fascinating textures as a result of the mixing of stone and metallic materials.
Tektites are glass objects created by the melting of terrestrial rocks by an asteroid collision with Earth. This melted and vaporized Earth rocks were thrown and blown high into the atmosphere where the material cooled into aerodynamic shapes as the blobs of plastic glass fell back down. Tektites are not meteorites but have their origin in catastrophic cosmic impacts.
Impactites are the altered rocks found at asteroid impact sites on Earth. Impactites are often glassy and frothy which demonstrates the tremendous heat released by asteroid collisions.
Unclassified Meteorites are genuine meteorites that have not been sent to a laboratory. Unclassified stone meteorites will show features like chondrules in the cut slice or windowed surfaces we place on them. If they have fusion crust on the outside or metal grains internally these features will show. It is from our supply of genuine but unclassified meteorites that we manufacture our meteorite cabochons.