MILE HIGH METEORITES

Mile High Meteorites was established in 1996, one of the first meteorite businesses on the internet and soon became the place where beginning and experienced meteorite collectors could purchase rare and exotic meteorites.   We offer many types of meteorites for sale, including: iron meteorites, stony-iron (pallasite) meteorites, achondrite meteorites, meteorites from the Moon and Mars,  and historic meteorites with documentation. Many of the meteorites we sell are used for meteorite jewelry, meteorite knives, inlays within dinosaur bone, and other artisanal forms.

Mile High Meteorites founder and president Matt Morgan, oversees all operations of the business. He spent the last three decades building one of the most trustworthy and respected meteorite businesses on the internet.

We have served the collecting and museum community -worldwide- through sales, exchanges, donations, and consultation. We thank all of our past customers and welcome all our new ones to the experience of meteorite collecting.

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SALES INVENTORY

Certificates of Authenticity and additional photos available upon request

Esquel Pallasite 36-8

Esquel, Argentina (Pallasite)

One look at this meteorite and you will understand why the Esquel pallasite is known as the "King of the Pallasites" amongst collectors, The Esquel pallasite is prized for its golden gem-quality peridot (olivine) crystals, some can be faceted for jewelry. Very impressive, highest quality, and now hard to locate. 36.8 gram slice with edge of original exterior. Etched on one side.

Esquel 140g Pallasite Slice

Esquel, Argentina (Pallasite)

One look at this meteorite and you will understand why the Esquel pallasite is known as the "King of the Pallasites" amongst collectors, The Esquel pallasite is prized for its golden gem-quality peridot (olivine) crystals, some can be faceted for jewelry. Very impressive, highest quality, and now hard to locate. Large and rare 140 gram slice with an edge of the original exterior.  Etched on one side.

Seymchan pallasite

Seymchan, Russia (Pallasite)

Gorgeous elongated slice of the Seymchan pallasite.  Clear golden and orange olivine crystals abound and are surrounded by glistening metal. Highly polished on both sides. 52 grams.

Allende 473g

Allende, Mexico (CV3)

Museum-quality, super fresh, 473 gram complete Allende meteorite. I purchased this piece about a decade ago from dealer Blaine Reed and sold it to a collector. Blaine received it from Arizona State University. The Allende meteorite is important because it is the largest known carbonaceous chondrite fall and contains some of the oldest material formed in the solar system, providing unique insights into the early history of planets and the origin of organic compounds. A rare offering. Consignment piece.

Imilac 196

Imilac, Chile (Pallasite)

The Imilac pallasite is one of the most famous stony-iron meteorites, prized for its translucent golden olivine crystals set in an iron-nickel matrix. Large complete individuals like this 196 g specimen are especially desirable today, as intact pieces with unbroken olivine are increasingly scarce on the market. Consignment piece.

Seymchan 1.954kg

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 1.945 kg end cut with clear delineation of olivine and iron with Widmanstatten pattern! Really cool example.  Consignment piece,

NWA 869 2.63kg

NWA 869 (L3-6), Morocco

NWA 869 is a brecciated ordinary chondrite whose interior reveals a beautiful mix of chondrules, metal flakes, and light and dark clasts, offering a window into the early processes that shaped the solar system. Its varied textures preserve evidence of impact and metamorphism, making it an excellent example of the dynamic history of asteroid parent bodies. 2.63 kg complete specimen that would be fantastic when cut. Consignment piece.

NWA 170224 A4 Mesosiderite

NWA 17025 (Mesosiderite type A4)

NWA 17025 is a rare type A4 mesosiderite, one of only six known in this classification, distinguished by its fine-grained silicate matrix intricately mixed with nickel-iron metal. Its unique texture records intense heating and mixing processes, making it an extraordinary witness to the violent collisions and differentiation events of the early solar system. 368 gram complete specimen with fusion crust, ready to be cut to show its internal beauty! Consignment piece.

NWA 15491 5kg ureilite

NWA 15491

This is the 5 kg ureilite main mass (largest and only piece) of NWA 15491. The complete piece is composed of a coarse-grained mosaic of olivine and pyroxene with accessory metal, sulfides, and graphite. Ureilites are especially prized for their carbon content, often containing graphite and even microscopic diamonds formed during ancient impacts, and they preserve evidence of catastrophic collisions and partial melting that reveal the violent history of early planetesimals in the solar system. Consignment piece,

Timertine 76 grams

Timétrine 001, Algeria (Basalt-bearing Lunar Melt)

Discovered in 2024 near Gao, Mali, Timétrine 001 is a striking lunar melt breccia featuring a dark melt and light feldspathic bands. The cut face reveals diverse clasts set in glassy melt, including anorthosite, basalt, and breccia-in-breccia textures. 76 gram complete slice with mirror polish.

NWA 15658 Eucrite Melt

NWA 15658, Morocco (Eucrite Melt Breccia)

Likely formed by a powerful impact on its parent asteroid, possibly Vesta, this meteorite features fragments of basalt rock and mineral grains within a dark, shock-melted matrix. The main minerals include pyroxene and plagioclase, with the melted areas showing signs of flow. You can also find traces of silica, chromite, ilmenite, and iron sulfide. 
Giant 141.5 gram complete slice with mirror polished face - paired with NWA 15658.

El Eglab 82.8g

El Eglab, Algeria (Mesosiderite)

Discover the stunning complexity of the El Eglab mesosiderite, a breccia containing large mineral fragments up to 5 mm, including olivine, orthopyroxene, and ~60% metal (kamacite and taenite). This specimen also features mafic lithic clasts with intergranular or microgabbroic textures. The matrix boasts a diverse mineral suite, including pigeonite, anorthite, silica polymorphs, chromite, ilmenite, merrillite, and troilite—a remarkable piece of cosmic history. 82.8 gram complete slice.

NWA 6355 13.2g

NWA 6355, Morocco (Lunar Feldspathic Breccia)

Rare offering! NWA 6355 is a remarkable lunar meteorite classified as a feldspathic breccia, showcasing its unique, fragmented texture formed by ancient impacts on the Moon's surface. It's chemistry is compositionally similar to the lunar soil samples collected from the Apollo 16 site. This similarity suggests that NWA 6355 may have originated near the Apollo 16 region, providing a tangible connection to the Moon's highlands and offering valuable insights into its geological history. 10.2 gram complete slice.

NWA 15658 Eucrite Melt

NWA 15658, Morocco (Eucrite Melt Breccia)

Likely formed by a powerful impact on its parent asteroid, possibly Vesta, this meteorite features fragments of basalt rock and mineral grains within a dark, shock-melted matrix. The main minerals include pyroxene and plagioclase, with the melted areas showing signs of flow. You can also find traces of silica, chromite, ilmenite, and iron sulfide. 
Big 138 gram complete slice with mirror polished face. Bargain priced while they last! Other slices available.

NWA 14682 25g Meteorite

NWA 14682, Morocco (Eucrite, unbrecciated)

Basaltic eucrite with a "needle-like" texture. Eucrites likely originate from the asteroid Vesta as basalt flows similar to volcanic lava flows on Earth.  25 gram slice.

NWA 13682 Eucrite

NWA 14682, Morocco (Eucrite, unbrecciated)

Basaltic eucrite with a "needle-like" texture. Eucrites likely originate from the asteroid Vesta as basalt flows similar to volcanic lava flows on Earth. 123 gram complete slice.

Saint-Severin LL6 meteorite weighing 28.87g

Saint-Severin, France (LL6)

On June 27, 1966, residents of Saint-Séverin, France and nearby villages witnessed a series of explosions and a sonic boom.  Not long after, a meteorite of 113 kg was extracted from a crater that measured 60 cm in depth and 80 cm in diameter.  This 28.87 gram complete slice comes from my large mass that I acquired from Robert Haag.  The slice is beautifully brecciated, has some fusion crust and measures a sizable 120 mm X 95 mm!

NWA 5515 39.6

NWA 5515, Algeria (CK4)

This extraordinary piece of NWA 5515, a CK4 meteorite, represents the Karoonda-type carbonaceous chondrites, known for their high oxidation states and thermal metamorphism.  Believed to originate from a differentiated asteroid shared with the CV chondrites, this specimen reflects a formation history shaped by prolonged thermal processing and oxidation in the outer regions of the solar nebula. 39.6 gram complete slice

Seymchan 13g

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 13 gram slice with golden olivine (peridot), mirror polish on both sides.

Timetrine 001 27g

Timétrine 001, Mali (Basalt-bearing Lunar Melt)

Discovered in 2024 near Gao, Mali, Timétrine 001 is a striking lunar melt breccia featuring a dark melt and light feldspathic bands. The cut face reveals diverse clasts set in glassy melt, including anorthosite, basalt, and breccia-in-breccia textures. 27 gram complete slice with mirror polish.

Vinales 30.4 g

Vinales, Cuba (L6)

On February 1, 2019, a brilliant daytime fireball streaked across the skies of Pinar del Río, Cuba, followed by loud sonic booms and ground-shaking rumbles. A shower of meteorites fell across the scenic Viñales Valley, a UNESCO World Heritage site. Many stones landed in fields, forests, rooftops, and even smashed a laptop! Fresh and beautifully brecciated 30.4 gram slice.

El Eglab Mesosiderite 44.9g

El Eglab, Algeria (Mesosiderite)

Discover the stunning complexity of the El Eglab mesosiderite, a breccia containing large mineral fragments up to 5 mm, including olivine, orthopyroxene, and ~60% metal (kamacite and taenite). This specimen also features mafic lithic clasts with intergranular or microgabbroic textures. The matrix boasts a diverse mineral suite, including pigeonite, anorthite, silica polymorphs, chromite, ilmenite, merrillite, and troilite—a remarkable piece of cosmic history. 44.9 gram complete slice.

Krymka LL3.2 meteorite 24.47g

Krymka (Chondrite LL3.2)

Stunning 24.47 gram part slice of a very rare LL3.2 chondrite. The Krymka meteorite was observed to fall on January 21, 1946 in the Ukraine.  It is a very primitive chondrite (thus the LL3.2 designation) having undergone very little metamorphism on its parent body.  The slice is packed with multi-colored chondrules and is rimmed by fresh fusion crust on the natural edges. Kyrmka also contains "mysterite" which are dark patches of unknown celestial origin. Slice comes with copies of two labels from the Ivan Franko National University of Lviv.

Seymchan 14 g

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 14 gram slice with golden olivine (peridot), mirror polish on both sides.

Allende 28.6g

Allende, Mexico (CV3)

The Allende meteorite fell on February 8, 1969 over the Chihuahua state of Mexico. Over 2.2 tons of fragments were recovered over a 8 km X 50 km area. Allende has been extensively studied and is known to contain calcium aluminum inclusions that are older than the Earth and newly discovered grains that are likely older than our Sun!  FRESH 28.6 gram end section with vintage dealer label.

Seymchan 10g

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 10 gram slice with golden olivine (peridot), mirror polish on both sides.

Canyon Diablo 80.1g

Canyon Diablo, Arizona (Iron-IAB)

Canyon Diablo meteorites are famous for their location - Meteor Crater near Winslow, Arizona. The crater was formed over 50,000 years ago when a 50-m-wide iron meteorite slammed into the desert floor creating a crater 1200 m wide and 170 m deep. This 80.1 gram complete piece has a nice shape with several points.

Murchison Meteorite

Murchison, Australia (Carbonaceous Chondrite-CM2)

The Murchison meteorite fell on September 28, 1969 near the village of Murchison in southeastern Australia. Murchison is one of the most studied meteorites of all time. It is rich in carbon, contains amino acids and calcium-aluminum inclusions. In 2020, researchers determined Murchison contains silicon-carbide minerals that are nearly 7 billion years old! This is extremely hard to obtain due to its scientific importance.
2.0 gram crusted fragment with cut face. Smaller pieces available.

Gebil Kamil 53.5

Gebil Kamil, Egypt (Iron-Ungr. Ataxite)

An individual iron meteorite from the Gebel Kamil crater that was formed by an impact about 5,000 years ago! A great and currently affordable iron meteorite tied to a crater-forming event. 53.5 gram specimen.

NWA 13877, Morocco (CK 3.0-3.2)

NWA 13877, Morocco (CK 3.0-3.2)

NWA 13877 is a rare example of a Karoonda-type carbonaceous chondrite named after a meteorite recovered in the Karoonda region of Australia in 1930. The NWA 13877 is related to CV and CO carbonaceous chondrites which contain abundant magnetite and unique calcium-aluminum inclusions (CAIs) which formed in the early nebula during the formation of our solar system. This slice of NWA 13877, classified by New Mexico's Institute of Meteoritics contains the above mentioned CAIs plus abundant chondrules within its greyish-brown colored matrix. Classified as a CK3 with characteristics of a CK3.0-3.2 which means it is an example of a meteorite with virtually unaltered carbonaceous material. 33.8 gram complete slice ~2 mm in thickness.

Putinga 15.1 g

Putinga, Brazil (L6)

On August 16, 1937, a brilliant bolide lit the afternoon sky over southern Brazil. The next day, locals near Putinga discovered several large meteorites buried deep in the soil — the largest weighing 57 kg and 45 kg, recovered from depths of up to 3 meters. Additional stones were later found across multiple municipalities, with a total recovered mass of about 300 kg. Rich in Fe-Ni metal and containing minor troilite, chromite, and merrillite, Putinga is a well-equilibrated L6 ordinary chondrite. Its intersecting shock features, including maskelynite from converted plagioclase, record a violent impact history before its arrival on Earth. 15.1 gram slice with fusion crust.

NWA 11182 Lunar 20.2

NWA 11182 (Lunar, feldspathic breccia)

This unique complete slice reveals a breathtaking fragmental breccia with white feldspathic clasts and fine-grained lithic fragments set in a dark-gray ground mass. A rare and remarkable addition for any collector, it showcases feldspathic and microgabbro clasts alongside shock melt, some with vesicles. 20.2g complete slice.

Gebel Kamil 72.3g

Gebil Kamil, Egypt (Iron-Ungr. Ataxite)

An individual iron meteorite from the Gebel Kamil crater that was formed by an impact about 5,000 years ago! A great and currently affordable iron meteorite tied to a crater-forming event. 72.2 gram specimen.

NWA 16803 R-Chondrite 44 g

NWA 16803, Morocco (R5)

A rare R-type chondrite that was recovered in Morocco in 2020. R-chondrites originate from near the surface of chondritic asteroids and are implanted by solar wind gases. The “R” is from the namesake Rumuruti, which fell January 28, 1934 in Kenya. 44 gram complete slice with high polish.

NWA 16803 R5 Chondrite

NWA 16803, Morocco (R5)

A rare R-type chondrite that was recovered in Morocco in 2020. R-chondrites originate from near the surface of chondritic asteroids and are implanted by solar wind gases. The “R” is from the namesake Rumuruti, which fell January 28, 1934 in Kenya. 116 gram end section with original exterior on back side, one polished face.

Gibeon 74.9g

Gibeon, Namibia (Iron - IVA, fine octahedrite)

Amazing slice with an outstanding  Widmanstatten pattern! Polished one one side and etched on both sides. 74.9 grams.

Allende 5.8 gram

Allende, Mexico (CV3)

The Allende meteorite fell on February 8, 1969 over the Chihuahua state of Mexico. Over 2.2 tons of fragments were recovered over a 8 km X 50 km area. Allende has been extensively studied and is known to contain calcium aluminum inclusions that are older than the Earth and newly discovered grains that are likely older than our Sun! 5.8 g fragment.

Gebel Kamil 136.8g

Gebel Kamil, Egypt (Iron-Ungr. Ataxite)

An individual iron meteorite from the Gebel Kamil crater that was formed by an impact about 5,000 years ago! A great and currently affordable iron meteorite tied to a crater-forming event. 136.8 gram specimen.

Canyon Diablo 5.5kg

Canyon Diablo, Arizona (Iron-IAB)

Canyon Diablo meteorites are famous for their location - Meteor Crater near Winslow, Arizona. The crater was formed over 50,000 years ago when a 50-m-wide iron meteorite slammed into the desert floor creating a crater 1200 m wide and 170 m deep. HUGE 5.5 kg end section with etched face. Consignment piece.

Cape York 211g slice

Cape York, Greenland (IIIAB)

The Cape York meteorite, one of the largest iron meteorites ever discovered, is estimated to have fallen to Earth around 10,000 years ago. Found in Greenland, this meteorite has been an invaluable source of metal for the indigenous Inuit people, who used it for tools and weapons. Its discovery in the early 19th century has provided significant insights into the composition and history of our solar system. 211 gram etched slice with original Greenland postage stamps honoring the meteorite!

Aiquile 393g meteorite

Aiquile, Bolivia (H5)

The Aiquile meteorite is a dramatic witnessed fall from Bolivia, recorded on November 20, 2016, as brilliant fireballs and sonic booms startled communities across the region. This specimen is a weakly oriented H5 chondrite, displaying subtle flow lines and a rich black fusion crust from its fiery descent through Earth’s atmosphere. Aiquile stands out as one of the most striking and well-documented falls of the 21st century. This 393 gram complete specimen is a choice addition to any serious meteorite collection.

Muonionalusta 229g

Muonionalusta, Sweden (IVA)

The Muonionalusta meteorite, discovered in northern Sweden in 1906, is one of the oldest known meteorites, estimated to have fallen to Earth about one million years ago. Composed primarily of iron and nickel, it exhibits a striking Widmanstätten pattern when etched, revealing its crystalline structure. Stunning 229 gram slice.

Admire 206g Pallasite

Admire, Kansas (Pallasite)

206 gram slice with outstanding angular golden olivine crystals. The Admire pallasites were plowed up by a famer tilling his fields in Kansas in 1891. Many of the olivine crystals in the Admire pallasite have been faceted by fine jewelers around the world.

NWA 10822 Lunar Meteorite 2.7 g

NWA 10822, Morocco/Algeria (Lunar)

A very affordable complete fragment with many anorthosite clasts in a grayish matrix.  Orange spots are areas of desert soil.  This feldspathic breccia likely originates from the nearside of the moon.
2.7g fragment.

NWA 10822 lunar 5.3g

NWA 10822, Morocco/Algeria (Lunar)

This feldspathic breccia likely originates from the nearside of the moon.
5.3 gram complete end section. A stunning and affordable example of a piece of our nearest neighbor.

Juancheng 147.3 gram

Juancheng, China (H5)

On February 15, 1997, a brilliant fireball with trailing smoke and sparks streaked over Shandong Province before ending in a loud, resonating explosion. More than 1,000 small stones fell across a 10.5 × 4.3 km area near the Yellow River, the largest weighing 2.7 kg, with a total recovered mass exceeding 100 kg.

Juancheng is an H5 ordinary chondrite, typically showing fresh black fusion crust and light gray interiors. Notably, one stone reportedly crashed through a roof and landed directly in a pot on a stove — a dramatic end to a long journey through space. 147 gram complete specimen with black fusion crust.

Zagora 008 19.4g Eucrite

Zagora 008, Morocco (Fragmental monomict eucrite breccia)

A new and fresh eucrite breccia from the Zagora area of Morocco.  Composition is approximately 60% pyroxene and 35% plagioclase. The pyroxene compositions are uniformly consistent with a single cumulate eucrite lithology. Pyroxenes are highly equilibrated with distinct high-Ca and low-Ca compositional separation. 19.4 gram complete slice with weathered crust.

Seymchan Meteorite

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 9 gram slice with golden olivine (peridot), mirror polish on both sides.

Bechar 010 10.7g Lunar Meteorite

Bechar 010, Algeria (Lunar Feldspathic Breccia)

Our newly classified lunar feldspathic breccia! Composed of olivine, pyroxene and plagioclase minerals set in a fine-grained glassy and recrystallized feldspathic matrix.  Also contains microgabbroic clasts, iron-nickel metal, troilite and chromite. 10.7 gram complete slice, mirror polish on both sides.

NWA 17059 50g

NWA 17059, Algeria (Diogenite)

Diogenites are coarse-grained achondritic meteorites composed primarily of orthopyroxene, often with minor olivine, chromite, and metal. They formed deep within the crust of asteroid 4 Vesta, representing slow-cooled plutonic rocks. Most diogenites are brecciated from impact processes and delivered to Earth via fragments ejected from Vesta's surface. 50 gram complete slice, mirror polished on one side. 

Amo 5.5 gram

Amo, Indiana, USA (L5)

On December 10, 2024, a bright fireball west of Indianapolis produced one of the largest U.S. meteorite falls recorded by NEXRAD radar. The strewnfield covered Amo, Coatesville, and Fillmore, with detections lasting over nine minutes. First stones, recovered the next day, are fresh L5 ordinary chondrites with black fusion crust and light gray interiors. Our last 5.5 gram slice with fresh fusion crust.

Seymchan 19g

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 15 gram slice with golden olivine (peridot), mirror polish on both sides.

Abbott 85.9 gram meteorite from UNM

Abbott, New Mexico (H3-5)

Abbott meteorite was found between 1951 and 1960 in Colfax County, New Mexico with a total weight of about 21 kg. It is an unusual class of chondritic meteorite called a regolith breccia containing both carbonaceous and chondritic fragments, melt pockets and trapped solar-wind gases. This 85.9 gram half stone is from University of New Mexico Institute of Meteoritics collection. Specimen is accompanied by UNM specimen card and bag.

Seymchan 19gram

Seymchan, Russia (Pallasite)

A sample of the inner workings of an asteroid! Gorgeous and very stable stony-iron pallasite with gem-quality olivine set in an iron-nickel matrix. Pallasites give us a glimpse of the internal structure of differentiated asteroids as their chemical composition and visual texture suggest they formed deep within their parent body. 19 gram slice with golden olivine (peridot), mirror polish on both sides.

Canyon Diablo56.1 gram

Canyon Diablo, Arizona (IAB)

Canyon Diablo meteorites are famous for their location - Meteor Crater near Winslow, Arizona. The crater was formed over 50,000 years ago when a 50-m-wide iron meteorite slammed into the desert floor creating a crater 1200 m wide and 170 m deep. This 51.6 complete piece has a nice shape with several points.

Zagora 008 Eucrite Meteorite 24.4g

Zagora 008, Morocco (Fragmental monomict eucrite breccia)

A new and fresh eucrite breccia from the Zagora area of Morocco. Composition is approximately 60% pyroxene and 35% plagioclase. The pyroxene compositions are uniformly consistent with a single cumulate eucrite lithology. Pyroxenes are highly equilibrated with distinct high-Ca and low-Ca compositional separation. 24.4 gram end section with weathered crust.

NWA 13543 19.4 gram

NWA 13543 (CV3)

Complete slice of an excellent CV3 carbonaceous chondrite with stunning chondrules and CAI's.
19.4 gram complete slice.

Canyon Diablo 94g

Canyon Diablo, Arizona (Iron - IAB)

Canyon Diablo meteorites are famous for their location - Meteor Crater near Winslow, Arizona. The crater was formed over 50,000 years ago when a 50-m-wide iron meteorite slammed into the desert floor creating a crater 1200 m wide and 170 m deep. This 94 gram complete piece has a nice shape.

Tsarev 21.7g slice

Tsarev, Russia (L5)

The Tsarev meteorite fall probably occurred on December 6, 1922, was recovered in 1968 and recognized as a meteorite in 1979. The meteorite's recovery took place in the fields surrounding the village of Tsarev in the former USSR. This complete slice is full of shiny metalflake, highly polished to a mirror finish and rimmed by weathered fusion crust.  21.7 gram complete slice.

Odessa 134g

Odessa, Texas (Iron - IAB)

The Odessa, Texas iron meteorite is a classic American meteorite from one of the largest impact sites in the United States. First discovered in 1922, fragments come from a crater field formed over 60,000 years ago. Now protected as a historical landmark, no more specimens can be legally collected from the site. Own a piece of U.S. meteorite history while they’re still available. Historic piece collected in the early 1980s. Nicely shaped 134 gram complete specimen.

Gibeon 80g

Gibeon, Namibia (Iron - IVA)

Superb Widmanstatten pattern on this 80.4 gram slice with an edge of the original meteorite surface.

NWA 13518 R-chondrite 8.4g

NWA 13518, Algeria/Mali (R 4-5)

A rare R-type chondrite that was recovered near the Mali-Algeria border in 2019. R-chondrites originate from near the surface of chondritic asteroids and are implanted by solar wind gases. The “R” is from the namesake Rumuruti, which fell January 28, 1934 in Kenya. 8.4 gram complete slice with high polish on both sides.

NWA 15953 44.4 gram

NWA 15953, Algeria (Diogenite)

Diogenites are rare achondrite meteorites from deep within the crust of asteroid Vesta, composed mainly of orthopyroxene. Their crystalline texture and greenish hue make them a unique and scientifically important addition to any collection. 44.4 gram complete slice, mirror polished on one side.

NWA 15662 20.5 Gram

NWA 15662, Algeria (LL3)

This extraordinary meteorite is packed with unequilibrated chondrules, many displaying stunning porphyritic textures with glass or mesostasis. Under reflected light microscopy and electron microprobe examination, some chondrules reveal intricate decorations of troilite grains. A fascinating piece that showcases the complexity and beauty of our solar system's early formation.
20.5 gram complete slice.

Seymchan 53.3g

Seymchan, Russia (IIE/Pallasite)

53.3 gram iron-rich slice, deep-etched on both sides. Cluster of schreibersite on one edge. Gorgeous example.

Sikhote-Alin meteorite 8g

Sikhote-Alin, Russia (Iron - IIAB)

Nice shape and character on this 8g complete Sikhote-Alin meteorite.

NWA 16087 9g

NWA 16087, Morocco (Howardite)

Howardites represent the regolith or surface "soil" of an asteroid! They contain fragmented pieces of eucrites and diogenites and are impregnated with solar wind gases. This is a 9 gram slice of a howardite from the 7.45 kg main mass we purchased in 2023.

Muonionalusta 208g

Muonionalusta, Sweden (IVA)

The Muonionalusta meteorite, discovered in northern Sweden in 1906, is one of the oldest known meteorites, estimated to have fallen to Earth about one million years ago. Composed primarily of iron and nickel, it exhibits a striking Widmanstätten pattern when etched, revealing its crystalline structure. Stunning 208g slice.

Sikhote-Alin 26g meteorite

Sikhote-Alin, Russia (Iron-IIAB)

Really nice example of a thumbprinted Sikhote-Alin with gray-black fusion crust.  26 grams.

Springwater 27-2

Springwater, Canada (Pallasite)

Originally discovered by famed meteorite hunter H.H. Nininger in 1931, the Springwater pallasites were Canada's first pallasites. Stabilized to inhibit rusting, 27.2g end section with natural surface.

Seymchan 75.4g

Seymchan, Russia (IIE/Pallasite)

75.4 gram iron-rich slice, deep-etched on both sides. Cluster of schreibersite on bottom right corner. Gorgeous example.

NWA 16087 Howardite Meteorite 208.3g

NWA 16087, Morocco (Howardite)

Howardites represent the regolith or surface "soil" of an asteroid!  They contain fragmented pieces of eucrites and diogenites and are impregnated with solar wind gases.  This is a huge 208.3 gram complete slice of a howardite from the 7.45 kg main mass we purchased in 2023.

Imilac Pallasite

Imilac, Chile (Pallasite)

This complete slice of the Imilac pallasite etched on both sides. The olivine (peridot) crystals are golden-yellow in color - cosmic jewels! The Imilac pallasite was first recovered from the Atacama Desert in Chile back in 1822. 6.46 gram slice rimmed by the original exterior with glowing olivine.

NWA 13446 1.7g

NWA 13446, Algeria (Olivine-rich Igneous Achondrite)

NWA 13446 is a rare ungrouped cumulate achondrite that consists dominantly of zoned olivine (~90%) with intercumulus assemblages of low-Ca pyroxene, augite and sodic plagioclase-like glass. The polished surface reveals blades of olivine that are layered and blobs of metal. See the Meteoritical Bulletin entry for NWA 13346 here. This 1.7 gram slice has an edge of weathered fusion crust.

NWA 16087 27g

NWA 16087, Morocco (Howardite)

Howardites represent the regolith or surface "soil" of an asteroid! They contain fragmented pieces of eucrites and diogenites and are impregnated with solar wind gases. This is a 27 gram slice of a howardite from the 7.45 kg main mass we purchased in 2023.

Sikhote-Alin 37g

Sikhote-Alin, Russia (Iron - IIAB)

Nice shape and character on this 37g complete Sikhote-Alin meteorite.

NWA 13543 CV3 20.8 gram

NWA 13543 (CV3)

Complete slice of an excellent CV3 carbonaceous chondrite with stunning chondrules and CAI's.
20.8 gram complete slice.

Seymchan 85.7

Seymchan, Russia (IIE/Pallasite)

85.7 gram iron-rich slice, deep-etched on both sides. Cluster of schreibersite top left corner. Gorgeous example.

Odessa Washington 151

Odessa, Texas (Iron-IAB)

“The Washington Profile”
This Odessa, Texas iron meteorite bears a striking resemblance to the profile of George Washington, with rugged detail that echoes the classic silhouette seen on U.S. quarters and sculptures. Natural shaping and ancient patina features give it both character and historical appeal. A fun and patriotic conversation piece from outer space. 151 grams.

NWA 15953 74g

NWA 15953, Algeria (Diogenite)

Diogenites are rare achondrite meteorites from deep within the crust of asteroid Vesta, composed mainly of orthopyroxene. Their crystalline texture and greenish hue make them a unique and scientifically important addition to any collection. 74 gram complete slice, mirror polished on one side.

Sikhote-Alin Meteorite 41

Sikhote-Alin, Russia (Iron - IIAB)

Nicely thumbprinted 41 gram complete Sikhote-Alin meteorite. Examples like these are tough to find these days.

Imilac Pallasite

Imilac, Chile (Pallasite)

This complete slice of the Imilac pallasite etched on both sides. The olivine (peridot) crystals are golden-yellow in color - cosmic jewels! The Imilac pallasite was first recovered from the Atacama Desert in Chile back in 1822. 5.93 gram slice rimmed by the original exterior with glowing olivine.

Imilac Pallasite

Imilac Chile (Pallasite)

This complete slice of the Imilac pallasite etched on both sides. The olivine (peridot) crystals are golden-yellow in color - cosmic jewels! The Imilac pallasite was first recovered from the Atacama Desert in Chile back in 1822. 5.75 gram slice rimmed by the original exterior with glowing olivine.

Canyon Diablo Meteorite 164g

Canyon Diablo, Arizona (Iron - IAB)

Canyon Diablo meteorites are famous for their location - Meteor Crater near Winslow, Arizona. The crater was formed over 50,000 years ago when a 50-m-wide iron meteorite slammed into the desert floor creating a crater 1200 m wide and 170 m deep. 164 gram complete specimen with nice characteristics.

Sikhote-Alin 10g

Sikhote-Alin, Russia (Iron - IIAB)

Good small piece with character and fusion crust. Weighs 10.0 grams.

Allende meteorite 6g

Allende, Mexico (CV3)

The Allende meteorite fell on February 8, 1969 over the Chihuahua state of Mexico.  Over 2.2 tons of fragments were recovered over a 8 km X 50 km area.  Allende has been extensively studied and is known to contain calcium aluminum inclusions that are older than the Earth and newly discovered grains that are likely older than our Sun! 6 gram end piece. 

Gebel Kamil 138.6g

Gebel Kamil, Egypt (Iron-Ungr. Ataxite)

An individual iron meteorite from the Gebel Kamil crater that was formed by an impact about 5,000 years ago! A great and currently affordable iron meteorite tied to a crater-forming event. 72.3 gram specimen.

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