Moon & Mars Rocks For Sale

There was a time not so many years ago when the collector could not buy meteorites from the Moon or from Mars. There were none from the Moon except the samples returned by Apollo astronauts. There were only three meteorites from Mars and they were and still are so expensive that they are beyond the budget of many collectors. Fortunately, that is no longer the case. There have in the last few years been recovered from the deserts of the world dozens of meteorites from both the Moon and Mars that are available for the meteorite collector. These meteorites have all gone through rigorous testing and analysis to verify that they truly originate on the Moon or on Mars. We offer some wonderful samples here in beautiful display boxes that will make these specimen treasured items in any meteorite collection.


Featured Meteorite Dealers


Top Meteorite

Meteorite JewelryTOP Meteorite is a trusted source for rare and significant meteorites of exceptional quality. They also offer a unique selection of exquisite meteorite jewelry. TOP Meteorite is happy to assists with appraisals, institutional curation, acquisitions, specimen restoration, and private expeditions.

Lunar MeteoritesTOP Meteorite is a science forward meteorite company founded by author, researcher, hunter, and educator Dustin Dickens. Dustin brings a strong scientific aptitude to TOP Meteorites’ approach to curation, focusing on martian and lunar meteorites, ungrouped achondrites, and primitive & carbonaceous chondrites. Dustin is continuing his education in meteoritics with a focus in geochemistry. TOP Meteorite offers institutional research discounts on all specimens.


The Meteorite Exchange, Inc.

Meteorite for SaleJim and Paul have been offering meteorites for sale on the Internet since 1996. They guarantee the authenticity of every specimen they sell and they only buy meteorites from select trusted sources . They update their catalog often and have a wide variety of meteorites to choose from in all price ranges.

Tektites for SaleThey also have a large variety of impactites and tektites for sale. Many of the tektite specimens are from the Darryl Futrell Collection of Tektites.

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Selected Meteorites For Sale

Meteorites For Sale
Meteorites For Sale
Moon & Mars Rocks For Sale
Stone Meteorites For Sale
Iron Meteorites For Sale
Stony Iron Meteorites For Sale
Meteorite Jewelry
Meteorite Books For Sale
  • NWA 13974 Lunar Impact Melt Breccia
    SR0225 (NWA 13974)NWA 13974 is a typical example of what one should expect to find while exploring on the near-side lunar surface in the vicinity of any large mare region. This Moon rock shows the result of thousands of close by impact events which pulverized the regolith, and in many cases melted some of the small pieces together with the tremendous heat generated by those impacts. This area would have been constantly impacted, pulverized, and re-melted again and again. With a small hand lens, one can easily see a dozen or more greenish olivine clasts plus more than a half dozen white anorthosite clasts that
  • NWA 12593 Moon Dust
    moon-dust-nwa-12593These 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.
  • NWA 12630: Lunar Feldspathic Breccia
    SR0224 (NWA 12630)NWA 12630 is an absolutely spectacular Moon rock! It is also an unusual lunar breccia because most of the clasts it displays contain only a single mineral. The absence of multiple breccias within this breccia suggests it was ejected from deep in the surface regolith. With only the naked eye, more than a dozen 1-3mm white and gray anorthosite clasts, plus more than a dozen 1-2mm black orthopyroxene clasts are easily visible. With a simple magnifying glass, many dozens of smaller clasts containing these same minerals are seen, plus dozens of smaller yellowish brown olivine clasts. One face of
  • NWA 12269: Martian Shergottite
    NWA 12269NWA 12269 is a rare and most unusual Mars rock. It is very fine grained and displays the expected low-calcium pyroxene, clear silica, plus black impact melt glass. However, it contains none of the olivine normally found in Shergottites! That makes this particular meteorite extremely important because it demonstrates the accretion of Mars did not produce a homogenous liquid mantle like occurred with the accretion of Earth. Instead, it is evidence the accretion of Mars produced a heterogeneous semi-liquid mantle with zones containing different mineral mixtures. The mineralogy of NWA 12269 also
  • Mars Rocks – Mars Meteorites
    Mars Rock / Martian Meteorite For SaleWe 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.
  • Moon Rocks | Lunar Meteorites For Sale
    Moon Rocks / Lunar Meteorites For SaleView our Moon Rock Lunar Meteorites for sale on our website. These quality lunar 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 Moon Meteorite.
  • NWA 2995: Lunar Feldspathic Breccia
    SR0219 (NWA 2995)NWA 2995 is a jaw-dropping spectacular meteorite! It displays dozens of 1-6mm anorthosite and basalt clasts easily seen with the naked eye, and hundreds of 0.5-1mm clasts easily seen with a simple magnifying glass. These clasts are of various anorthosites, basalts, plus many examples of clasts within a clast. Lunar orbital data indicates the very deep and thin crusted South Pole-Aitken Impact Basin is the most likely place of origin for this meteorite. This would explain some black pyroxene material not being extrusive mare basalt, but instead being intrusive mantle basalt from a fissure in
  • NWA 2975: Martian Shergottite
    SR0220 (NWA 2975)NWA 2975 is truly a delightful Mars rock to examine, and dozens of large olivine and pyroxene crystal shapes are easily visible beneath its melted surface crust. Shergottites are from near the surface of Mars and contain many tiny cracks from countless nearby impacts. An impact that ejects a Shergottite from Mars would create a shock wave that passes through these cracks creating a black melt glass. Any cracks open to the surface would contain Mars atmosphere, and the shock wave would trap and preserve that Martian atmosphere inside a melt glass bubble. There is no way to know if this
  • NWA 11474: Lunar Feldspathic Breccia
    SR0217 (NWA 11474)NWA 11474 broke into many small fragments without fusion crust as it entered Earth's atmosphere. This is one of the larger fragments that has been sliced in half to expose its interior. These fragments were still hot when they landed in the Sahara Desert, and some of the brown or tan desert sand melted and fused onto the meteorite's surface which can be seen on the back of this specimen. On the polished interior face, more than a dozen 1mm or larger anorthosite clasts are visible with the naked eye; and shock melt glass plus dozens more anorthosite clasts are revealed with just a simple
  • NWA 11474: Lunar Feldspathic Breccia
    SR0216 (NWA 11474)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,
  • NWA 8682: Lunar Feldspathic Breccia
    SR0214 (NWA 8682)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
  • NWA 998: Martian Nakhlite
    SR0202 (NWA 998)NWA 998 is an extremely rare example of a Nakhlite and one of the very few available to collectors. Its dark olive or black pyroxene crystals and light olive or tan olivine crystals are easily seen without magnification. The serpentine surfaces of the olivine crystals definitely indicates this molten rock interacted with water; and the large crystal size indicates an extended cooling period in a thick lava flow. These very obvious features strongly suggest this liquid magma interacted with steam in a volcanic eruption and then slowly cooled in a thick lava flow near a shield volcano on Mars.
  • Tissint: Martian Shergottite
    SR0209 (Tisint)Tissint is identical to the Shergottite EETA 79001, which is the meteorite containing Martian atmosphere in impact melt glass bubbles that proved all SNC meteorites are from Mars! Both of these Shergottites are also unusual in containing olivine in the form of giant megacryst clasts. Two of these 1.5mm broken olivine megacrysts are exposed on the top left of this specimen; and the typical Shergottite pattern of pyroxene crystals is seen over the entire surface. All of the visible plagioclase impact melt glass bubbles were broken open when this sample fragmented, but it is certainly possible
  • Zagami: Martian Shergottite
    SR0206 (Zagami)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
  • NWA 6963: Martian Shergottite
    SR0205 (NWA 6963)NWA 6963 contains gigantic pyroxene crystals that are actually eight times the size by volume of typical Shergottite crystals! It also shows many large transparent silica crystals. A typical Shergottite is thought to result from magma that erupted from a fissure in the Martian crust and then flowed onto the surface where it quickly cooled. But the huge crystals in this Shergottite suggests it remained within the fissure where it cooled more slowly and did not erupt onto the surface. The large shock melt glass bubble in this specimen would have preserved a sample of Mars atmosphere and then
  • NWA 8609: Lunar Feldspathic Breccia
    SR0211 (NWA 8609)NWA 8609 is a terrific lunar highland meteorite to examine with only the naked eye. It shows more than a dozen 2-5mm anorthosite clasts and countless smaller clasts. There are also a few 3mm size pyroxene clasts and some melt glass to see. Many of the larger clasts are themselves breccias containing olivine clasts within them. The huge clasts plus very little melt glass indicate this meteorite is from deeper in the regolith and was not part of the top surface regolith. This is the ideal lunar meteorite to enjoy with just the naked eye, but you can use a magnifying glass to view this meteorite
  • NWA 482: Lunar Impact Melt
    SR0208 (NWA 482)NWA 482 is an extremely rare lunar meteorite because it contains only highland anorthosite crust minerals! It contains absolutely no detectable basalt minerals! The darker colored areas are impact melted plagioclase. The mineralogy of this meteorite strongly suggests its origin was on the Moon's far side and from very deep in the lunar crust. This meteorite contains only deep anorthosite crust minerals that have been melted and remelted by countless impacts over billions of years. Fusion crust is visible on the angled edge of this specimen. NWA 482 is totally unique among all the known lunar