{"title":"Achondrites","description":"\u003cp\u003eAchondrites are a type of stony meteorite that lack chondrules. Chondrules are the small, round inclusions seen in most stony meteorites in the chondrite family. These meteorites formed through a melting and recrystallization processes on their parent bodies, such as asteroids, the Moon, or Mars. This makes them significantly more 'evolved' compared to chondrites, which are considered 'primitive'.\u003c\/p\u003e\n\u003cp\u003eAchondrites come from differentiated celestial bodies, meaning their parent bodies experienced enough internal heat to separate into distinct layers, with heavy metals forming a core and lighter silicate materials forming a crust and mantle. Achondrites represent materials from the outer layers of these differentiated bodies, often resembling volcanic or igneous rocks found on Earth. They formed as molten rock cooled and solidified, erasing the original chondrule structures that would have existed before melting occurred. As a result, these meteorites provide valuable information about planetary processes such as volcanism, impacts, and crust formation.\u003c\/p\u003e\n\u003cp\u003eThere are several important subgroups of achondrites, each associated with specific parent bodies. HED meteorites (howardites, eucrites, and diogenites) are believed to come from Asteroid 4 Vesta. Lunar meteorites come from the Moon, and Martian meteorites originate from Mars. Each of these subtypes offers crucial insights into the geological history of their parent body, including volcanic activity, surface impacts, and the internal structure of these objects.\u003c\/p\u003e\n\u003cp\u003eWhilst achondrites make up only about 8% of all known meteorites, they are particularly important for planetary science. Because they come from bodies that have undergone differentiation, achondrites help researchers understand the processes that shaped not only these individual objects but also the larger mechanisms of planetary formation and evolution in the early solar system. Their study helps scientists piece together the history of planets and large asteroids, providing clues to their structure and development.\u003c\/p\u003e","products":[{"product_id":"nwa-13187-martian-shergottite-diabasic","title":"NWA 13187 - Martian Shergottite (Diabasic) - Complete Slice - 6.97g - Northwest Africa","description":"\u003cp data-start=\"119\" data-end=\"549\"\u003eNWA 13187 is a Martian Shergottite purchased in Morocco in 2019, with a reported total known weight of 1.6 kg. As a Shergottite, it represents basaltic igneous material from Mars, formed through volcanic processes before being ejected from the planet by a powerful impact event. Its Martian origin is supported by its classification and mineral chemistry, placing it within one of the main recognised groups of Martian meteorites.\u003c\/p\u003e\n\u003cp data-start=\"551\" data-end=\"962\"\u003eSpecimens of NWA 13187 typically show a grey to dark, speckled interior with a diabasic igneous texture. Reported mineralogy includes zoned clinopyroxene and other phases consistent with Martian Shergottites, giving prepared slices and fragments a distinctive crystalline appearance. Some pieces may retain desert-weathered exterior surfaces, while cut faces reveal the internal volcanic structure more clearly.\u003c\/p\u003e\n\u003cp data-start=\"964\" data-end=\"1418\"\u003eFor collectors, NWA 13187 offers a recognised Martian meteorite with strong scientific interest and relatively limited available material. Its Shergottite classification, 2019 recovery history, and clear Martian context make it appealing for collections focused on planetary meteorites, Mars material, or rare Achondrites. Each specimen represents a genuine piece of Mars, formed by volcanic activity and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50435463086406,"sku":"MST-07\/16","price":692.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/WIZP0023.jpg?v=1726246490"},{"product_id":"sebkha-el-melah-001-2-45g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 2.45g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543157936454,"sku":"AWA-09\/23","price":110.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha_09_23-4.jpg?v=1773335970"},{"product_id":"sebkha-el-melah-001-2-89g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 2.89g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543482274118,"sku":"AWA-09\/26","price":130.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha_09_26-4.jpg?v=1773335713"},{"product_id":"sebkha-el-melah-001-2-81g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 2.81g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543495512390,"sku":"AWA-09\/24","price":128.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha_09_24-4.jpg?v=1773335292"},{"product_id":"sebkha-el-melah-001-5-41g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 5.41g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543529328966,"sku":"AWA-09\/25","price":245.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha_09_25-4.jpg?v=1773335063"},{"product_id":"sebkha-el-melah-001-2-93g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 2.93g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543541354822,"sku":"AWA-09\/28","price":133.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha_09_28-4.jpg?v=1773334518"},{"product_id":"sebkha-el-melah-001-1-99g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 1.99g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543549612358,"sku":"AWA-09\/21","price":90.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha0921-4.jpg?v=1773334145"},{"product_id":"sebkha-el-melah-001-2-75g","title":"Sebkha el Melah 001 - Aubrite (Enstatite Crystal) - Complete Individual - 2.75g - Mali","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cp data-start=\"129\" data-end=\"505\"\u003eSebkha el Melah 001, often abbreviated to SeM 001, is a rare Aubrite found in Mali in March 2022. Aubrites are Enstatite Achondrites, formed under highly reduced, oxygen-poor conditions on an early differentiated parent body. Approximately 17 kg of material was recovered from the Wad Alhath region, making Sebkha el Melah 001 one of the more significant modern Aubrite finds.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"911\"\u003eSpecimens of Sebkha el Melah 001 are visually distinctive, often appearing as pale, shard-like stones with a white to cream interior. It is described as an unbrecciated Aubrite with an unusual coarse pyroxenitic pegmatite texture, including exceptionally large Enstatite crystals in some material. Some specimens preserve a pale fusion crust, while others show darker crust or natural weathered surfaces.\u003c\/p\u003e\n\u003cp data-start=\"913\" data-end=\"1334\"\u003eFor collectors, Sebkha el Melah 001 offers a rare opportunity to acquire a modern Aubrite with strong scientific and visual interest. Its pale colour, coarse crystalline texture, and low-weathering character make it stand out from many other Achondrites. Each specimen represents ancient igneous material formed in a highly unusual parent body environment, preserving a distinctive record of early solar system processes.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":50543565898054,"sku":"AWA-09\/22","price":125.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Sebkha0922-4.jpg?v=1773333132"},{"product_id":"taoudenni","title":"Taoudenni - Diogenite - Slice - 15g - Mali","description":"\u003cp data-start=\"119\" data-end=\"490\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites.\u003c\/p\u003e\n\u003cp data-start=\"492\" data-end=\"951\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly.\u003c\/p\u003e\n\u003cp data-start=\"953\" data-end=\"1380\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53617544036678,"sku":"TDN-01\/03","price":180.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni11-2.jpg?v=1773078371"},{"product_id":"lunar-bechar-feldspathic-breccia","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.47g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53617901863238,"sku":"BEC-08\/05","price":63.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0805-6.jpg?v=1773314582"},{"product_id":"nwa-13777-ungrouped-achondrite","title":"NWA 13777 - CK6-an Carbonaceous Chondrite - Slice  - 9.24g - Algeria","description":"\u003cp data-start=\"26\" data-end=\"523\"\u003eNWA 13777 is a rare CK6-an Carbonaceous Chondrite purchased in Nouadhibou, Mauritania, in early 2021. The CK group is known for Carbonaceous meteorites that have experienced significant thermal metamorphism, and the type 6 classification indicates a high degree of recrystallisation on the parent body. The ‘an’ designation marks it as anomalous, meaning it differs in some respects from typical CK6 material, adding further scientific and collector interest. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"525\" data-end=\"981\"\u003eSpecimens of NWA 13777 are described as dark greyish rock without fusion crust. As a highly metamorphosed Carbonaceous Chondrite, visible chondrules may be subdued or difficult to distinguish, with the texture generally more compact and recrystallised than less altered Carbonaceous material. This gives it a more uniform appearance while still preserving the chemical character of an ancient Carbonaceous parent body. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"983\" data-end=\"1478\"\u003eFor collectors, NWA 13777 offers a scarce opportunity to acquire an anomalous CK6 Carbonaceous Chondrite with a recognised classification. Its unusual CK6-an status, Northwest African provenance, and thermally altered character make it especially appealing for collections focused on Carbonaceous Chondrites, rare classifications, or altered early solar system material. Each specimen represents primitive asteroid material that has been significantly transformed by heat over billions of years.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53618527469894,"sku":"CK6-06\/01","price":1229.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/NWA13777-4.jpg?v=1773076403"},{"product_id":"tatahouine-tektite","title":"Tatahouine - Diogenite - Fragment - 1.56g - Tunisia","description":"\u003cp data-start=\"120\" data-end=\"542\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle.\u003c\/p\u003e\n\u003cp data-start=\"544\" data-end=\"936\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors.\u003c\/p\u003e\n\u003cp data-start=\"938\" data-end=\"1363\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53619282248006,"sku":"TAT-02\/14","price":52.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine05-7.jpg?v=1773073099"},{"product_id":"nwa-15856","title":"NWA 15856 - Eucrite - Complete Slice - 21.27g - Mauritania","description":"\u003cp data-start=\"119\" data-end=\"505\"\u003eNWA 15856 is a Polymict Eucrite found near Ouargla, Algeria, in 2020 and officially classified as an HED Achondrite. As a Eucrite, it is part of the meteorite family strongly linked to asteroid 4 Vesta, representing basaltic crustal material from an early differentiated body. The Meteoritical Bulletin records NWA 15856 as a single 530 g stone, with its main mass held by Sean Mahoney.\u003c\/p\u003e\n\u003cp data-start=\"507\" data-end=\"995\"\u003eSpecimens of NWA 15856 show a brecciated texture, with angular to sub-rounded cumulate and basaltic Eucrite clasts set within a fine-grained fragmental matrix. Minor Diogenite clasts are also present, making up less than 10 percent by volume, along with accessory phases including silica-rich glass, troilite, and iron-nickel metal. The original stone is described as having heavily weathered fusion crust over around 60 percent of its surface, with desert varnish covering the remainder.\u003c\/p\u003e\n\u003cp data-start=\"997\" data-end=\"1424\"\u003eFor collectors, NWA 15856 offers a scarce and well-documented Vestan Achondrite with strong visual and scientific interest. Its Polymict Eucrite classification records impact mixing on Vesta’s crust, while its single-stone recovery and limited total mass add to its appeal. Each specimen represents ancient basaltic material from asteroid 4 Vesta, shaped by volcanic activity, impact processing, and eventual delivery to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53619448643910,"sku":"EUC-06\/01","price":226.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/EucriteNWA1585601-2.jpg?v=1773062505"},{"product_id":"smeira-003-martian-shergottite-olivine-phyric-3-51g","title":"Smeïra 003 - Martian Shergottite (Olivine-Phyric) - 3.51g","description":"\u003cp data-start=\"26\" data-end=\"496\"\u003eSmeïra 003 is a rare Martian Shergottite found in Tindouf, Algeria, with the find reported from 2021 and official approval published in 2024. It was reportedly found by a shepherd near Hasi Monir, around 45 km west-northwest of Oum El Assel. With a recorded mass of 174.3 g, Smeïra 003 is a very limited Martian meteorite, representing igneous material formed on Mars before being ejected from the planet by a powerful impact event. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"498\" data-end=\"1027\"\u003eSpecimens of Smeïra 003 show a relatively fine-grained texture with dark green and dark brown ferro-magnesian silicate grains, colourless maskelynite, and numerous black shock melt veins. It is classified more specifically as an olivine-phyric Shergottite, with mineralogy including clinopyroxene, olivine, maskelynite, chromite, ilmenite, iron sulfide, and merrillite. These features reflect both its Martian volcanic origin and the intense shock processes involved in its launch from Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"1029\" data-end=\"1521\"\u003eFor collectors, Smeïra 003 offers a scarce opportunity to acquire a recently approved Martian meteorite with strong scientific and visual interest. Its low total known weight, Algerian provenance, and olivine-phyric Shergottite classification make it especially appealing for focused Mars collections and rare planetary meteorite displays. Each specimen represents genuine material from Mars, preserving part of the planet’s volcanic history and its journey from the Martian surface to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53721899794758,"sku":"MST-08\/07","price":844.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Smeira0807-4.jpg?v=1732287368"},{"product_id":"nwa-13187-martian-shergottite-diabasic-6-26g","title":"NWA 13187 - Martian Shergottite (Diabasic) - Complete Slice - 6.26g - Northwest Africa","description":"\u003cp data-start=\"119\" data-end=\"549\"\u003eNWA 13187 is a Martian Shergottite purchased in Morocco in 2019, with a reported total known weight of 1.6 kg. As a Shergottite, it represents basaltic igneous material from Mars, formed through volcanic processes before being ejected from the planet by a powerful impact event. Its Martian origin is supported by its classification and mineral chemistry, placing it within one of the main recognised groups of Martian meteorites.\u003c\/p\u003e\n\u003cp data-start=\"551\" data-end=\"962\"\u003eSpecimens of NWA 13187 typically show a grey to dark, speckled interior with a diabasic igneous texture. Reported mineralogy includes zoned clinopyroxene and other phases consistent with Martian Shergottites, giving prepared slices and fragments a distinctive crystalline appearance. Some pieces may retain desert-weathered exterior surfaces, while cut faces reveal the internal volcanic structure more clearly.\u003c\/p\u003e\n\u003cp data-start=\"964\" data-end=\"1418\"\u003eFor collectors, NWA 13187 offers a recognised Martian meteorite with strong scientific interest and relatively limited available material. Its Shergottite classification, 2019 recovery history, and clear Martian context make it appealing for collections focused on planetary meteorites, Mars material, or rare Achondrites. Each specimen represents a genuine piece of Mars, formed by volcanic activity and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722042564934,"sku":"MST-07\/17","price":999.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/NWA1318701-1.jpg?v=1732288289"},{"product_id":"nwa-13187-martian-shergottite-diabasic-6-36g","title":"NWA 13187 - Martian Shergottite (Diabasic) - Complete Slice - 6.36g - Northwest Africa","description":"\u003cp data-start=\"119\" data-end=\"549\"\u003eNWA 13187 is a Martian Shergottite purchased in Morocco in 2019, with a reported total known weight of 1.6 kg. As a Shergottite, it represents basaltic igneous material from Mars, formed through volcanic processes before being ejected from the planet by a powerful impact event. Its Martian origin is supported by its classification and mineral chemistry, placing it within one of the main recognised groups of Martian meteorites.\u003c\/p\u003e\n\u003cp data-start=\"551\" data-end=\"962\"\u003eSpecimens of NWA 13187 typically show a grey to dark, speckled interior with a diabasic igneous texture. Reported mineralogy includes zoned clinopyroxene and other phases consistent with Martian Shergottites, giving prepared slices and fragments a distinctive crystalline appearance. Some pieces may retain desert-weathered exterior surfaces, while cut faces reveal the internal volcanic structure more clearly.\u003c\/p\u003e\n\u003cp data-start=\"964\" data-end=\"1418\"\u003eFor collectors, NWA 13187 offers a recognised Martian meteorite with strong scientific interest and relatively limited available material. Its Shergottite classification, 2019 recovery history, and clear Martian context make it appealing for collections focused on planetary meteorites, Mars material, or rare Achondrites. Each specimen represents a genuine piece of Mars, formed by volcanic activity and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722170523974,"sku":"MST-07\/18","price":1015.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/NWA1318702-2.jpg?v=1732288702"},{"product_id":"amgala-001-shergottite-olivine-phyric-1-02g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 1.02g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722471268678,"sku":"MSA-02\/14","price":109.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/AmgalaReiker01-03_7524ef85-7980-4143-8ada-28a7f8c81965.jpg?v=1732291298"},{"product_id":"amgala-001-shergottite-olivine-phyric-2-37g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 2.37g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722494173510,"sku":"MSA-02\/17","price":253.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Amgala_Reiker_02-10.jpg?v=1732292436"},{"product_id":"amgala-001-shergottite-olivine-phyric-1-34g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 1.34g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722506494278,"sku":"MSA-02\/11","price":142.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Amgala_Reiker_03-2.jpg?v=1732292360"},{"product_id":"amgala-001-shergottite-olivine-phyric-1-25g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 1.25g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722512294214,"sku":"MSA-02\/09","price":133.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/AmgalaReiker04-02_a1ced3ed-45de-407b-98f4-d77c1facd10c.jpg?v=1732292491"},{"product_id":"amgala-001-shergottite-olivine-phyric-0-99g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 0.99g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722527105350,"sku":"MSA-02\/19","price":105.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/AmgalaReiker05-01.jpg?v=1732292687"},{"product_id":"amgala-001-shergottite-olivine-phyric-1-88g","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 1.88g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722529988934,"sku":"MSA-02\/07","price":200.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/AmgalaReiker06-1.jpg?v=1732292801"},{"product_id":"amgala-001-shergottite-olivine-phyric-3-24g-2pc","title":"Amgala 001 - Martian Shergottite (Olivine-Phyric) - 2pc - 3.24g - Western Sahara","description":"\u003cp data-start=\"26\" data-end=\"491\"\u003eAmgala 001 is a Martian Shergottite found near Meharrize in Saguia el Hamra, Western Sahara, with multiple stones recovered in December 2022. It is officially classified as a Martian meteorite, specifically a Shergottite, placing it within the main group of volcanic meteorites from Mars. Reported recovered material totals around 34.67 kg, including a largest individual of 5.2 kg, making it a significant modern Martian find. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"493\" data-end=\"996\"\u003eSpecimens of Amgala 001 typically show a weathered brown exterior with a knobby surface, while fresh interiors can appear greenish grey with darker olivine phenocrysts. Its mineralogy includes zoned olivine, clinopyroxene, maskelynite, and accessory phases, with opaque shock veins and secondary calcite veinlets recorded in descriptions. These features reflect both its Martian volcanic origin and the intense shock event that launched it from the surface of Mars. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"998\" data-end=\"1460\"\u003eFor collectors, Amgala 001 offers a recognised and relatively recent Martian meteorite with strong scientific and visual interest. Its Shergottite classification, substantial recovered mass, and distinctive greenish-grey interior make it appealing for collections focused on Mars material or planetary Achondrites. Each specimen represents genuine Martian rock, formed by volcanic processes on another planet and delivered to Earth after a journey through space.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":53722535559494,"sku":"MSA-01\/15","price":344.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/AmgalaReiker09-11.jpg?v=1732292901"},{"product_id":"nwa-15856-21-27-g-copy","title":"NWA 15856 - Eucrite - Complete Slice - 25.47g - Mauritania","description":"\u003cp data-start=\"26\" data-end=\"450\"\u003eNWA 15856 is a Polymict Eucrite found near Ouargla, Algeria, in 2020 and officially classified as an HED Achondrite. As a Eucrite, it is part of the meteorite family strongly linked to asteroid 4 Vesta, representing basaltic crustal material from an early differentiated body. The Meteoritical Bulletin records NWA 15856 as a single 530 g stone, with its main mass held by Sean Mahoney. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"452\" data-end=\"978\"\u003eSpecimens of NWA 15856 show a brecciated texture, with angular to sub-rounded cumulate and basaltic Eucrite clasts set within a fine-grained fragmental matrix. Minor Diogenite clasts are also present, making up less than 10 percent by volume, along with accessory phases including silica-rich glass, troilite, and iron-nickel metal. The original stone is described as having heavily weathered fusion crust over around 60 percent of its surface, with desert varnish covering the remainder. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"980\" data-end=\"1407\"\u003eFor collectors, NWA 15856 offers a scarce and well-documented Vestan Achondrite with strong visual and scientific interest. Its Polymict Eucrite classification records impact mixing on Vesta’s crust, while its single-stone recovery and limited total mass add to its appeal. Each specimen represents ancient basaltic material from asteroid 4 Vesta, shaped by volcanic activity, impact processing, and eventual delivery to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56131745120582,"sku":"EUC-06\/08","price":271.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/EucriteNWA1585602-1.jpg?v=1773063483"},{"product_id":"nwa-15856-18-49-g","title":"NWA 15856 - Eucrite - Complete Slice - 26.44g - Mauritania","description":"\u003cp data-start=\"26\" data-end=\"450\"\u003eNWA 15856 is a Polymict Eucrite found near Ouargla, Algeria, in 2020 and officially classified as an HED Achondrite. As a Eucrite, it is part of the meteorite family strongly linked to asteroid 4 Vesta, representing basaltic crustal material from an early differentiated body. The Meteoritical Bulletin records NWA 15856 as a single 530 g stone, with its main mass held by Sean Mahoney. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"452\" data-end=\"978\"\u003eSpecimens of NWA 15856 show a brecciated texture, with angular to sub-rounded cumulate and basaltic Eucrite clasts set within a fine-grained fragmental matrix. Minor Diogenite clasts are also present, making up less than 10 percent by volume, along with accessory phases including silica-rich glass, troilite, and iron-nickel metal. The original stone is described as having heavily weathered fusion crust over around 60 percent of its surface, with desert varnish covering the remainder. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"980\" data-end=\"1407\"\u003eFor collectors, NWA 15856 offers a scarce and well-documented Vestan Achondrite with strong visual and scientific interest. Its Polymict Eucrite classification records impact mixing on Vesta’s crust, while its single-stone recovery and limited total mass add to its appeal. Each specimen represents ancient basaltic material from asteroid 4 Vesta, shaped by volcanic activity, impact processing, and eventual delivery to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56131835691334,"sku":"EUC-06\/12","price":282.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/EucriteNWA1585603-3.jpg?v=1773064497"},{"product_id":"tatahouine-diogenite-tunisia-1-56-g-copy","title":"Tatahouine - Diogenite - Fragment - 1.84g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132539547974,"sku":"TAT-02\/18","price":61.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine03-7.jpg?v=1773073192"},{"product_id":"tatahouine-diogenite-tunisia-2-33-g","title":"Tatahouine - Diogenite - Fragment - 2.33g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132857102662,"sku":"TAT-02\/19","price":77.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine03-8.jpg?v=1773074150"},{"product_id":"tatahouine-diogenite-tunisia-1-76-g","title":"Tatahouine - Diogenite - Fragment - 1.76g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132878532934,"sku":"TAT-02\/25","price":59.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine04-8.jpg?v=1773074653"},{"product_id":"tatahouine-diogenite-tunisia-2-33-g-1","title":"Tatahouine - Diogenite - Fragment - 2.33g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132943708486,"sku":"TAT-02\/26","price":77.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine04-7.jpg?v=1773074807"},{"product_id":"tatahouine-diogenite-tunisia-1-67-g","title":"Tatahouine - Diogenite - Fragment - 1.67g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132945838406,"sku":"TAT-02\/28","price":56.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine01-8.jpg?v=1773074903"},{"product_id":"tatahouine-diogenite-tunisia-1-67-g-copy","title":"Tatahouine - Diogenite - Fragment - 1.63g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132958519622,"sku":"TAT-02\/38","price":55.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine02-7.jpg?v=1773075074"},{"product_id":"tatahouine-diogenite-tunisia-1-63-g-copy","title":"Tatahouine - Diogenite - Fragment - 1.79g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56132983292230,"sku":"TAT-02\/42","price":60.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine05-8.jpg?v=1773075239"},{"product_id":"tatahouine-diogenite-tunisia-1-79-g-copy","title":"Tatahouine - Diogenite - Fragment - 1.53g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133017338182,"sku":"TAT-02\/46","price":51.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine02-8.jpg?v=1773075455"},{"product_id":"tatahouine-diogenite-tunisia-1-64-g","title":"Tatahouine - Diogenite - Fragment - 1.64g - Tunisia","description":"\u003cp data-start=\"26\" data-end=\"486\"\u003eTatahouine is a historic witnessed Diogenite fall from Tunisia, which fell near Foum Tatahouine on 27 June 1931. The fall was reported after a low atmospheric explosion, scattering many small fragments over an area northeast of the village. As a Diogenite, Tatahouine belongs to the HED Achondrite family, strongly associated with asteroid 4 Vesta, and represents material from deeper within Vesta’s crust or upper mantle. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"488\" data-end=\"918\"\u003eSpecimens of Tatahouine are typically pale green to yellow-green, with dark shock veins and a crystalline texture dominated by orthopyroxene. Most recovered material consists of small angular fragments, with larger pieces being particularly uncommon. Its distinctive colour, fragile nature, and historic fall provenance make it one of the most recognisable Diogenites available to collectors. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"920\" data-end=\"1345\"\u003eFor collectors, Tatahouine offers a rare combination of witnessed fall history, classic HED classification, and strong visual character. Its connection to Vesta, limited recovered mass, and long-standing scientific interest make it especially appealing for Achondrite, witnessed fall, and historic meteorite collections. Each specimen represents ancient Vestan material connected to a clearly documented fall in North Africa.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133063278918,"sku":"TAT-02\/48","price":55.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Tatahouine01-7.jpg?v=1773075620"},{"product_id":"taoudenni-diogenite-slice-15-5-g","title":"Taoudenni - Diogenite - Fragment - 15.5g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133136580934,"sku":"TDN-01\/10","price":186.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni04-3.jpg?v=1773079505"},{"product_id":"taoudenni-diogenite-slice-14-1-g","title":"Taoudenni - Diogenite - Fragment - 14.1g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133149458758,"sku":"TDN-01\/15","price":169.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taudenni12-5.jpg?v=1773078894"},{"product_id":"taoudenni-diogenite-slice-14-1-g-copy","title":"Taoudenni - Diogenite - Fragment - 54g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133167546694,"sku":"TDN-01\/18","price":646.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni03-3.jpg?v=1773078995"},{"product_id":"taoudenni-diogenite-slice-38-g","title":"Taoudenni - Diogenite - Fragment  - 38g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133173772614,"sku":"TDN-01\/20","price":455.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni09-5_c811fc62-cc37-4496-92b4-3b00d4fb7ad0.jpg?v=1773079148"},{"product_id":"taoudenni-diogenite-slice-15-8-g","title":"Taoudenni - Diogenite - Fragment  - 15.8g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133202215238,"sku":"TDN-01\/22","price":189.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni01-2.jpg?v=1773079652"},{"product_id":"taoudenni-diogenite-slice-16-3-g","title":"Taoudenni - Diogenite - Fragment - 16.3g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133204771142,"sku":"TDN-01\/23","price":196.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni10-4.jpg?v=1773079784"},{"product_id":"taoudenni-diogenite-slice-19-4-g","title":"Taoudenni - Diogenite - Fragment - 19.4g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133208965446,"sku":"TDN-01\/24","price":233.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni02-3.jpg?v=1773079932"},{"product_id":"taoudenni-diogenite-slice-15-2-g","title":"Taoudenni - Diogenite - Fragment - 15.2g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133211128134,"sku":"TDN-01\/25","price":182.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taoudenni05-05.jpg?v=1773080030"},{"product_id":"taoudenni-diogenite-slice-7-6-g","title":"Taoudenni - Diogenite - Fragment - 7.6g - Mali","description":"\u003cp data-start=\"26\" data-end=\"435\"\u003eTaoudenni is a Diogenite from northern Mali, found in 2007 around 15 km north of the Taoudenni salt mines. As part of the HED Achondrite family, it is linked to asteroid 4 Vesta and represents material from deeper within Vesta’s crust or upper mantle. A single stone of 24.37 kg was recovered, giving Taoudenni a limited but well-documented place among Vestan meteorites. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"437\" data-end=\"934\"\u003eSpecimens of Taoudenni are typically greenish-grey to pale grey and show the coarse, crystalline texture expected of a Diogenite. The meteorite is composed mainly of orthopyroxene, with minor olivine reported in some descriptions, reflecting slow crystallisation within its parent body before later impact excavation. Some material may retain patches of fusion crust, while prepared fragments and slices reveal the crystalline internal structure more clearly. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"936\" data-end=\"1363\"\u003eFor collectors, Taoudenni offers a recognised and relatively scarce Diogenite with strong planetary significance. Its connection to Vesta, limited recovered mass, and attractive crystalline texture make it appealing for collections focused on Achondrites, HED meteorites, or differentiated asteroid material. Each specimen represents ancient Vestan rock, formed deep within an early planetary body and later delivered to Earth.\u003c\/p\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56133216469318,"sku":"TDN-01\/30","price":90.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Taudenni13-5.jpg?v=1773080177"},{"product_id":"lunar-bechar-feldspathic-breccia-1-32-g","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.32g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141591380294,"sku":"BEC-08\/09","price":56.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0809-6.jpg?v=1773234450"},{"product_id":"lunar-bechar-feldspathic-breccia-1-88-g","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.88g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141595148614,"sku":"BEC-08\/14","price":80.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0814-5.jpg?v=1773314873"},{"product_id":"lunar-bechar-feldspathic-breccia-1-88-g-copy","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.44g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141655703878,"sku":"BEC-08\/11","price":61.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0811-7.jpg?v=1773314809"},{"product_id":"lunar-bechar-feldspathic-breccia-1-86-g","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.86g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141656883526,"sku":"BEC-08\/17","price":80.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0817-6.jpg?v=1773313800"},{"product_id":"lunar-bechar-feldspathic-breccia-1-42-g","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.42g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141688275270,"sku":"BEC-08\/21","price":60.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0805-6_b9e22f8d-19b6-4f4b-b9fa-090628c300cc.jpg?v=1773314711"},{"product_id":"lunar-bechar-feldspathic-breccia-1-19-g","title":"Bechar 003 - Lunar Feldspathic Breccia - Fragment - 1.19g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"120\" data-end=\"560\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space.\u003c\/p\u003e\n\u003cp data-start=\"562\" data-end=\"1020\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands.\u003c\/p\u003e\n\u003cp data-start=\"1022\" data-end=\"1439\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56141690503494,"sku":"BEC-08\/27","price":51.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar0827-6.jpg?v=1773313320"},{"product_id":"lunar-bechar-feldspathic-breccia-1-26-g","title":"Bechar 003 - Lunar Feldspathic Breccia - End Cut - 1.26g - Algeria","description":"\u003cdiv class=\"flex-shrink-0 flex flex-col relative items-end\"\u003e\n\u003cdiv class=\"pt-0\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke flex h-8 w-8 items-center justify-center overflow-hidden rounded-full\"\u003e\n\u003cdiv class=\"h-full w-full\"\u003e\n\u003cdiv class=\"gizmo-shadow-stroke overflow-hidden rounded-full\"\u003e\n\u003cp data-start=\"26\" data-end=\"504\"\u003eBechar 003 is a Lunar Feldspathic Breccia found near Bechar, Algeria, in 2022. It belongs to a group of likely paired Lunar meteorites from the same region, sometimes referred to as the Bechar 003 clan, which includes several closely related stones. As a Feldspathic Breccia, it represents fragmented material from the Moon’s ancient highland crust, formed and reworked by repeated impact events before a later impact ejected it into space. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"506\" data-end=\"1002\"\u003eSpecimens of Bechar 003 typically show light brown weathered exteriors and medium grey interiors with small pale clasts. Many stones lack fusion crust, consistent with the published descriptions of the find. Prepared fragments and slices can reveal the brecciated lunar texture more clearly, with feldspar-rich material and impact-processed clasts set within a finer matrix. This structure reflects the long and complex impact history of the Lunar Highlands. \u003cspan class=\"\" data-state=\"closed\"\u003e\u003c\/span\u003e\u003c\/p\u003e\n\u003cp data-start=\"1004\" data-end=\"1421\"\u003eFor collectors, Bechar 003 offers a recognised and accessible Lunar meteorite with strong scientific context and attractive brecciation. Its official classification, Algerian provenance, and connection to the ancient Moon make it especially appealing for Lunar collections. Each specimen represents genuine Moon rock, preserving material from the lunar highlands and the billions of years of impacts that shaped them.\u003c\/p\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e\n\u003c\/div\u003e","brand":"OuterSpacer Meteorites","offers":[{"title":"Default Title","offer_id":56161664926022,"sku":"BEC-15\/25","price":67.0,"currency_code":"EUR","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/files\/Bechar_1525-5.jpg?v=1773317540"}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0757\/0518\/8678\/collections\/20200528_220146.jpg?v=1723380823","url":"https:\/\/outerspacer.com\/collections\/achondrites.oembed?page=3","provider":"OuterSpacer Meteorites","version":"1.0","type":"link"}