On Offer: MARTIAN AUGITE BASALT METEORITE 0.64g | NWA 8159 | Worlds Rarest Martian Meteorite Type: Augite Basalt Origin: MARS Official name: NWA 8159 Description: 0.64 gram partial slice of perhaps the rarest martian meteorite ever discovered; NWA 8159 Martian Augite Basalt meteorite. This meteorite represents a unique ejection event on Mars, not related to the SNC group, the martian breccias or any other known martian meteorite. Only 149 grams of this meteorite has ever been recovered and is perhaps the rarest most significant martian meteorite discovered to date. This is a piece of Mars ejected by another meteorite impacting the surface of the Red Planet and hurling it to Earth. What you get: 0.64g NWA 8159 Martian Meteorite Specimen as Shown, Membrane Storage/Display Box, & signed 5x7 double sided color Certificate of Authenticity. I offer a 100% no questions asked 15 day return policy. SEE OFFICIAL METEORITICAL SOCIETY ENTRY BELOW
Northwest Africa 8159 | |||||||||||||||||||||
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Basic information | Name: Northwest Africa 8159 This is an OFFICIAL meteorite name. Abbreviation: NWA 8159 Observed fall: No Year found: 2013 Country: Morocco Mass: 149.4 g | ||||||||||||||||||||
Classification history: |
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Comments: | Approved 10 Dec 2013 | ||||||||||||||||||||
Writeup |
Writeup from MB 102:
Northwest Africa 8159 (NWA 8159) Morocco Purchased: 2013 Classification: Martian (augite basalt) History: Purchased by Brahim Tahiri from a Moroccan hunter and sent to his partner Sean Tutorow for classification in 2013. Physical characteristics: Single stone, weathered exterior with yellow-brown patina, light colored desert soil coating on one side. Saw cut reveals a very fine-grained, gray-green interior, with a few small melt veins present, but one vein was up to 1 mm thick, lithology offsets at vein boundaries suggest slight brecciation. Petrography: (C. Agee, UNM ) Microprobe examination of a two polished mounts shows intergranular texture with approximately 50% augite, 40% plagioclase and maskelynite, 5% olivine. Augites have equant habits 10-200 μm with igneous zoning. Some augite crystals are rimmed with Fs-rich orthopyroxene. Plagioclase with shock-fractured prismatic laths up to 500 × 100 μm, but many are smaller (~50 × 10 μm), approximately half of the plagioclase has been converted to maskelynite, and is observed as unfractured, glassy casts. Olivine ~100 μm, most with resorbed or coronal grain boundaries. Ubiquitous magnetite, most grains 10-100 μm. Minor ilmenite, merrillite, Cl-apatite, and Cr-spinel. Trace calcite and barite assumed to be desert weathering products. Geochemistry: (C. Agee, N. Muttik, F. McCubbin, UNM ) EMPA. Augite Fs38.6±11Wo30.4±11.0, Fe/Mn=36±4, n=78; orthopyroxene rims Fs62.3±5.9Wo0.6±0.3, Fe/Mn=23±3, n=6; plagioclase An58.2±2.3Ab41.5±2.4Or0.3±0.2, n=7; maskelynite An58.1±1.8Ab41.6±1.7Or0.2±0.0, n=5; olivine Fa66.2±3.8, Fe/Mn=50±5, n=15; large shock melt vein (mean value from EMPA with 20 μm beam) SiO2=46.14±0.94, TiO2=0.67±0.09, Al2O3=10.63±1.22, Cr2O3=0.14±0.02, FeO=24.89±1.92, MnO=0.50±0.04, MgO=4.02±0.39, CaO=9.10±0.38, Na2O=1.80±0.17, P2O5=0.29±0.03, Cl=0.067±0.022 (all wt%), n=10. (Karen Ziegler, UNM ) Oxygen isotope values of 5 acid-washed aliquots of bulk sample, 1.2, 1.2, 1.8, 2.0, 1.0 mg, gave δ17O = 2.406, 2.405, 2.093, 2.532, 2.329, δ18O = 4.089, 3.947, 3.328, 4.197, 3.880, Δ17O = 0.247, 0.321, 0.336, 0.316, 0.280 (linearized, all permil). Classification: Martian (augite basalt). This is a martian meteorite based on oxygen isotopes, Fe/Mn of augite and olivine, and An-content of plagioclase and maskelynite. This martian meteorite is a fine grained olivine-bearing augite basalt that does not appear to be a SNC type although there are some aspects of it that resemble SNC. The augite and olivine compositions and crystallization trends are similar to nahklites, in particular MIL03346. It does not resemble most shergottites in that pigeonite is absent, and orthopyroxene is only a minor phase present as Fe-rich rims on some augite grains, however plagioclase compositions are similar to shergottites, in particular the low potassium labradorites in QUE94201. Shock pressures appear to have been lower than for shergottites, perhaps similar to Chassigni and some nakhlites, as only about half the plagioclase has been transformed to maskelynite. Magnetite is the dominant oxide phase in this meteorite, the only other martian meteorite that shares this aspect is basaltic breccia NWA7034 and its pairings. Specimens: 24.57 g including a two probe mounts on deposit at UNM , Reed holds 2.21 g, Sean Tutorow holds the main mass. | ||||||||||||||||||||
Data from: MB102 Table 0 Line 0: |
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