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Northwest Africa 8190 | |||||||||||||||||||||||||||||
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Basic information | Name: Northwest Africa 8190 This is an OFFICIAL meteorite name. Abbreviation: NWA 8190 Observed fall: No Year found: 2007 Country: (Northwest Africa) Mass: 660 g | ||||||||||||||||||||||||||||
Classification history: |
This is 1 of 86 approved meteorites classified as CK3. [show all] Search for other: Carbonaceous chondrites, Carbonaceous chondrites (type 3), CK chondrites, CK3 chondrites, and CV-CK clan chondrites | ||||||||||||||||||||||||||||
Comments: | Approved 24 Feb 2014 | ||||||||||||||||||||||||||||
Writeup |
Writeup from MB 103:
Northwest Africa 8190 (NWA 8190) (Northwest Africa) Purchased: 2007 Classification: Carbonaceous chondrite (CK3) Physical characteristics: Many pieces with a light brown weathered surface. This zone of severe weathering forms an up to 2 mm thick shell around each sample. Fractured surfaces are dark brown with blurred chondrules up to 3 mm in size. CAIs with sizes up to 8 mm have been observed. Very compact interior without any visible porosity. Petrography: (K. Metzler, IfP) The investigated sample consists of two distinct lithologies with sharp contact. The groundmass of both lithologies shows a fine-grained recrystallized texture, consisting of olivine grains and fewer pyroxene and plagioclase grains with sizes on the order of 50-100 μm. Magnetite and weathered sulfides are concentrated in the interstices and around larger objects like chondrules. Lithology 1 contains only sparse chondrules while lithology 2 contains subequal amounts of matrix and chondrules+CAIs. Many chondrules show rims of weathered opaque phases. Several large chondrules show relict Mg-rich olivine (Fa0.5-1) in the center and Fe-rich olivine at the margin. Geochemistry: (K. Metzler, IfP) The mean composition of olivine (except chondrule cores) is Fa32.8 (Fa28-38). Olivine grains contain about 0.5 wt% NiO (0.2-07 wt%). Olivine in chondrule cores is Ni-free and retained its original Mg-rich composition (Fa0.5-1). Low-Ca pyroxene is less abundant, with a range of compositions (Fs2-27). It is rich in Al with a mean concentration of about 4 wt% Al2O3. Ca-rich pyroxene also occurs. The compositional range of feldspar is An25.5-43.5. Magnetite is the most abundant opaque phase, with significant concentrations of elements other than Fe (n=2): MgO 1-1.5 wt%; Al2O3 3-3.5 wt%; TiO2 1 wt%; Cr2O3 3.5 wt%; NiO 0.5 wt%. The magnetite composition is characteristic for CK chondrites. Classification: CK chondrite based on mineral chemistry. Petrologic type (3.9) based on olivine variability (PMD=6) | ||||||||||||||||||||||||||||
Data from: MB103 Table 0 Line 0: |
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Institutions and collections |
IfP: Institut für Planetologie, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany (institutional address; updated 23 Jan 2012) Hmani: A. Hmani Moroccan Imports, 13 rue Jules Hardouin Mansart, 92600 Asnières, France (private address) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 103, MAPS 52, 1014, May 2017, http://onlinelibrary.wiley.com/doi/10.1111/maps.12888/full
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Geography: |
Statistics: This is 1 of 9699 approved meteorites from (Northwest Africa) (plus 1854 unapproved names) | ||||||||||||||||||||||||||||
Also see: |
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Revision history: |
This lists important revisions made to data for this record.
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