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Northwest Africa 13088 | |||||||||||||||||||||||||||||||
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Basic information | Name: Northwest Africa 13088 This is an OFFICIAL meteorite name. Abbreviation: NWA 13088 Observed fall: No Year found: 2017 Country: Morocco Mass: ![]() | ||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 17 approved meteorites classified as L3.1. [show all] Search for other: L chondrites, L chondrites (type 3), Ordinary chondrites, and Ordinary chondrites (type 3) | ||||||||||||||||||||||||||||||
Comments: | Approved 31 Jan 2020 | ||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 109:
Northwest Africa 13088 (NWA 13088) Morocco Purchased: 2017 Classification: Ordinary chondrite (L3.1) History: Purchased in Morocco by Brahim Tahiri in late 2017 and brought to Sean Tutorow in late December 2017. Tutorow donated 94.40 g to Cascadia for classification. Physical characteristics: Cascadia received two thin slices completely covered in a coating which darkens the sample and causes it to appear wet. Overall, the slices are dark orange-brown in color and show abundant chondrules. Some areas have chondrules set in an orange-brown background, while in other areas the background is dark brown to black. Boundaries between the two are generally indistinct, although there is one example of a sharp contact between a large (4 × 3 cm, truncated along the edge of the slice), angular, orange-brown colored clast and the rest of the slice, indicating that this sample is brecciated. Petrography: (M. Hutson and A. Ruzicka, Cascadia): The section is crossed by numerous weathering veins composed of calcite and iron-rich hydroxides. One edge of the section is less weathered and shows abundant discolored and partially-replaced troilite, much of it as rims around chondrules. Chondrules are distinct, and have an apparent mean diameter of 756±366 microns (N= 113). Two subtly different lithologies with indistinct boundaries are visible in thin section in optical and BSE imaging. One lithology (lithology A) has a somewhat higher proportion of forsteritic olivine grains than the other (lithology B); the overall lithology A clast appears slightly darker in BSE imaging. Chondrule mesostases in lithology A contain fewer crystallites than those of lithology B. Geochemistry: Mineral compositions and geochemistry: Olivine and pyroxene grains are highly unequilibrated: Fa17.7±10.7N=161; Fs11.5±10.1Wo1.0±1.1, N=82. There is no significant difference in Fa or Fs contents between the two lithologies. However, Cr2O3 in olivine suggests a slightly different petrographic subtype: Cr2O3 in olivine (lithology A) = 0.42±0.19 wt%, consistent with a subtype of 3.10, N=72; Cr2O3 in olivine (lithology B) = 0.19±0.21 wt%, consistent with a subtype of 3.15, N=84. Classification: Ordinary chondrite (L3.1) based on olivine fayalite content, overall Cr2O3 in olivine, and mean chondrule diameter. Specimens: Cascadia holds 90.3 g in six pieces, in addition to a polished thin section and a mounted butt. The main mass is held by Sean Tutorow, Arizona. | ||||||||||||||||||||||||||||||
Data from: MB109 Table 0 Line 0: |
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Institutions and collections |
Cascadia: Cascadia Meteorite Laboratory, Portland State University, Department of Geology, Room 17 Cramer Hall, 1721 SW Broadway, Portland, OR 97201, United States; Website (institutional address; updated 28 Oct 2011) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 109, in preparation (2020)
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Photos: |
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Geography:![]() |
Statistics: This is 1 of 1973 approved meteorites from Morocco (plus 37 unapproved names) (plus 1 impact crater) |