|
Northwest Africa 11040 | |||||||||||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Basic information | Name: Northwest Africa 11040 This is an OFFICIAL meteorite name. Abbreviation: NWA 11040 Observed fall: No Year found: 2016 Country: (Northwest Africa) Mass: 13 g | ||||||||||||||||||||||||
Classification history: |
This is 1 of 138 approved meteorites classified as Eucrite-unbr. [show all] Search for other: Achondrites, Eucrites, and HED achondrites | ||||||||||||||||||||||||
Comments: | Approved 13 Jan 2017 | ||||||||||||||||||||||||
Writeup |
Writeup from MB 106:
Northwest Africa 11040 (NWA 11040) (Northwest Africa) Purchased: 2016 Classification: HED achondrite (Eucrite, unbrecciated) History: A complete stone was purchased from Sean Tutorow’s eBay operation by Jason Utas Physical characteristics: One rough-surfaced, fusion crusted individual stone. Petrography: The texture is subophitic and unbrecciated. The mineralogy is typical eucritic (pyroxene and plagioclase with minor ilmenite, silica, Cr-spinel, troilite and trace olivine), except for an unusually high proportion of pure-Fe metal, originally roughly 0.6 vol%, although roughly 1/3 of that original metal has been replaced by Fe-oxides. Plagioclase is up to 4.8 mm in length (4.8 × 0.2 mm). Metal occurs dominantly as blocky grains, typically 0.1-0.2 mm across. Manifestations of thermal annealing, such as exsolution lamellae in pyroxene, are nearly undetectable, and about 30 vol% of the rock is mesostasis, so fine-grained as to appear opaque in transmitted light. The shock class is intermediate based on undulose extinction and planar fractures in pyroxene. Geochemistry: Pyroxenes are compositionally diverse and complex. For the most part, major-element compositions show a pattern typical of low-thermal-metamorphism eucrites (cf. Pasamonte), fanning out from a tight cluster at Fs29Wo5 (cores of larger grains) in the general direction of Fs45Wo30 (rims and fine-grained areas). However, in a few locales, pyroxene in fine-scale intergrowth with silica (pyroxene widths typically 1-3 microns) consists of a remarkably low-Ca variety, Fs49-51Wo1.0-1.5, along with a far lesser proportion of high-Ca composition (near Fs39Wo44). Also, curvy veinlike patches of oddly low-Ca composition (notably bright in backscattered electron images) are sprinkled within the cores of large pyroxenes. The average measured pyroxene composition (n=258) is Fs37Wo16 with FeO/MnO = 29±1.5. Plagioclase (n=23) is An79-91, average An84.6±3.4, excluding one anomalous analysis, An98. Olivine (n=5) is Fa69-71. Spinel (9 analyses of a single 0.6-mm grain) has Cr/(Al+Cr) ranging from 0.59-0.76. The Fe-metal has undetectable Ni (less than 0.1 wt%) and 0.15-0.23 wt% Co. INAA bulk-rock results include Na = 4.1 mg/g, Sc = 28 μg/g, Cr = 1.9 mg/g, Fe = 138 mg/g, Sm = 3.2 μg/g. Classification: The meteorite is an unbrecciated eucrite. | ||||||||||||||||||||||||
Data from: MB106 Table 0 Line 0: |
|
||||||||||||||||||||||||
Institutions and collections |
UCLA: Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, United States (institutional address; updated 17 Oct 2011) |
||||||||||||||||||||||||
Catalogs: |
| ||||||||||||||||||||||||
References: | Published in Gattacceca J., Bouvier A., Grossman J., Metzler K., and Uehara M. (2019) Meteoritical Bulletin, no. 106. Meteorit. Planet. Sci. 54 in press.
| ||||||||||||||||||||||||
Geography: |
Statistics: This is 1 of 9710 approved meteorites from (Northwest Africa) (plus 1853 unapproved names) | ||||||||||||||||||||||||
Also see: |
This lists the most popular meteorites among people who looked up this meteorite.
| ||||||||||||||||||||||||
Revision history: |
This lists important revisions made to data for this record.
|