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Sueilila 005 | |||||||||||||||||||||||||||||||||||||
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Basic information | Name: Sueilila 005 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2018 Country: Western Sahara Mass: 282 g | ||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 340 approved meteorites classified as Lunar (feldsp. breccia). [show all] Search for other: Lunar meteorites | ||||||||||||||||||||||||||||||||||||
Comments: | Approved 7 Nov 2019 | ||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 108:
Sueilila 005 24.658°N, 14.692°W Rio de Oro, Western Sahara Find: 2015-Apr Classification: Lunar meteorite (feldspathic breccia) History: The stone was found by two Moroccan hunters in April 2015 in a barren region. Further searching in the area led to the recovery of other similar-appearing stones totaling 15.6 kilograms, but this first stone was considered to be possibly different (because of the presence of some larger lithic clasts), and it was excluded from the classification of the other stones as a group under the name NWA 10495. Subsequently the first stone was sold by the finders to a Moroccan dealer, who in turn sold it in February 2018 at the Tucson Gem and Mineral Show to representatives of ArtAncient (a British antiquities dealer). Physical characteristics: A single, dark brown stone (282 g) lacking fusion crust but exhibiting a glossy weathering patina. Sawcuts reveal a very fine grained interior with diffuse larger whitish to black clasts. Petrography: (A. Irving and S. Kuehner, UWS; P. Carpenter, WUSL) Breccia consisting of sporadic gabbroic anorthosite and rare dunite clasts in a fine grained crystalline matrix. Minerals are anorthite, exsolved pigeonite, orthopyroxene, pigeonite, subcalcic augite, olivine, ilmenite, Ti chromite (with variable Ti content) and secondary barite. Geochemistry: Anorthite (An97.1-97.4Or0.0, N = 2), low-Ca pyroxene host (Fs50.1Wo6.0, FeO/MnO = 58), augite exsolution lamella (Fs25.1Wo40.9, FeO/MnO = 59), augite host (Fs26.6Wo40.2, FeO/MnO = 57), orthopyroxene exsolution lamella (Fs56.1Wo1.7, FeO/MnO = 55), orthopyroxene (Fs39.6-41.7Wo2.7-3.2, FeO/MnO = 59-63), pigeonite (Fs26.7Wo19.4, FeO/MnO = 55), subcalcic augite (Fs21.0-39.2Wo26.8-25.1, FeO/MnO = 46-59), olivine (Fa41.3-56.8, FeO/MnO = 89-99, N = 3), olivine in dunite clast (Fa46.7-48.0, FeO/MnO = 93-97, N =2). Classification: Lunar (feldspathic breccia). This specimen is from the same strewnfield as the NWA 10495 stones and is very likely paired with them. Specimens: 21.5 g in the form of two slices (one polished) at UWB; remainder with ArtAncient, Chelsea Creek, 31 Imperial Road, London SW6 2FR, UK. | ||||||||||||||||||||||||||||||||||||
Data from: MB108 Table 0 Line 0: |
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Institutions and collections |
UWS: University of Washington, Department of Earth and Space Sciences, 70 Johnson Hall, Seattle, WA 98195, United States (institutional address; updated 15 Jan 2012) WUSL: Washington Univ., One Brookings Drive, St. Louis, MO 63130, United States (institutional address; updated 17 Oct 2011) UWB: University of Washington, Burke Museum of Natural History and Culture, Box 353010 Seattle, WA 98195, United States (institutional address; updated 9 Oct 2023) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 108 (2020) Meteorit. Planet. Sci. 55, 1146-1150
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Geography: |
Statistics: This is 1 of 50 approved meteorites from Rio de Oro, Western Sahara This is 1 of 280 approved meteorites from Western Sahara (plus 20 unapproved names) | ||||||||||||||||||||||||||||||||||||
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Revision history: |
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