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Tabas 001 | |||||||||||||||||||||||||||||||||||||
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Basic information | Name: Tabas 001 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2016 Country: Iran Mass: ![]() | ||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 8581 approved meteorites (plus 4 unapproved names) classified as L5. [show all] Search for other: L chondrites, L chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||||
Comments: | Approved 18 Dec 2017 | ||||||||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 106:
Tabas 001 33°39.12’N, 56°59.77’E Khorasan, Iran Find: 15 Jan 2016 Classification: Ordinary chondrite (L5) History: The meteorite was found in the desert of Iran by Mr. Zacharchuk and Mr. Kryachko in January 15, 2016. Physical characteristics: The meteorite is broken into 14 pieces. A dark-brownish, partly eroded fusion crust is present. Petrography: The meteorite has brecciated chondritic texture. The main mass (host) composes of chondrules fragments, mineral grains and minor well formed chondrules of 300-900 µm in diameter of BO, RP, PO, PP, POP, rare of C types, troilite (~3 vol%), minor metal FeNi, iron hydroxides, accessory chromite. The main mass contains of ~15 vol% of the angular rock clasts of 5-15 mm in size. Some of them are composed of brecciated chondritic material, similar to that of the host. The clasts of another type are comprised by recrystallized medium-grained aggregates of pyroxene, feldspar (up to 400 µm in size) and olivine, minor troilite and metal grains. Geochemistry: Mineral compositions and geochemistry: the host and fine-grained clasts are composed of olivine Fa24.9±0.3 (N=15) and pyroxene Fs20.5±0.1Wo1.5±0.2 (N=15); the medium-grained clasts are composed of Fa20.4±0.2 (N=15) and Fs17.4±0.2Wo2.6±0.8 (N=13). Classification: Based on the texture and composition, the meteorite is classified as ordinary chondrite breccia composed of L5 host with L5 and H7 clasts (L5 polymict breccia). Specimens: A type specimen of 962 g total weight and thin section are on deposit at Vernad, the finders hold the main mass. | ||||||||||||||||||||||||||||||||||||
Data from: MB106 Table 0 Line 0: |
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Institutions and collections |
Vernad: Vernadsky Institute of Geochemistry and Analytical Chemistry, Russia (institutional address; updated 21 Feb 2016) IGEM: Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry, Russian Academy of Sciences, Staromonetny Per., 35, Moscow, 119017 , Russia (institutional address; updated 16 Dec 2010) |
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Catalogs: |
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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.
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Photos: |
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Geography:![]() |
Statistics: This is 1 of 10 approved meteorites from Khorasan, Iran This is 1 of 373 approved meteorites from Iran (plus 1 unapproved name) | ||||||||||||||||||||||||||||||||||||
Proximity search: |