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Chug Chug 015 | |||||||||||||||||||||||||||||||||||||||
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Basic information | Name: Chug Chug 015 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2018 Country: Chile Mass: 3.06 kg | ||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 256 approved meteorites classified as H5/6. [show all] Search for other: H chondrites, H chondrites (type 4-7), Ordinary chondrites, and Ordinary chondrites (type 4-7) | ||||||||||||||||||||||||||||||||||||||
Comments: | Approved 16 Nov 2019 | ||||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 108:
Chug Chug 015 22°29.573’S, 69°14.896’W Antofagasta, Chile Find: 2018 Oct 16 Classification: Ordinary chondrite (H5/6) History: Meteorite (1 piece) was found on October 16, 2018, by Ilya Chaplygin during a desert meteorite search organized by Timur Kryachko. Physical characteristics: Single stone, 3055 g, with angular shape, flat sides, and rounded edges, covered with dull dark-brown fusion crust partly missing on the edges. One side is broken revealing solid brown surface. Bottom part is covered with light-colored desert material. Fresh cut of the meteorite is dark gray and exhibits lots of fine grained metal. Dimensions 10.5 × 15 × 8.5 cm. Petrography: (P. Yu. Plechov, FMMR). The meteorite contains rare relics of barred-olivine chondrules about 300 μm in diameter. Olivine, low-Ca pyroxene, plagioclase and metallic blebs are the main minerals in matrix. Metallic blebs (200-400 μm) have irregular shape and consist of kamacite, taenite and troilte. Plagioclase grains are about 50 µm. This indicates a petrological type of 5 or 6 for the meteorite. Olivine has no undulatory extinction, and opaque shock veins and melt pockets are absent, indicating a shock stage of S1. Rare dark-yellowish cracks (up to 1 mm in length) occur. Olivine, pyroxene, chromite, metal and troilite are fresh and not weathered. No oxidation rims around troilite or metal (weathering grade W0). Geochemistry: Mineral composition and Geochemistry: EDS analyses (V.I. Taskaev, IGEM RAS). The primary chondrite paragenesis includes olivine Fa18.8±0.3 (N=20), orthopyroxene Fs15.9±0.7Wo1.3±0.2 (N=15), plagioclase Ab82.1An11.5Or6.4 (N=2), clinopyroxene En49.3Fs5.5Wo45.1 (N=1). Composition of kamacite (in wt.%, N=12): Fe 93.5, Ni 5.6, Co 0.6. Taenite (N=9) contain 43.1 and 0.1 wt.% of Ni and Co, respectively. Classification: (P. Yu. Plechov, FMMR). Ordinary chondrite, H5/6, W0, S1 Specimens: Mr. I. Chaplygin holds main mass 2.5 kg. 475 g, FMMR. | ||||||||||||||||||||||||||||||||||||||
Data from: MB108 Table 0 Line 0: |
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Institutions and collections |
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) FMMR: Fersman Mineralogical Museum, Leninskiy prospekt 18 korpus 2, Moscow, Russia, 119071, Russia; Website (institutional address; updated 24 Feb 2018) |
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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 3442 approved meteorites from Antofagasta, Chile (plus 12 unapproved names) (plus 1 impact crater) This is 1 of 3471 approved meteorites from Chile (plus 13 unapproved names) (plus 1 impact crater) | ||||||||||||||||||||||||||||||||||||||
Proximity search: | |||||||||||||||||||||||||||||||||||||||
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Revision history: |
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