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Mercantour | |||||||||||||||||||||||||||||||||
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Basic information | Name: Mercantour This is NOT an official name: Discredited meteorite. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2014 Country: France Mass: ![]() | ||||||||||||||||||||||||||||||||
Classification history: |
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Comments: |
Entered 15 May 2016 Revised 2 Nov 2016: | ||||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from MB 105:
Mercantour 44.145°N, 7.311°E Provence-Alpes-Cote d’Azur, France Find: 2014 Sept 25 Classification: Ordinary chondrite (L4-6) History: A systematic search of moraines and rocky surfaces by Eric Paillery led to this single discovery in the Southern Alps granitic massif, within Mercantour National Park, near 2900 m elevation. Physical characteristics: A single angular fragment, covered ~30% by a relatively fresh fusion crust. Gray color with minor rust spots. Inner surface sometimes covered by a carbonate rind. Little patina visible. A few small rounded quartz grains inserted in cracks, with a light-orange soil matrix. Petrography: Breccia with type 4 to 6 clasts (major class 4 to 5). Distinguishing type 4, 5 and 6 was done based on polished section observation of the morphology and overall texture of chondrules and metal grains. Mean chondrule diameter 707±39 μm. One fine-grained clast with low metal and troilite content was observed. Weathering at microscopic scale is hardly detectable but macroscopic rust spots indicate W1. Geochemistry: Type 6 lithology: olivine Fa27.7 (n=1), orthopyroxene Fs21.2Wo0.7 (n=1). Type 4 lithology: olivine Fa24.7 (n=1), orthopyroxene Fs20.2Wo2.1 (n=1). Classification: in the L group is based on magnetic susceptibility and chondrule size. Petrography (SEM and reflected optical microscopy) indicates a L4-6 breccia. Specimens: 22.6 g at CEREGE. Writeup from MB 107: Mercantour: name discredited.
Mercantour has been abolished as a meteorite name due to significant doubt about the location and date of the find. As reported in Rochette et al. (2017), trace elements measurements (M. D’Orazio, UPisa) reveal a signature similar to that observed in meteorites found in hot deserts, with significant Ba and Sr enrichment. This meteorite is now called Nova 054. [Editor's note, 3 July 2020: information submitted by L. Ferrière] | ||||||||||||||||||||||||||||||||
Bibliography: |
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Data from: MB105 Table 0 Line 0: |
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Institutions and collections |
CEREGE: CEREGE
BP 80
Avenue Philibert, Technopole de l'Arbois
13545 Aix-en-Provence Cedex 4
France, France (institutional address; updated 29 Oct 2018) LPI: Lunar and Planetary Institute, 3600 Bay Area Blvd., Houston, TX 77058 , United States; Website (institutional address; updated 20 Jun 2022) UPisa: Dipartimento di Scienze della Terra, Università di Pisa, Italy (institutional address; updated 3 Aug 2010) |
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References: | Published in Meteoritical Bulletin, no. 105, MAPS 52, 2411, September 2017. http://onlinelibrary.wiley.com/doi/10.1111/maps.12944/full Published in Meteoritical Bulletin, no. 107, MAPS 55, 460-462
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