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Watson 013 | |||||||||||||||||||||||||||||||||||||||
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Basic information | Name: Watson 013 This is an OFFICIAL meteorite name. Abbreviation: There is no official abbreviation for this meteorite. Observed fall: No Year found: 2010 Country: Australia Mass: 47.1 g | ||||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 710 approved meteorites (plus 2 unapproved names) classified as H3. [show all] Search for other: H chondrites, H chondrites (type 3), Ordinary chondrites, and Ordinary chondrites (type 3) | ||||||||||||||||||||||||||||||||||||||
Comments: | Approved 28 Jan 2013 | ||||||||||||||||||||||||||||||||||||||
Writeup |
Writeup from MB 102:
Watson 013 30°34’30.0"S, 131°30’5.9"E South Australia, Australia Found: 14 Apr 2010 Classification: Ordinary chondrite (H3) History: Single piece found by A. Tomkins on the Nullarbor Plain. Petrography: (A. Tomkins, Monash) Well-defined chondrules (most <1 mm, some to 2 mm) in a highly porous light-colored transparent matrix; there is no matrix glass. Plagioclase to 20 μm. Chondrule types include RP, POP, PP, BO and PO; there are rare very finely recrystallized glassy chondrules. Chondrule mesostases finely recrystallized (<1 μm). The porosity is variable, being more porous in zones where <5% of metal is rusted, less porous in domains where metal is >20% rusted. Fe-Ni metal grains (10-15%) are variably irregular and approximately twice as abundant as troilite, with which they are occasionally conjoined. Most conjoined metal-troilite grains have sharp contacts, and there are rare domains of troilite in metal with adjacent Cu metal. Olivine grains show sharp extinction. Geochemistry: (A. Tomkins, Monash) Microprobe analyses show that olivine and pyroxene compositions are highly heteorgeneous: olivine Fa18.6-28.1, mean=20.7 mol%, std=4.1, n=5; Low-Ca pyroxene Fs9.3-17.9, mean=15.7 mol%, std=3.2, n=5; Wo0.6-4.0. Average compositions are most consistent with a H chondrite designation. Classification: Ordinary chondrite (H3, S2, W1). The type 3 classification is based on the heterogeneity of olivine and pyroxene compositions; the glass recrystallization implies upper type 3. | ||||||||||||||||||||||||||||||||||||||
Data from: MB102 Table 0 Line 0: |
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Institutions and collections |
Monash: Building 28
School of Geosciences
Monash University
Victoria 3800
Australia, Australia (institutional address; updated 12 Dec 2012) |
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Catalogs: |
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References: | Published in Meteoritical Bulletin, no. 102, MAPS 50, 1662, September 2015
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Geography: |
Statistics: This is 1 of 241 approved meteorites from South Australia, Australia (plus 3 unapproved names) (plus 4 impact craters) This is 1 of 719 approved meteorites from Australia (plus 11 unapproved names) (plus 27 impact craters) | ||||||||||||||||||||||||||||||||||||||
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Also see: |
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Revision history: |
This lists important revisions made to data for this record.
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