Ungrouped Chondrite Meteorite Slice 1.64g I NWA 12273 I Very Rare - TOP
Ungrouped Chondrite Meteorite Slice 1.64g I NWA 12273 I Very Rare - TOP
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Description:
Official name: NWA 12273
Description: A beautiful 1.64 gram partial slice of the ungrouped chondrite NWA 12273. Polished on one side, and rough wire cut finish on reverse. This meteorite defies any known classification, hence the "ungrouped, or "-ung" designation. All that the researchers can say about how this meteorite fits into the current meteoritic taxonomy, is that it is a chondrite. Which is much like asking an ornithologist what type of bird you had discovered and having them come back after extensive analysis and saying its official taxonomy was, "Bird Ungrouped". With visual characteristics similar to a Bencubbinite but with Oxygen isotopic overlap with the LL chondrites, this is a very strange and scientifically significant meteorite. This meteorite is a bit of a cosmic irony seeing as it is extremely metal rich and the LL chondrites are so named for being relatively metal poor. This meteorite pairs with the Chondrite-ung NWA 12379.
What you get: 1.64 gram Ungrouped Chondrite Meteorite Specimen as Shown, Membrane Storage/Display Box, signed 5x7 double sided color Certificate of Authenticity
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OFFICIAL METEORITICAL SOCIETY ENTRY BELOW
Northwest Africa 12273Basic informationName: Northwest Africa 12273
This is an OFFICIAL meteorite name.
Abbreviation: NWA 12273
Observed fall: No
Year found: 2018
Country: (Northwest Africa)
Mass: 280 gClassification
history:Recommended: Chondrite-ung [explanation]
This is 1 of 24 approved meteorites classified as Chondrite-ung. [show all]
Search for other: Ungrouped chondritesComments:Approved 11 Dec 2018Writeup
Writeup from MB 107:
Northwest Africa 12273 (NWA 12273)
(Northwest Africa)
Purchased: 2018
Classification: Ungrouped chondrite
History: Purchased by Jay Piatek from a Moroccan meteorite dealer on October 25, 2018.
Physical characteristics: Dense, single individual. Fusion crust absent; abundant bright metal; scattered small chondrules are visible.
Petrography: (C. Agee, UNM) This meteorite consists of approximately 75% metal in the form of kamacite (~90%) and taenite (~10%) grains, diameters ranging from 50-500 m. Minor troilite was observed throughout. Silicates occur primarily in the form of chondrules, most are porphyritic, diameters in the range 100-500 m, making up approximately 20% of this meteorite.
Geochemistry: (C. Agee) Olivine Fa 26.2 3.3, Fe/Mn=55 5, n=29; low-Ca pyroxene Fs 15.3 1.8Wo 0.7. 0.2, Fe/Mn=23 2, n=11. Oxygen isotopes (K. Ziegler, UNM): 3 acid-washed fragments analyzed by laser fluorination gave 18O= 5.258, 5.613, 7.249; 17O= 3.939, 3.971, 4.786; 17O= 1.163, 1.007, 0.959 (linearized, all per mil, TFL slope=0.528).
Classification: Ungrouped chondrite. This is a metal-rich chondrite with oxygen isotopes that overlap with LL-chondrites. The olivine Fa content is consistent with L3, however the low-Ca pyroxene Fs is consistent with H4. The high metal content is inconsistent with ordinary chondrite. Texturally, this meteorite resembles a CB-b, however the oxygen isotopes and Fa and Fs are unlike CB chondrites.
Specimens: 23.2 g including a probe mount on deposit at UNM, Jay Piatek holds the main mass of 240 g.
Data from:
MB107
Table 0
Line 0:
Place of purchase:MoroccoDate:P 2018Mass (g):280Pieces:1Class:Chondrite-ungShock stage:lowWeathering grade:lowFayalite (mol%):26.2 3.3Ferrosilite (mol%):15.3 1.8Wollastonite (mol%):0.7 0.2Classifier:C. Agee, UNMType spec mass (g):23.2Type spec location:UNM
ID: NWA122731906
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