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Lunar Meteorite: Northwest Africa (NWA) 3163, 4483, and 4881 (paired stones)

Mauritania or Algeria


  



NWA 3163
(photos courtesy of Greg Hupé)



Sawn slice of NWA 3163
(photo by Randy Korotev)

 

Slices of NWA 4881, with exterior (left)
(photo by Randy Korotev)



A different slice on NWA 4881
(photo by Randy Korotev)

  

Slice of NWA 4483.
(photo by Randy Korotev)


from The Meteoritical Bulletin, no. 90, Meteoritics & Planetary Science 41, 1383-1418 (2006)

Northwest Africa 3163

Mauritania or Algeria
Find: August 2005

Achondrite (lunar, feldspathic granulitic impactite)

History: In August 2005, G. Hupé purchased a 1634 g stone from a Moroccan dealer in Ouarzazate.

Petrography and Geochemistry: (A. Irving and S. Kuehner, UWS) The exterior is almost completely coated by a thin, transparent, greenish fusion crust. The pale gray interior has multiple shock fractures (with very minor calcite coatings) and some thin glass veins. Poikiloblastic recrystallized breccia, with larger grains of plagioclase (~70 vol%) enclosing much smaller grains (less than 100 µm across) of pyroxenes (~20 vol%), olivine (~10 vol%), and accessory Ti-chromite (Cr/(Cr+Al) = 0.714–0.736; Mg/(Mg+Fe) = 0.121– 0.143; TiO2 = 9.1–18.4 wt%), ilmenite, troilite, and metal (Ni = ~15 wt%). Anorthitic plagioclase (An97.4-98.2) has been converted by shock almost entirely to maskelynite (although domains of birefringent, less-shocked feldspar remain). Pigeonitic pyroxene grains have very fine-scale exsolution lamellae of augite (Fs14.5-16.1 Wo40.2-40.5; FeO/MnO = 41.7– 43.8) within orthopyroxene Fs32.0-33.9 Wo4.4-5.8; FeO/MnO = 55.5–61.2). Olivine (Fa38.0-40.9; FeO/MnO = 91.7–110).

Classification: Achondrite (lunar, feldspathic granulitic impactite).

Specimens:
A 20.1 g type specimen and one polished thin section are on deposit at UWS. G. Hupé holds the main mass.
from The Meteoritical Bulletin, no. 93, Meteoritics & Planetary Science 43, 571-632 (2007)

Northwest Africa 4881

Mauritania or Algeria
Find: 2005

Achondrite (lunar, granulitic breccia)

History: Found in 2005 and purchased by Stefan Ralew in January 2007 from a dealer in Ouarzazate, Morocco.

Physical characteristics: A single, broken, irregular conical stone (606 g) partially covered by translucent, pale greenish fusion crust and with a pale grey-brown interior.

Petrography: (A. Irving and S. Kuehner, UWS) Fine grained recrystallized breccia composed of larger plagioclase grains (converted partially to maskelynite) poikilitically enclosing very small grains (mostly 30-80 microns) of low-Ca pyroxenes, olivine, Ti-chromite, ilmenite, troilite and metal.

Mineral compositions and geochemistry: Olivine (Fa40.4-58.8, FeO/MnO = 91-100), plagioclase (An96.1-98Or<0.1), pigeonite (Fs32.0-64.5Wo9.5-13.1, FeO/MnO = 51.1-62).

Classification: Achondrite (lunar, granulitic breccia). This stone is paired with Northwest Africa 3163 (Irving et al., 2006) and Northwest Africa 4483; in combination these specimens evidently represent naturally broken pieces from a crusted lunar meteorite weighing at least 2448 g.

Specimens: A total of 20 g of sample and one polished mount are on deposit at UWS. Ralew holds the main mass.
from The Meteoritical Bulletin, No. 94, September 2008. Meteoritics & Planetary Science 43, 1551–1588 (2008)

Northwest Africa 4483

Algeria
Find: July 2006

Achondrite (lunar, granulitic breccia)

History: Purchased by Stefan Ralew in July 2006 from a dealer in Erfoud, Morocco.

Physical characteristics: Twelve broken fragments of very fine-grained, pale grey rock with a combined weight of 208 g.

Petrography (A. Irving and S. Kuehner, UWS): Fine grained recrystallized breccia composed of larger plagioclase grains (converted mainly to maskelynite) poikilitically enclosing very small grains (mostly 30-80 microns) of low-Ca pyroxene (some with very fine augite exsolution lamellae), olivine, Ti-chromite, ilmenite, troilite and metal.

Geochemistry: Olivine (Fa30.9-60.8, FeO/MnO = 88.1- 106), plagioclase (An96.2-98Or<0.1), orthopyroxene(Fs14.3Wo2.0, FeO/MnO = 52.6), pigeonite (Fs36.4- 75.1Wo6.3-13.5, FeO/MnO = 62.9-66.5).

Classification: Achondrite (lunar, granulitic breccia). Possibly paired with Northwest Africa 3163 (Irving et al., 2006).

Specimens: A total of 20 g and one polished mount are on deposit at UWS. Ralew holds the main mass.


More Information

Meteoritical Bulletin Database

NWA 3163 | NWA 4483 | NWA 4881

References

Fernandes V. A., Irving A. J., Kuehner S. M., Gellissen M., Korotev R. L., and Bandfield J. L. (2009) Petrology, bulk composition, Ar-Ar age and IR emission spectrum of lunar granulite Northwest Africa 4881 (abstract). In Lunar and Planetary Science XL, abstract no. 2009, 40th Lunar and Planetary Science Conference, Houston.

Hudgins J. A. and Spray J. G. (2009) Lunar granulitic breccias: Differences between Apollo and meteorite samples (abstract). 72th Annual Meeting of the Meteoritical Society, number 5157.

Irving A. J., Kuehner S. M., Korotev R. L., Rumble D. III, and Hupé G. M. (2006) Mafic granulitic impactite NWA 3163: A unique meteorite from the deep lunar crust (abstract). In Lunar and Planetary Science XXXVII, abstract no. 1365, Lunar and Planetary Institute, Houston.

Korotev R. L. (2006) New geochemical data for a some poorly characterized lunar meteorites (abstract). In Lunar and Planetary Science XXXVII, number 1404, Lunar and Planetary Institute, Houston.

Korotev R. L., Irving A. J., and Bunch T. E. (2008) Keeping up with the lunar meteorites – 2008 (abstract). In Lunar and Planetary Science XXXIX, abstract no. 1209, 39th Lunar and Planetary Science Conference, Houston.

Korotev R. L., Zeigler R. A., Irving A. J., and Bunch T. E. (2009) Keeping up with the Lunar Meteorites — 2009 (abstract). In Lunar and Planetary Science XL, abstract no. 1137, 40th Lunar and Planetary Science Conference, Houston.

Nishiizumi K. and Caffee M. W. (2006) Constraining the number of lunar and martian meteorite falls (abstract). In Meteorit. Planet. Sci. 41, p. A133, 69th Annual Meeting, Meteoritical Society.

Chemical Classification

Overview | NWA 3163



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Prepared by:

Randy L. Korotev


Department of Earth and Planetary Sciences
Washington University in St. Louis


Please don't contact me about the meteorite you think you’ve found until you read this and this.

e-mailkorotev@wustl.edu

Last revised: 01-Jun-2009