LEW85332: A C2 Chondrite in the CR Clan

Details LEW85332: A C2 Chondrite in the CR Clan LEW85332: A C2 Chondrite in the CR Clan

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992metic..27r.278p&link_type=abstract

Meteoritics, vol. 27, no. 3, volume 27, page 278

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Scientific paper

Introduction. LEW85332 was described as a unique C3 chondrite [1] and we undertook this study to learn more about its relationship to other carbonaceous chondrites. We find it to be a C2 chondrite with significant similarites to CR2 chondrites. This linkage extends to the ALH85085 [2] and Acfer 182 [3,4] chondrites, although there are some important differences among them. Petrologic and isotopic similarities define the CR clan, which consists of CR chondrites and their three relatives noted above (and Bencubbin). Some differences are due to major component abundances (chondrules, matrix, metal), and some to minor differences between components, but the similarities are greater and define the clan. Results. Petrogically, LEW85332 has over 60% (vol) chondrules, about 30% matrix and matrix clasts, and about 4-7% metal. Extensive weathering makes modal abundances uncertain. Chondrules are anhydrous, about 170 micrometers wide [1] and of all textural types. ALH85085 chondrules average 20 micrometers and are mainly pyroxene-rich, whereas Acfer 182 is more like LEW85332. Matrix is hydrous and occurs as interstitial matrix, matrix clasts, and chondrule rims [5]. The matrix contains phyllosilicates and magnetite framboids. Matrix clasts are not foreign [1], but part of the chondrite, making it C2. This is also the case for Acfer 182 [3], and perhaps ALH85085. Phyllosilicates are mainly saponite and serpentine [5], and their composition is similar to that in CR chondrites. The water/rock ratio was low. Metal abundances in LEW85332 [1] are lower than in Acfer 182 (9.3 vol%) [4] and ALH85085 (22%) [6]. However, FeNi composition is the same, with a positive Ni-Co trend equivalent to the solar abundance ratio. This is the same as that in CR chondrites [7]. LEW85332 contains 0.5% carbon, combusting between 200 and 500 degrees C, indicating fine-grained, poorly crystalline carbon, or organic material. It contains 259 ppm nitrogen with delta^15N = +249o/oo. Most nitrogen is released between 200 and 500 degrees C, but at 325 C the delta^15N reaches +306o/oo indicating at least two N-bearing components with differing C/N atomic ratios. The LEW85332 nitrogen isotopic composition is intermediate between ALH85085, Acfer 182 and CR chondrites, closer to CR. The extremely heavy, high- temperature component found in ALH85085 is absent (or nearly so) in LEW85332. Nitrogen abundance is similar to ALH85085, but lower than in CRs. The oxygen isotopic composition of LEW85332 is delta^18O = -0.92, delta^17O = -1.93. This, plus ALH85085 and Acfer 182 define a line (figure) identical to that of the CR chondrite mixing line (slope = 0.7) [7]. The composition of LEW85332 is close to that of unaltered olivine and pyroxene in Renazzo and Al Rais. Conclusions. (1) The important similarities between components in LEW85332 and CR2 chondrites put it in the CR clan. (2) Recognition of LEW85332, Acfer 182, and ALH85085 as relatives in the CR clan indicates that carbonaceous chondrites can no longer be classified only into coherent groups with highly similar characteristics. Recognition of clan relationships will be needed for IDPs and micrometeorites. (3) LEW85332, Acfer 182, and ALH85085 contain hydrous matrices and anhydrous chondrules, and the implications of this observation requires further study. References. [1] Rubin, A.E. and Kallemeyn, G.W. (1990) Meteoritics 25, 215-225. [2] Weisberg, M.K. et al. (1990) Meteoritics 25, 269-279. [3] Prinz, M. and Weisberg, M.K. (1992) LPSCXXIII, 1109-1110. [4] Bischoff, A. et al. (1992) Acfer 182 ms. GCA (in press). [5] Brearley, A.J. (1992) LPSCXXIII, 155-156. [6] Weisberg, M.K. et al. (1988) EPSL 91, 19-32. [7] Weisberg, M.K. et al. (1992) CR chondrite ms. GCA (in press).

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