Other
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28..461w&link_type=abstract
Meteoritics, vol. 28, no. 3, volume 28, page 461
Other
Antarctic Meteorites, H Chondrites, Meteorite Streams, Meteorites, Composition, Terrestrial Ages, Trace Elements, Volatile Elements
Scientific paper
Dodd et al. [1] found that, from their circumstances of fall, 17 H chondrites ("H Cluster 1") which fell in May, from 1855 to 1895, are distinguishable from other H chondrite falls and apparently derive from a co-orbital stream of meteoroids. From data for 10 moderately to highly labile trace elements (Rb, Ag, Se, Cs, Te, Zn, Cd, Bi, Tl, In), they used two multivariate statistical techniques--linear discriminant analysis and logistic regression--to demonstrate that 1. 13 H Cluster 1 chondrites are compositionally distinguishable from 45 other H chondrite falls, probably because of differences in thermal histories of the meteorites' parent materials; 2. The reality of the compositional differences between the populations of falls are beyond any reasonable statistical doubt. 3. The compositional differences are inconsistent with the notion that the results reflect analytical bias. We have used these techniques to assess analogous data for various H chondrite populations [2-4] with results that are listed in Table 1. These data indicate that 1. There is no statistical reason to believe that random populations from Victoria Land, Antarctica, differ compositionally from each other. 2. There is significant statistical reason to believe that the H chondrite population recovered from Victoria Land, Antarctica, differs compositionally from that from Queen Maud Land, Antarctica, and from falls. 3. There is no reason to believe that the H chondrite population recovered from Queen Maud Land, Antarctica, differs compositionally from falls. 4. These observations can be made either by data obtained by one analyst or several. These results, coupled with earlier ones [5], demonstrate that trivial explanations cannot explain compositional differences involving labile trace elements in pairs of H chondrite populations. These differences must then reflect differences of preterrestrial thermal histories of the meteorites' parent materials. Acceptance of these differences as preterrestrial has led to predictions subsequently verified by others (meteoroid and asteroid stream discoveries, differencesin thermoluminescence or TL). We predict that a TL difference will be seen between the populations of falls defined by Dodd et al. [1]. References: [1] Dodd R. T. et al. (1993) JGR, submitted. [2] Lingner D. W. et al. (1987) GCA, 51, 727-739. [3] Dennison J. E. and Lipschutz M. E. (1987) GCA, 51, 741-754. [4] Wolf S. F. and Lipschutz M. E. (1993) in Advances in Analytical Geochemistry (M. Hyman and M. Rowe, eds.), in press. [5] Wang M.-S. et al. (1992) Meteoritics, 27, 303. [6] Lipschutz M. E. and Samuels S. M. (1991) GCA, 55, 19-47. Table 1, which appears in the hard copy, shows a multivariate statistical analysis of H chondrite population pairs using 10 labile trace elements (number of meteorites in population in parentheses).
Lipschutz Michael E.
Wolf Steven F.
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