Other
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28..350f&link_type=abstract
Meteoritics, vol. 28, no. 3, volume 28, page 350
Other
Aiou El Atrouss, Ellemeet, Garland, Ibbenburen, Johnstown, Manegoan, Peckelsheim, Roda, Shalka, Tatahouine
Scientific paper
This research represents a continuing effort to understand the petrogenesis of diogenites and their relationship to eucrites. Our present suite of 17 diogenites includes: Aioun El Atrouss, Ellemeet, Garland, Ibbenburen, Johnstown, Manegoan, Peckelsheim, Roda, Shalka, Tatahouine, EET 83246, EET 83247, EET 87530, EET A79002, LEW 88008, and olivine diogenites ALH 84001 and ALH A77256. In our previous studies [1,2], we reported major, minor, and trace element systematics for a subgroup of 13 of these samples. In these studies, we concluded that Fe/Mg was compromised by post-crystallization annealing reactions. We also demonstrated [1] strong, positive correlations between Cr and Al along several trajectories on a Cr-Al data display. REE and Zr-Ti systematics indicate that most sampled diogenites represent cumulates from similar basaltic melts. These modeled melt compositions are similar to eucrites but show a greater compositional range. Here we further explore the Al-Cr-Ti systematics. Figure 1 (figures include over 1,000 high quality EMP analyses) is a Ti-Al plot that shows a main trend with a positive correlation between Ti and Al. Rhoda and one of the assemblages in polymict Garland have elevated Ti concentrations relative to the main trend while Manegoan has relatively depleted Ti concentrations. Figure 2 is a (Cr+Ti) vs. Al plot with a main trend that shows a strong, positive correlation between (Cr+Ti) and Al. Manegoan occupies the high (Cr+Ti)-Al end of the trend while Peckelsheim occupies the low end. Olivine diogenite ALH A77256 falls distinctly off the trend. However, ALH 84001, our only other olivine diogenite, plots with the other diogenite in the main trend. Several things are indicated by these systematics. The positive correlation of (Cr+Ti) vs. Al indicate that the most important charge balance couples are ^VITi^4+-^IVAl(sub)2, ^VITi^3+-^IVAl, ^VICr^3+-^IVAl, and ^VIAl-^IVAl. The ^VIAl-^IVAl couple is relatively more important in olivine diogenite ALH A77256, which accounts for its data plotting below the main trend. It should be noted that the main trend and the ALH A77256 trend have less scatter near the bottom of the data arrays than near the top. In fact, lines drawn through the bottom of the arrays project through the origin. Some of the reason for the scatter, other than subsolidus annealing effects [3], may be the result of different Ti^3+/Ti^4+ ratios in OPX resulting from variable fO2 environments. A possible charge balance equation, for other then quadrilateral components is: ^VITi^3++2^VITi^4++^VICr^3++^VIAl^3+=^IVAl (Na is so low it can be ignored). The cores of most OPX grains probably still retain their igneous signatures; therefore, the high Al, Cr, Ti end of the main trend likely reflects melt compositions enriched in these elements. Acknowledgment. This research was supported by NASA Grant NAGW- 3347 and the Institute of Meteoritics. References. [1] Papike J. J. et. al. (1993) LPS XXIV, 1109-1110. [2] Shearer C. K. et al. (1993) LPS XXIV, 1289-1290. [3] Papike J. J. and Spilde M. N. (1993) This volume. Fig. 1, which appears here in the hard copy, shows Al vs. Ti atoms per formula unit. Fig. 2, which appears here in the hard copy, shows Ti + Cr vs. Al in atoms per formula unit.
Fowler G. W.
Papike James J.
Shearer Charles K.
Spilde Michael N.
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