the elements determined, in spite of substantial variations between bulk Allende and that meteorite's spheroidal Ca-Al-rich inclusions (Chou et al., 1976). ACKNOWLEDGMENTS.-We are indebted to R. Bild, R. Glimp, J. Kimberlin, K. Robinson, and L. Sundberg for assistance. Neutron irradiations at the UCLA and Ames Laboratories reactors were handled by J. Brower and A.F. Voight and their associates. This work was supported by NSF Grant GA 32084. 1450±40 c , 1400 e , 1300 f , l700 g 3370±100 c , 3300±100 d , 3300', 3000 f 200 e , 250 f , 1800±1200 g 130±22 c , 70 e , l70 f 3680±100 c , 3900±100 d , 3600 e , 4200 f , 4200 g 640±20 c , 650±40 d , 600 e , 700 f , 600 g 11.0±0.5 c , 12.2±0.2 d , ll e , 10 g 0.027±0.001 c 0.19±0.01 c 3.0±0.1 c , 2 e 0.44±0.02 c , 0.7 e 1.25±0.06 c , l e 0.20±0.01 c , 0.2 e 0.91±0.05 c , 0.9 e 0.29±0.01 c , 0.5 e 0.107±0.005 c ,0.1 e 0.43±0.02 c , 0.6 e 0.074±0.005 c , 0.09 e 0.42±0.02 c , 0.6 e 0.12±0.1 c ,0.1 e 0.31±0.02 c , 0.3 e 0.049±0.001 c 0.32±0.02 c , 0.4 e 0.058±0.002 c * The In value determined for 10-2 is 0.02±0.01; the large error limit is imposed due to an analyzer malfunction during counting. b The Cd value for 12-2 could not be determined because of a laboratory accident during the chemical processing.