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Thermal metamorphic history of a Ca,Al‐rich inclusion constrained by high spatial resolution Mg isotopic measurements with NanoSIMS 50L
Authors:Motoo ITO  Scott MESSENGER
Affiliation:1. Robert M. Walker Laboratory for Space Science, NASA Johnson Space Center, ARES, Mail Code KR, 2101 NASA Parkway, Houston, Texas 77058, USA;2. Lunar and Planetary Institute, USRA‐Houston, 3600 Bay Area Blvd. Houston, Texas 77058, USA
Abstract:Abstract– Mg isotope data were collected by NanoSIMS with high‐precision and high‐spatial resolution from a coarse‐grained type B Ca‐, Al‐rich inclusion (CAI), EK1‐6‐3, in the Allende CV3 chondrite to evaluate the time scale of parent body thermal metamorphism. The CAI melilite and fassaite contain excesses of 26Mg (26Mg*) from the in‐situ decay of 26Al; the inferred initial ratio, (26Al/27Al)0 = (5.8 ± 2.4) × 10?5, is consistent with many previously reported coarse‐grained CAIs from CV chondrites (e.g., MacPherson et al. 1995 ). However, the anorthite has heterogeneous (26Al/27Al)0, ranging from 1.8 × 10?5 to 3.3 × 10?6. The 26Al‐26Mg systematics within the anorthite is consistent with thermal diffusion of Mg isotopes during metamorphism. We also show that the heterogeneous distribution of 26Mg* in anorthite could have resulted from thermal diffusion of 26Mg* over a 0.6–0.8 Ma time span. Mg diffusion thus may be responsible for the (26Al/27Al)0 heterogeneity within anorthite in CAIs.
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