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Greenwood, R.C. and Franchi, I.A.
(2005).
URL: http://www.lpi.usra.edu/meetings/am2005/pdf/7006.p...
Abstract
From the introduction: Small planetary bodies accreted within 2.4 Myr of solar system formation [1]. The primitive materials (CAIs, chondrules, matrix) incorporated into these asteroids were altered by a variety of secondary processes, including aqueous alteration, shock metamorphism, thermal metamorphism and melting. Here we look primarily at the role played by thermal metamorphism and melting in altering the oxygen isotope systematics of asteroidal materials.
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- Item ORO ID
- 8484
- Item Type
- Conference or Workshop Item
- Extra Information
- Abstract #7006
- Keywords
- asteroids;
- Academic Unit or School
-
Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM) - Depositing User
- Kyra Proctor