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I-Xe studies of individual chondrules: What can they tell us about chondrule formation?
- Source :
- Lunar and Planetary Inst., Papers Presented to the Conference on Chondrules and the Protoplanetary Disk.
- Publication Year :
- 1994
- Publisher :
- United States: NASA Center for Aerospace Information (CASI), 1994.
-
Abstract
- In the past 14 years, I-Xe studies have been performed on nearly 100 individual chondrules from five different meteorites. More than half the studied chondrules come from the unequilibrated ordinary chondrites (UOC's) Chainpur, Semarkona, and Tieschitz. However, 'unequilibrated' does not necessarily mean 'unaltered,' and the I-Xe studies of chondrules from UOC's have ultimately been interpreted in terms of postformation alteration. Two types of constraints on chondrule formation are discussed: (1) the duration, location, and timing of postformation alteration (in solids over a 50-m.y. span); and (2) the ages of the earliest formed chondrules (a few million years after the earliest solids).
- Subjects :
- Astrophysics
Subjects
Details
- Language :
- English
- Database :
- NASA Technical Reports
- Journal :
- Lunar and Planetary Inst., Papers Presented to the Conference on Chondrules and the Protoplanetary Disk
- Publication Type :
- Report
- Accession number :
- edsnas.19950012914
- Document Type :
- Report