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- Publisher
- Wiley
- Copyright
- "Copyright © 1974 Wiley Subscription Services, Inc., A Wiley Company"
- ISSN
- 1086-9379
- eISSN
- 1945-5100
- DOI
- 10.1111/j.1945-5100.1974.tb00063.x
- Publisher site
- See Article on Publisher Site
Abstract
Observed differences in the abundance ratios of moderately volatile elements found in ordinary chondrites relative to CI chondrites may have resulted from a continuous loss of nebular gas from the ordinary‐chondrite formation region during condensation. If this occurred, the nebular volatility of these elements should be inversely correlated with their abundance ratios. Such a nebular gas loss can occur as a result of momentum exchange between solids and gases, as a result of interactions between the nebular gas and solar photons or particles at the surface of the nebula, or as a result of the settling of previously condensed solids to the median plane of the nebula.
Journal
Meteoritics & Planetary Science – Wiley
Published: Mar 1, 1974