Woolum, D. S. and Burnett, D. S. and Benjamin, T. M. and Rogers, P. S. Z. and Duffy, C. J. and Maggiore, C. J. (1986) A Test of Solar-System Abundance Smoothness. Meteoritics, 21 (4). pp. 543-544. ISSN 0026-1114. doi:10.1111/j.1945-5100.1986.tb00200.x. https://resolver.caltech.edu/CaltechAUTHORS:20150506-105708306
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Abstract
Carbonaceous chondrite (C1) elemental abundances are thought to represent the average solar system ("cosmic") composition (see e.g. Anders and Ebihara, 1982) based on the agreement between C1 and photospheric abundances and on the smoothness of heavy element abundances of odd mass nuclei when plotted as a function of mass number (A). The latter argument presently determines the accuracy of the identification.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1986 Meteoritical Society. | |||||||||
| Issue or Number: | 4 | |||||||||
| DOI: | 10.1111/j.1945-5100.1986.tb00200.x | |||||||||
| Record Number: | CaltechAUTHORS:20150506-105708306 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20150506-105708306 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 57273 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 06 May 2015 18:28 | |||||||||
| Last Modified: | 10 Nov 2021 21:10 |
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