Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 20 March 1992:
Vol. 255. no. 5051, pp. 1551 - 1553
DOI: 10.1126/science.255.5051.1551

Articles

Evidence for Ammonium-Bearing Minerals on Ceres

TRUDE V. V. KING 1, R. N. CLARK 1, W. M. CALVIN 1, D. M. SHERMAN 1, and R. H. BROWN 2

1 U.S. Geological Survey, Denver, CO 80225
2 Jet Propulsion Laboratory, Pasadena, CA 91109

Spectra obtained from recent telescopic observation of 1-Ceres and laboratory measurements and theoretical calculations of three component mixtures of Ceres analog material suggest that an ammoniated phyllosilicate is present on the surface of the asteroid, rather than H2O frost as had been previously reported. The presence of an ammoniated phyllosilicate, most likely ammoniated saponite, on the surface of Ceres implies that secondary temperatures could not have exceeded 400 kelvin.

Submitted on November 13, 1991
Accepted on February 3, 1992


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Oxygen and Asteroids.
T. H. Burbine, A. S. Rivkin, S. K. Noble, T. Mothe-Diniz, W. F. Bottke, T. J. McCoy, M. D. Dyar, and C. A. Thomas (2008)
Reviews in Mineralogy and Geochemistry 68, 273-343
   Abstract »    Full Text »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)