File:Smooth chondriteIDP.jpg

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Description	This is a scanning electron microscope image of an interplanetary dust particle that has roughly chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micrometer grains, clustered in a random open order. References E. K. Jessberger, T. Stephan, D. Rost, P. Arndt, M. Maetz, F. J. Stadermann, D. E. Brownlee, J. P. Bradley, G. Kurat (2001). Properties of Interplanetary Dust: Information from Collected Samples, in Grün, E., Gustafson, B.A.S., Dermott, S.F., Fechtig, H. (Eds.) Interplanetary Dust, pp. 253–294, Springer-Verlag.
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Author	The authors of this figure are Don Brownlee, University of Washington, Seattle, and Elmar Jessberger, Institut für Planetologie, Münster, Germany. See the "Jessberger" chapter in the Grün at Interplanetary Dust (2001) book for more details.
Permission (Reusing this file)	This file is licensed under Creative Commons Attribution 2.5 License: https://creativecommons.org/licenses/by/2.5/

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	09:21, 21 September 2005		757 × 502 (177 KB)	Amara (talk \| contribs)	== Summary == This is a scanning electron micrscope image of an interplanetary dust particle that has roughly chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers o
	19:50, 20 September 2005		333 × 221 (41 KB)	Amara (talk \| contribs)	This is a scanning electron micrscope image of an interplanetary dust particle that has roughly chondritic elemental composition and is highly smooth (chondritic smooth: "CS"). CS types are usually aggregates of large numbers of sub-micromet

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