smooth Chondriteidp.jpg

Smooth_chondriteIDP.jpg ‎(757 × 502 pixels, file size: 177 KB, MIME type: image/jpeg)

Summary

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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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Date
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
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This file is licensed under Creative Commons Attribution 2.5 License: https://creativecommons.org/licenses/by/2.5/


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current09:21, 21 September 2005Thumbnail for version as of 09:21, 21 September 2005757 × 502 (177 KB) (talk | )== 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 2005Thumbnail for version as of 19:50, 20 September 2005333 × 221 (41 KB) (talk | )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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Smooth chondriteIDP.jpg

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