Image:Porous chondriteIDP.jpg
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[edit] Summary
This is a scanning electron micrscope image of an interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of sub-micrometer grains, clustered in a random open order. The authors of this figure are Don Brownlee, University of Washington, Seattle, and Elmar Jessberger, Institut für Planetologie, Münster, Germany. This file is licensed under Creative Commons Attribution 2.5 License: http://creativecommons.org/licenses/by/2.5/
See the (Jessberger chapter in in Grün, E., Gustafson, B.A.S., Dermott, S.F., Fechtig, H. (Eds.) Interplanetary Dust book for more details on this kind of dust particle.
[edit] 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.
[edit] Licensing
| This work is licensed under the Creative Commons Attribution 2.5 License. |
File history
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| Date/Time | Dimensions | User | Comment | |
|---|---|---|---|---|
| current | 03:50, 22 September 2005 | 700×466 (140 KB) | Amara (Talk | contribs) | (== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of) |
| 09:19, 21 September 2005 | 876×583 (199 KB) | Amara (Talk | contribs) | (== Summary == This is a scanning electron micrscope image of a interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of) | |
| 19:17, 20 September 2005 | 350×233 (49 KB) | Amara (Talk | contribs) | (This is a scanning electron micrscope image of a interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of sub-micrometer) | |
| 18:58, 20 September 2005 | 876×583 (198 KB) | Amara (Talk | contribs) | ( [Porous_chondriteIDP.jpg]|porous chondrite]] This is a scanning electron micrscope image of a interplanetary dust particle that has roughly chondritic elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually) |
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