File:Porous chondriteIDP.jpg

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Porous_chondriteIDP.jpg ‎(700 × 466 pixels, file size: 140 KB, MIME type: image/jpeg)

Summary

Description
English: This is a scanning electron microscope 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 Donald E. Brownlee, University of Washington, Seattle, and Elmar Jessberger, Institut für Planetologie, Münster, Germany.

This file is licensed under Creative Commons Attribution 2.5 License: https://creativecommons.org/licenses/by/2.5/ See the (Jessberger chapter 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.

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.
Date 22 September 2005 (original upload date)
Source Transferred from en.wikipedia to Commons by Common Good using CommonsHelper.
Author The original uploader was Amara at English Wikipedia.

Licensing

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Original upload log

The original description page was here. All following user names refer to en.wikipedia.
  • 2005-09-22 03:50 Amara 700×466× (143481 bytes) This is a scanning electron micrscope image of a interplanetary dust particle that has roughly [[chondrule|chondritic]] elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of
  • 2005-09-21 09:19 Amara 876×583× (203735 bytes) This is a scanning electron micrscope image of a interplanetary dust particle that has roughly [[chondrule|chondritic]] elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of
  • 2005-09-20 19:17 Amara 350×233× (50479 bytes) This is a scanning electron micrscope image of a interplanetary dust particle that has roughly [[chondrule|chondritic]] elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually aggregates of large numbers of sub-micrometer
  • 2005-09-20 18:58 Amara 876×583× (203078 bytes) [Porous_chondriteIDP.jpg]|porous chondrite]] This is a scanning electron micrscope image of a interplanetary dust particle that has roughly [[chondrule|chondritic]] elemental composition and is highly rough (chondritic porous: "CP"). CP types are usually

Captions

Chondrite interplanetary dust particle

Items portrayed in this file

depicts

cosmic dust

File history

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Date/TimeThumbnailDimensionsUserComment
current20:30, 18 March 2009Thumbnail for version as of 20:30, 18 March 2009700 × 466 (140 KB)File Upload Bot (Magnus Manske) {{BotMoveToCommons|en.wikipedia|year={{subst:CURRENTYEAR}}|month={{subst:CURRENTMONTHNAME}}|day={{subst:CURRENTDAY}}}} {{Information |Description={{en|This is a scanning electron microscope image of an interplanetary dust particle that has roughly [[:en:

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