Fiila:Porous chondriteIDP.jpg

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Porous_chondriteIDP.jpg(700 × 466 piksela (govvačuoggá), fiilasturrodat: 140 KiB, MIME-tiipa: image/jpeg)

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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.
Beaivemearri 22. čakčamánnuta 2005 (alkuperäinen tallennuspäivä)
Gáldu Transferred from en.wikipedia to Commons by Common Good using CommonsHelper.
Vuoigŋadahkki Alkuperäinen tallentaja oli Amara projektissa Wikipedia kielellä eaŋgalsgiella

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  • 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

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Chondrite interplanetary dust particle

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dálánjukčamánnu 18 b. 2009 dii. 20.30Govaš njukčamánnu 18 b. 2009 dii. 20.30 vurkejuvvon veršuvnnas700 × 466 (140 KiB)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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