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Tugna:Porous chondriteIDP.jpg

Porous_chondriteIDP.jpg ‎(700 × 466 pixel, tiddi n ufaylu: 140 KB/KO, anaw n MIME: image/jpeg)

Afaylu agi yusad seg : Wikimedia Commons. Ahat yeseqdec deg isenfaṛen nniḍen. Aglam-is ɣef asebter n aglam ye beqqeḍ ddaw-agi.

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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.
Azemz 22 Ctember 2005 (date de téléversement originale)
Aɣbalu Transféré de en.wikipedia à Commons par Common Good utilisant CommonsHelper.
Ameskar Original téléversé par Amara sur Wikipédia Taglizit.

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Journal des téléversements d’origine

La page de description originale était ici. Tous les noms d'utilisateur qui suivent se rapportent à 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

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Chondrite interplanetary dust particle

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Lux a18 Meɣres 2009 à 20:30Tugna tamectuḥt i lqem n 18 Meɣres 2009 à 20:30700 × 466 (140 KB/KO)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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