Abstract
This paper discusses measured textures, porosity, chemical compositions and the minerals of interplanetary dust and meteorites from primitive planetesimals and how this information can be used to explain some of the observed physical and chemical properties of meteor phenomena.
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Acknowledgements
I thank Ed Murad for his constructive review. The material is based upon work supported by the National Aeronautics and Space Administration under Grants NAG5-11762 and NNG05GG10G issued through the Office of Space Science and by RTOPS from the Cosmochemistry and Origins of Solar Systems Research Programs.
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RIETMEIJER, F.J. INTERPLANETARY DUST AND CARBONACEOUS METEORITES: CONSTRAINTS ON POROSITY, MINERALOGY AND CHEMISTRY OF METEORS FROM RUBBLE-PILE PLANETESIMALS. Earth Moon Planet 95, 321–338 (2004). https://doi.org/10.1007/s11038-005-9037-7
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DOI: https://doi.org/10.1007/s11038-005-9037-7