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Densities of 5-15 micron interplanetary dust particlesWe have measured the densities of about 100 5-15 micron stratospheric IDPs. Great care was taken to minimize selection bias in the sample population. Masses were determined using an absolute x-ray analysis technique with a transmission electron microscope, and volumes were found using scanning electron microscope imagery. Unmelted chondritic particles have densities between 0.5 and 6.0 g/cc. Roughly half of the particles have densities below 2 g/cc, indicating appreciable porosity, but porosities greater than about 70 percent are rare. IDPs with densities above 3.5 g/cc usually contain large sulfide grains. We find no evidence of bimodality in the unmelted particle density distribution. Chondritic spherules (melted particles) have densities near 3.5 g/cc, consistent with previous results for deep sea spherules.
Document ID
19940011894
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Love, S. G.
(Washington Univ. Seattle, WA, United States)
Joswiak, D. J.
(Washington Univ. Seattle, WA, United States)
Brownlee, D. E.
(Washington Univ. Seattle, WA, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M
Subject Category
Astrophysics
Accession Number
94N16367
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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