2004
DOI: 10.1111/j.1945-5100.2004.tb00952.x
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Aerogel keystones: Extraction of complete hypervelocity impact events from aerogel collectors

Abstract: Abstract-In January 2006, the Stardust mission will return the first samples from a solid solar system body beyond the Moon and the first samples of contemporary interstellar dust ever collected. Although sophisticated laboratory instruments exist for the analysis of Stardust samples, techniques for the recovery of particles and particle residues from aerogel collectors remain primitive. Here, we describe our recent progress in developing techniques for extracting small volumes of aerogel, which we have called… Show more

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Cited by 102 publications
(94 citation statements)
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“…Therefore, these may not be representative of the features preserved in the Stardust collectors where the encounter velocity was approximately 6 km/s. The LEO-derived impact events tend to show a high degree of particle fragmentation on the micron and sub-micron scales (e.g., Hörz et al 2000;Westphal et al 2004). Therefore, it is reasonable to assume that if cometary particles are similar to fluffy anhydrous IDPs, they may exhibit similar behavior upon collision with the silica aerogel collectors, even at the lower velocity.…”
Section: Particle Characterization Using a Nuclear Microprobementioning
confidence: 99%
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“…Therefore, these may not be representative of the features preserved in the Stardust collectors where the encounter velocity was approximately 6 km/s. The LEO-derived impact events tend to show a high degree of particle fragmentation on the micron and sub-micron scales (e.g., Hörz et al 2000;Westphal et al 2004). Therefore, it is reasonable to assume that if cometary particles are similar to fluffy anhydrous IDPs, they may exhibit similar behavior upon collision with the silica aerogel collectors, even at the lower velocity.…”
Section: Particle Characterization Using a Nuclear Microprobementioning
confidence: 99%
“…The development of the extraction technique described in Westphal et al (2002Westphal et al ( , 2004) is a significant milestone. However, it is only the first stage of the analytical strategy for Stardust particles.…”
Section: Particle Characterization Using a Nuclear Microprobementioning
confidence: 99%
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