Capture of hypervelocity particles in aerogel: in ground laboratory and low earth orbit

Citation
Mj. Burchell et al., Capture of hypervelocity particles in aerogel: in ground laboratory and low earth orbit, PLANET SPAC, 47(1-2), 1999, pp. 189-204
Citations number
26
Categorie Soggetti
Space Sciences
Journal title
PLANETARY AND SPACE SCIENCE
ISSN journal
00320633 → ACNP
Volume
47
Issue
1-2
Year of publication
1999
Pages
189 - 204
Database
ISI
SICI code
0032-0633(199901/02)47:1-2<189:COHPIA>2.0.ZU;2-S
Abstract
We have investigated in the laboratory the capture in aerogel (density 92.5 +/- 0.5 kg m(-3)) of small particles travelling at (5.1 +/- 0.2) km s(-1). The particles used were soda glass spheres and irregularly shaped olivine and iron particles, with mean diameters in the range 75-355 microns. We hav e measured the impact site for each particle, characterised by the mean dia meter of the entrance hole in the aerogel, the minimum and maximum radii of the damaged region in the surface of the aerogel around the entrance hole, the length of the track in the aerogel caused by passage of the particle i nto the aerogel's interior, and the diameter of the captured particle (if s een) found near the end of the track. For each type of particle we establis h relationships between the observed parameters and the pre-impact particle size. We find that the processes resulting in the observed surface feature s and the capture of the particles in the interior of the aerogel are diffe rent. We also find that the particle shape (spherical/irregular) does not u nduly influence penetration depths in the aerogel. We have studied the effe cts of non-normal incidence on the observed impact features and find that t he angle of incidence can be reconstructed to within +/-2 degrees. We compare the laboratory obtained data with that measured for four particl es captured in a sample of aerogel flown in a Low Earth Orbit on board the EuReCa spacecraft. The density of one of the particles is predicted to be ( 1776 +/- 346) km m(-3). Using the ability to reconstruct impact direction t he probable nature of the particles is shown to be micrometeoroids with ret rograde trajectory. (C) 1999 Elsevier Science Ltd. All rights reserved.