Laboratory hypervelocity impact experiments were conducted to verify the pe
rformance of aerogel dust collectors used for gathering meteoroids and spac
e debris in the near-Earth environment and to derive the relationships of v
arious parameters characterizing the projectile with morphology of tracks l
eft by the penetrating projectile in the aerogel collector pad. Silica aero
gel collectors of 0.03 g/cm(3) density were impacted at velocities ranging
from 1 to 14 km/s with projectiles of aluminum oxide, olivine, or soda-lime
glass, with diameters ranging from 10 to 400 mu m. At impact velocities be
low 6 km/s the projectiles were captured without fragmentation by the aerog
el collector and, in many instances, without complete ablation even at 12 k
m/s. The shapes and dimensions of the penetration tracks left in the aeroge
l collector were correlated with the impact parameters, and the results per
mitted derivation of a series of equations relating the track dimensions to
incoming projectile size, impact energy, and other projectile parameters.
A simplified model, similar to meteor-entry phenomena, was used to predict
the trends in experimental penetration track lengths and the diameters of c
aptured projectiles.