Current debris models are able to predict the growth of the space debris pr
oblem and suggest that spacecraft must employ armor or bumper shields for s
ome orbital altitudes now and that the problem will become worse as a funct
ion of time. The practical upper limit to the velocity distribution is on t
he order of 40 km/s and is associated with the natural environment. The vel
ocity distribution of the man-made component peaks at 9-10 km/s with maximu
m velocity in the 14-16 km/s range. Experience in space has verified that t
he "high probability of impact" particles are in the microgram to milligram
range. These particles can have very significant effects on coatings, insu
lators, and thin metallic layers. The surface of thick materials becomes pi
tted and the local debris component is enhanced by ejecta from the impact e
vents. In this paper, the HYPER facility is described which produces a reas
onable simulation of the man-made space debris spectrum in a controlled env
ironment. The facility capability is discussed in terms of drive geometry,
energetics, velocity distribution, diagnostics, and projectile/debris loadi
ng. The facility has been used to study impact phenomena on Space Station F
reedom's solar array structure, the calibration of space debris collectors,
other solar array materials, potential structural materials for use in the
space, electrical breakdown in the space environment, and as a means of cl
arifying or duplicating the impact phenomena on surfaces which have been ex
posed in space. (C) 1999 Elsevier Science Ltd. All rights reserved.