The stream meteoroid impact probability for space platforms is reviewed and
found to be very low under normal circumstances. While the literature cont
ains numerous accounts of spacecraft apparently suffering damage and/or int
erference during meteoroid stream encounters, we find that there is, in fac
t, very little evidence to support such claims. This conclusion may not be
valid, however, during meteor storms, when the flux of visual meteors can i
ncrease by factors in excess of 10(3) to 10(4) of that from the sporadic ba
ckground. Special attention is directed towards the Leonid meteor storms of
1965 and 1966-the only meteor storms since the dawn of the space age. The
space platform impact probabilities during the 1966 storm were small but no
ne negligible, being of order 1% for an exposed surface area of 2 m(2) at a
limiting meteoroid mass of 10(-7) (and assuming a stream mass index s = 2.
0). The circumstances surrounding the possible encounters of the Pegasus II
and III, and Mariner 4 spacecraft with Leonid stream meteoroids are discus
sed in some detail. While the 1966 Leonid meteor storm is the strongest on
record (in the sense of the highest visual meteor rates) no apparent meteor
oid inflicted damage to a spacecraft can be unambiguously linked to it. Thi
s result is mostly a consequence of the small number and small size of spac
ecraft in Earth-orbit at the time of the 1966 storm. (C) 1999 Elsevier Scie
nce Ltd. All rights reserved.