We considered the effect of the wind on the entry of meteorites into the ve
nusian atmosphere by solving the entry equations involving a term related w
ith the wind drag. We found that the wind affects only the entry of iron me
teorites with masses less than 10(9) kg and stone meteorites with masses le
ss than 10(11) kg. Since meteorites that produce craters on Venus have mass
es exceeding these limits we conclude that the effect of the wind is neglig
ible in the processes of craterization of the surface of Venus. (C) 1999 El
sevier Science Ltd. All rights reserved.