  Conventional meteoroid theory assumes that the dominant mode of ablation is
by evaporation following intense heating during atmospheric flight. In this
paper we consider the question of whether sputtering may provide an alternative
disintegration process of some importance.For meteoroids in the mass range from
10^-3 to 10^-13 kg and covering a meteor velocity range from 11 to 71 km/s, we
numerically modeled both thermal ablation and sputtering ablation during
atmospheric flight. We considered three meteoroid models believed to be
representative of asteroidal (3300 kg m^-3 mass density), cometary (1000 kg
m^-3) and porous cometary (300 kg m^-3) meteoroid structures. Atmospheric
profiles which considered the molecular compositions at different heights were
used in the sputtering calculations. We find that while in many cases
(particularly at low velocities and for relatively large meteoroid masses)
sputtering contributes only a small amount of mass loss during atmospheric
flight, in some cases sputtering is very important. For example, a 10^-10 kg
porous meteoroid at 40 km/s will lose nearly 51% of its mass by sputtering,
while a 10^-13 kg asteroidal meteoroid at 60 km/s will lose nearly 83% of its
mass by sputtering. We argue that sputtering may explain the light production
observed at very great heights in some Leonid meteors. The impact of this work
will be most dramatic for very small meteoroids such as those observed with
large aperture radars.
