A computational model of a stationary plasma thruster (SPT) has been develo
ped using a quasineutral particle-in-cell/direct simulation Monte Carlo (PI
C-DSMC) model. This model is based on theoretical work showing that the plu
me consists of a quasineutral plasma with collisionless electrons in which
the magnetic field can be neglected. Details of the PIC-DSMC method are pre
sented as well as axisymmetric and three-dimensional results. Comparisons a
re made to new and previously reported experimental data. The model is show
n to produce results similar to laboratory measurements of the ion current
density and plume-induced sputter erosion rates. The model does not compare
as well with retarding potential analyzer measurements of the ion energy d
istribution, The results confirm previous observations that measurements ma
de in some ground facilities may substantially overpredict the amount of ba
ckflow current that will be experienced under operational conditions, A sur
face-sputtering model is used to predict the impact the plume has on solar
array interconnects and to show the impact an SPT thruster could have on a
communications satellite. The results show that the thruster should be cant
ed with respect to the solar array, lowering its effective thrust and speci
fic impulse.