The equations of motion have been solved numerically for the incompres
sible power law fluid flow past spherical and spheroidal solid particl
es. The finite element technique has been employed to obtain the veloc
ity and pressure fields prevailing around a particle. These have been
further processed to evaluate the individual contributions of pressure
and viscous forces to the total drag on spheres and spheroids (prolat
es and oblates). Streamline plots showing the nature of flow and the g
radual development of the wake region are also presented. The computed
drag results encompass wide ranges of physical and kinematic conditio
ns given by 1 greater-than-or-equal-to n greater-than-or-equal-to 0.4,
0.01 less-than-or-equal-to Re less-than-or-equal-to 100, and 0.2 less
-than-or-equal-to E less-than-or-equal-to 5. Extensive comparisons are
provided with previous theoretical and experimental results available
in the literature.