  We present a preliminary study of the star formation distribution within
three Virgo Cluster galaxies using the 24 micron Spitzer observations from the
Spitzer Survey of Virgo (SPITSOV) in combination with H-alpha observations. The
purpose of our study is to explore the relationship between the star formation
distribution within galaxies and the type (and phase) of interactions
experienced within the cluster environment. Neither highly-obscured star
formation nor strongly enhanced star-forming regions along the leading edges of
galaxies experiencing ICM-ISM interactions were found. However, very unobscured
star-forming regions were found in the outer parts of one galaxy (NGC 4402),
while relatively obscured star-forming regions were found in the extraplanar
regions of another galaxy (NGC 4522). We attribute the observed differences
between NGC 4402 and NGC 4522 to the direction of motion of each galaxy through
the ICM.
