  As one of the lowest metallicity star forming galaxies, with a nucleus of
several super star clusters, SBS0335-052E is the subject of substantial current
study. We present new insights on this galaxy based on new and archival high
spatial resolution NICMOS and ACS images. We provide new measurements and
limits on the size of several of the SSCs. The images have sufficient
resolution to divide the star formation into compact regions and newly
discovered extended regions, indicating a bi-modal form of star formation. The
star formation regions are dated via the equivalent width of the Pa alpha
emission and we find that two of the extended regions of star formation are
less than 10 million years old. Our previous finding that stellar winds confine
the photo-ionizing flux to small regions around individual stars is consistent
with the new observations. This may allow planet formation in what would
traditionally be considered a harsh environment and has implications for the
number of planets around globular cluster stars. In addition the images
pinpoint the regions of H2 emission as located in, but not at the center of the
two star forming super star clusters, S1 and S2.
