  We present two weak lensing reconstructions of the nearby ($z_{cl}=0.055$)
merging cluster Abell 3667, based on observations taken $\sim 1$ year apart
under different seeing conditions. This is the lowest redshift cluster with a
weak lensing mass reconstruction to date. The reproducibility of features in
the two mass maps demonstrate that weak lensing studies of low-redshift
clusters are feasible. These data constitute the first results from an X-ray
luminosity-selected weak lensing survey of 19 low-redshift ($z< 0.1$) southern
clusters.
