[en] A summary of recent observations of galaxy clustering is presented, including a brief review of redshift maps and galaxy clustering statistics. The current major uncertainty is the nature of clustering on scales in excess of 10h/sup -1/Mpc. How should one reconcile the small correlation length measured for galaxy-galaxy clustering with the large correlation length associated with the clustering of Abell clusters? Simple arguments are presented that argue the underlying mass fluctuations are most likely associated with a clustering scale no larger than that of individual galaxies