PHOTOMETRY OF THE OUTER HALO GLOBULAR-CLUSTERS NGC 5024 AND NGC 5053

New CCD photometry of the low-metallicity outer halo globular clusters NGC 5024 and NGC 5053 is used to construct BV color-magnitude diagrams that reach approximately 2 mag fainter than the turnoff in these clusters. A differential comparison of the color-magnitude diagrams with that of M92 indicates all three clusters are identical in age to within the uncertainties of the observations. With the addition of these two clusters, color-magnitude diagrams are now available for more than half of the globular clusters with [Fe/H] < - 2.0, and with the exception of Ruprecht 106, no discernible spread in age among these clusters is detected.