Abell 3627, also known as the Norma Cluster, is a rich, nearby galaxy cluster with catalogued cluster galaxies within the 2 Mpc Abell radius. Near the edge of the cluster lies the remarkable head-tail “Corkscrew Galaxy” 1610–60.5, characterised by its long, collimated and twisting radio tail. Koribalski et al. report on deep radio continuum images made with ASKAP data at 944 MHz and 1.4 GHz. While the brighter (younger) part of the Corkscrew Galaxy tail is highly collimated, the fainter (older) part shows increasing oscillation amplitudes, break-ups, and filaments. The host galaxy of the radio source, ESO 137-G007, is likely moving at high speed through the intracluster medium (ICM) perpendicular to our line-of-sight. Interactions of the radio galaxy tail with the Inter Cluster Medium are likely responsible for the tail collimation and its increasingly filamentary structure.