  We review the properties of the 22 millisecond radio pulsars currently known
in the globular cluster 47 Tucanae, and their implications for the mass and gas
content of the cluster. Further details can be found in the publications from
this project to date (Camilo et al. 2000; Freire 2000; Freire et al. 2001a,b;
Freire et al. 2003). Throughout the review, we look ahead to the future results
anticipated from this fascinating cluster.
