This paper describes recent improvements to the Parkes 64 m radio tele
scope, now 33 years old. It is being upgraded to allow rapid switching
between receivers, and to track the best-fitting focus as the elevati
on angle changes. Carried out under contract on behalf of NASA, the up
grade included installing a low-noise 2.3 GHz receiver for tracking th
e spacecraft Galileo in 1997. We explain the mechanical and structural
aspects of the upgrade, including the need to replace the existing fo
cus cabin with a larger unit, and the effect of the increased weight a
t the prime focus on the focusing characteristics and reflector accura
cy. Finally, we summarize the designs of the feed and receiver to opti
mize the antenna-efficiency/temperature ratio at 2.3 GHz for the Galil
eo mission.