After almost seventeen years since the first signal was detected, in January this year scientist at the observatory installed much more sophisticated detectors to analyze the interference. The readings provided by the detectors showed the strength of the signals in the range of 2.4 GHz, which was a familiar figure, a figure normally associated with Microwave ovens. Initial testing of the Microwave kept at the facility did not give perytons, however when the over door was opened during it was heating the food, suddenly the interference was detected.
Johnston said that the interference is a major issue when it comes to sophisticated observatories, and astronomers have always been raising concerns about the increasing radio interference in the atmosphere. However Johnston admitted that this problem is going to get much more complex considering the uncontrollable surge in mobile technology and radio communications. The reason most of the observatories are built in the middle of nowhere is because astronomers prefer to work under conditions where least possible local interference hinders their work.
During the Apollo missions to the moon, the Parkes Observatory was used to relay communication and telemetry signals to NASA, providing coverage for when the moon was on the Australian side of the Earth. The telescope also played a role in relaying data from the NASA Galileo mission to Jupiter that required radio-telescope support due to the use of its backup telemetry subsystem as the principal means to relay science data.
The observatory has remained involved in tracking numerous space missions up to the present day, including:
Apollo 11 broadcast
When Buzz Aldrin switched on the TV camera on the Lunar Module, three tracking antennas received the signals simultaneously. They were the 64 metre Goldstone antenna in California, the 26 metre antenna at Honeysuckle Creek near Canberra in Australia, and the 64 metre dish at Parkes.
In the first few minutes of the broadcast, NASA alternated between the signals being received from its two stations at Goldstone and Honeysuckle Creek, searching for the best quality picture.
A little under nine minutes into the broadcast, the TV was switched to the Parkes signal. The quality of the TV pictures from Parkes was so superior that NASA stayed with Parkes as the source of the TV for the remainder of the 2.5 hour broadcast. For a comprehensive explanation of the TV reception of the Apollo 11 broadcast, see “The Television Broadcasts” from the report “On Eagles Wings”.
On Monday, 31 October 2011, Google replaced its logo with a Google Doodle in honor of Parkes Observatory’s 50th Anniversary. It was only visible on Google in Australia.