Established 31 October 1961 Phone +61 2 6861 1777 | ||
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Website www.parkes.atnf.csiro.au Address Newell Hwy, Parkes NSW 2870, Australia Hours Closed now Thursday8:30AM–4:15PMFriday8:30AM–4:15PMSaturday8:30AM–4:15PMSunday8:30AM–4:15PMMonday8:30AM–4:15PMTuesday8:30AM–4:15PMWednesday8:30AM–4:15PMSuggest an edit Similar Green Bank Telescope, Arecibo Observatory, Jodrell Bank Observatory, Lovell Telescope, Canberra Deep Space Co | ||
Radio telescope time lapse parkes parkes observatory australia
The Parkes Observatory (also known informally as "The Dish") is a radio telescope observatory, located 20 kilometres north of the town of Parkes, New South Wales, Australia. It was one of several radio antennas used to receive live, televised images of the Apollo 11 moon landing on 20 July 1969. Its scientific contributions over the decades led the ABC to describe it as "the most successful scientific instrument ever built in Australia" after 50 years of operation.
Contents
- Radio telescope time lapse parkes parkes observatory australia
- This is the australian csiro parkes observatory
- Parkes Observatory Visitors Centre
- Radio telescope
- Hardware
- Receivers
- Historical non astronomy research
- Apollo 11 broadcast
- Mars rovers
- Astronomy research timeline
- In popular culture
- Relation to Breakthrough Listen
- References
The Parkes Observatory is run by the Commonwealth Scientific and Industrial Research Organisation (CSIRO) as part of the Australia Telescope National Facility (ATNF) network of radio telescopes. It is frequently operated together with other CSIRO radio telescopes, principally the array of six 22-metre (72 ft) dishes at the Australia Telescope Compact Array near Narrabri, and a single 22-metre (72 ft) dish at Mopra (near Coonabarabran), to form a very long baseline interferometry array.
This is the australian csiro parkes observatory
Parkes Observatory Visitors Centre
The Parkes Observatory Visitors Centre allows visitors to view the dish as it moves. There are exhibits about the history of the telescope, astronomy, and space science, and a 3-D movie theatre.
Radio telescope
The Parkes Radio Telescope, completed in 1961, was the brainchild of E.G. "Taffy" Bowen, chief of the CSIRO's Radiophysics Laboratory. During the Second World War, he had worked on radar development in the US and had made some powerful friends in the scientific community. Calling on this old boy network, he persuaded two philanthropic organisations, the Carnegie Corporation and the Rockefeller Foundation to fund half the cost of the telescope. It was this recognition and key financial support from the US that persuaded then prime minister Robert Menzies to agree to fund the rest of the project.
The radio telescope was declared a National Engineering Landmark by Engineers Australia.
Hardware
The primary observing instrument is the 64-metre (210 ft) movable dish telescope, second largest in the Southern Hemisphere, and one of the first large movable dishes in the world (DSS-43 'Deep Space Station'-43 at Tidbinbilla was extended from 64-metre (210 ft) to 70-metre (230 ft) in 1987, surpassing Parkes). After its completion it has operated almost continuously to the present day. The dish surface was physically upgraded by adding smooth metal plates to the central part to provide focusing capability for centimetre and millimetre length microwaves. The outer part of the dish remains a fine metal mesh, creating its distinctive two-tone appearance.
The 18-metre (59 ft) dish antenna was transferred from the Fleurs Observatory (Mills Cross) in 1963. Mounted on rails and powered by a tractor engine to allow the distance between it and the main dish to be easily varied, it was used as an interferometer with the main dish, and as a transmit uplink antenna in the Apollo program. It has been abandoned since the early 1980s.
The telescope has an altazimuth mount. It is guided by a small mock-telescope placed within the structure at the same rotational axes as the dish, but with an equatorial mount. The two are dynamically locked when tracking an astronomical object by a laser guiding system. This primary-secondary approach was designed by Barnes Wallis.
The success of the Parkes telescope led NASA to copy the basic design in their Deep Space Network, with matching 64 m dishes built at Goldstone, California, Madrid, Spain, and Tidbinbilla, Australia.
In 1998 Parkes telescope began detecting fast radio bursts and related signals named perytons. At the time it was theorised that these may have been a signals from another galaxy, emissions from neutron stars becoming black holes or interference from lightning strikes. In 2015 it was determined that perytons were caused by staff members opening the door of the facilities microwave oven during its cycle. When the microwave oven door was opened, 1.4 GHz microwaves from the magnetron shutdown phase were able to escape. ″Subsequent tests revealed that a peryton can be generated at 1.4 GHz when a microwave oven door is opened prematurely and the telescope is at an appropriate relative angle″. ″It is still not clear if microwave ovens can be blamed for all instances of peryton reception″.
Receivers
The receiving cabin is located at the focus of the parabolic dish, supported by three struts 27-metre (89 ft) above the dish. The cabin contains multiple radio and microwave detectors, which can be switched into the focus beam for different science observations.
The observatory is a part of the Australia Telescope National Facility network of radio telescopes. The 64m dish is frequently operated together with the Australia Telescope Compact Array at Narrabri and a single dish at Mopra, to form a very long baseline interferometry array.
Historical non-astronomy research
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:
The CSIRO has made several documentaries on this observatory, with some of these documentaries being posted to YouTube.
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 Australia replaced its logo with a Google Doodle in honor of Parkes Observatory's 50th Anniversary.
Mars rovers
In 2012 the Observatory received special signals from the Mars rover Opportunity (MER-B), to simulate the Curiosity rover UHF radio. This helped prepare for the then upcoming Curiosity (MSL) landing in early August—it successfully touched down on 6 August 2012.
Astronomy research timeline
1960s
1970s
1980s
1990s
2000s
In popular culture
Relation to Breakthrough Listen
The telescope will be used to search for radio waves in the 1–10 GHz range, a quiet zone uninterrupted by man-made or natural sources for the heavily funded project, Breakthrough Listen.