So Nelly and Skelton Key were fed up of me traipsing down to their patch in Essex, and demanded that I show them ‘Derelict Cambridge’. Well, due to land value there’s nothing here. I done my best tho and scraped together 5 sites. This being the last.
I wouldn’t normally leave the name out,=, it’s a well know site, especially if you’re local. There just seems to be an outrageous media frenzy going on at the mo, and I just don’t fancy seeing ridiculous “Urban Explorers raid on observatory headlines. The site is still in use, however these are now unused, or derelict.
So visited one lovely sunny afternoon with Nelly, Skeleton Key, Mr & Mrs Trogladyte, Cheiftan, and a guy with a video camera.
These Telescopes are 60-ft-diameter parabolic reflectors operating simultaneously at 1407 MHz and 408 MHz) designed to perform aperture synthesis interferometry. So there. And was completed around 1964.
There’s a few of them on rails, the idea being that even a few meters apart they could still ‘triangulate’ results from far away planets.
In 1971, Sir Martin Ryle described why, in the late 1950s, radio astronomers decided on the construction of this telescope: "Our object was twofold. First we wanted to extend the range of our observations far back in time to the earliest days of the Universe, and this required a large increase in both sensitivity and resolution. With greater resolution we hoped that we might be able to draw radio maps of individual radio sources with sufficient detail to give some indication of the physical processes which brought them into being."
The telescope was made up of three 120 ton dishes, each of which is 18 m in diameter. Two of the dishes are fixed, while the third can be moved along an 800 m long (half mile) rail track, at speeds of up to 6.4 km/h. There were 60 different stations along the track, which is straight to within 0.9 cm, and whose far end was raised by 5 cm to allow for the curvature of the Earth over its length. The observing frequencies were usually 408 MHz (75 cm; the resolution was 80 arcsec)[1] and 1.4 GHz (21 cm; the resolution was 20 arcsec, three times better than that of the unaided eye).
Spot The Skeleton Key:
Over a 20 year career, the telescope was used to map individual objects, and to do several deep field surveys. Though still occasionally used, it is now essentially retired (one of the dishes is occasionally used for undergraduate projects or by amateur radio astronomers).
The construction of this telescope and development of the Earth-rotation aperture synthesis used when operating it contributed to Martin Ryle and Antony Hewish receiving the Nobel Prize for Physics in 1974.
Group shot:
Video coming as soon as I find a suitable soundtrack. Really looking forward to everyone else’s pics - already seen a couple of Nelly‘s and they are epic!
Thanks for looking.
I wouldn’t normally leave the name out,=, it’s a well know site, especially if you’re local. There just seems to be an outrageous media frenzy going on at the mo, and I just don’t fancy seeing ridiculous “Urban Explorers raid on observatory headlines. The site is still in use, however these are now unused, or derelict.
So visited one lovely sunny afternoon with Nelly, Skeleton Key, Mr & Mrs Trogladyte, Cheiftan, and a guy with a video camera.
These Telescopes are 60-ft-diameter parabolic reflectors operating simultaneously at 1407 MHz and 408 MHz) designed to perform aperture synthesis interferometry. So there. And was completed around 1964.
There’s a few of them on rails, the idea being that even a few meters apart they could still ‘triangulate’ results from far away planets.
In 1971, Sir Martin Ryle described why, in the late 1950s, radio astronomers decided on the construction of this telescope: "Our object was twofold. First we wanted to extend the range of our observations far back in time to the earliest days of the Universe, and this required a large increase in both sensitivity and resolution. With greater resolution we hoped that we might be able to draw radio maps of individual radio sources with sufficient detail to give some indication of the physical processes which brought them into being."
The telescope was made up of three 120 ton dishes, each of which is 18 m in diameter. Two of the dishes are fixed, while the third can be moved along an 800 m long (half mile) rail track, at speeds of up to 6.4 km/h. There were 60 different stations along the track, which is straight to within 0.9 cm, and whose far end was raised by 5 cm to allow for the curvature of the Earth over its length. The observing frequencies were usually 408 MHz (75 cm; the resolution was 80 arcsec)[1] and 1.4 GHz (21 cm; the resolution was 20 arcsec, three times better than that of the unaided eye).
Spot The Skeleton Key:
Over a 20 year career, the telescope was used to map individual objects, and to do several deep field surveys. Though still occasionally used, it is now essentially retired (one of the dishes is occasionally used for undergraduate projects or by amateur radio astronomers).
The construction of this telescope and development of the Earth-rotation aperture synthesis used when operating it contributed to Martin Ryle and Antony Hewish receiving the Nobel Prize for Physics in 1974.
Group shot:
Video coming as soon as I find a suitable soundtrack. Really looking forward to everyone else’s pics - already seen a couple of Nelly‘s and they are epic!
Thanks for looking.