Everything about The Cambridge Interferometer totally explained
The
Cambridge Interferometer was a
radio telescope interferometer built by
Martin Ryle and
Antony Hewish in the early 1950s to the west of
Cambridge (between the Grange Road football ground and the current
Cavendish Laboratory). The interferometer consisted of an array of 4 fixed elements to survey the sky. It produced the two Cambridge catalogues of radio sources (the
2C catalogue of radio sources at 81.5 MHz, and the
3C catalogue of radio sources at 159 MHz, building on the work of the
Preliminary survey of the radio stars in the Northern Hemisphere
at 45 MHz - 214 MHz using the 2-element
Long Michelson Interferometer), discovering some of the most interesting astronomical objects known. The telescope was operated by the
Radio Astronomy Group of
Cambridge University.
Martin Ryle and
Antony Hewish received the
Nobel Prize for Physics in
1974 for this and other related work.
==
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