Martin Ryle

@Trinity College, Cambridge, Family and Personal Life

Sir Martin Ryle was a British astronomer who was one of the joint winners of Nobel Prize for Physics in 1974

Sep 27, 1918

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Biography

Personal Details

  • Birthday: September 27, 1918
  • Died on: October 14, 1984
  • Nationality: British
  • Famous: Oxford University, Trinity College, Cambridge, Scientists, Astronomers, Physicists
  • Universities:
    • Oxford University,Trinity College, Cambridge
    • University of Oxford
    • Christ Church
    • Oxford
    • Trinity College
    • Cambridge
    • Bradfield College
  • Notable Alumnis:
    • Oxford University
    • Trinity College
    • Cambridge
  • Birth Place: Brighton

Martin Ryle born at

Brighton

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Birth Place

In 1947, Martin Ryle married Ella Rowena Palmer; sister-in-law of fellow astronomer Sir Francis Graham-Smith. The couple had two daughters, Alison and Claire, and a son named John.

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Personal Life

They had a wonderfully happy marriage. The family enjoyed sailing and owned number of boats. Two of the boats were designed and built by Ryle himself.

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Personal Life

Ryle was active till his end. He died on 14 October 1984, at the age of 66, at Cambridge.

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Personal Life

Martin Ryle was born on 27 September 1918, in Sussex. His father, John Alfred Ryle, was a well-known physician and epidemiologist. Later, he was appointed to the first Chair of Social Medicine at Oxford University. His mother‘s name was Miriam (née Scully) Ryle. His uncle, Gilbert Ryle, was also a distinguished philosopher.

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Childhood & Early Years

Martin was the second child of his parents. He had four siblings; two brothers and two sisters. All the five siblings had their early education under a governess. Later Martin was admitted to Gladstone’s Preparatory School in Eaton Square, London.

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Childhood & Early Years

At the age of thirteen, Martin was sent to Bradfield College, a boarding and day school in Bradfield in the county of Berkshire, and passed out from there in 1936. Here, he developed an interest in radio engineering. Sometime now, he not only built his own radio transmitter, but also acquired a post office license for it.

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Childhood & Early Years

In 1936, Martin enrolled at Christ Church, a constituent college under the University of Oxford, with physics as his major. Here too he retained his interest in radio engineering and set up the university amateur radio station together with his fellow students. He graduated from there in 1939.

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Childhood & Early Years

In 1939, Martin Ryle briefly joined ionospheric research group at the Cavendish Laboratory at Cambridge University under J. A. Ratcliffe. However, the Second World War started soon after and with that Martin shifted to Telecommunication Research Establishment, which was working on radar system for R.A.F.

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Career

For the first two years, Ryle worked on the antennas for airborne radar equipment. Later, he was shifted to newly formed Radio Countermeasures Division. Here the main task was to jam transmitters against the German radar defense system and to devise radio-deception operations.

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Career

It may be noted that because of their work, Germany thought that the D-Day invasion would take place across the Strait of Dover, not at Normandy. Indeed, Ryle and his team had to work under a very stressful condition, having to find many immediate as well as practical solutions for tackling tricky situations.

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Career

During this period, the team also detected vulnerability in the Germany’s V-2 rocket radio guidance system. Very quickly, they developed a system through which the accurate aims of these rockets could be greatly disrupted, thereby reducing their harmful effects to a large extent.

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Career

About his war experience, Ryle later said that it helped him to learn many things about engineering and to understand and motivate people. At the same time, it also made him forgot all that he had learned about physics.

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Career

The invention of a more effective aperture synthesis in 1960s is definitely the biggest achievement OF Martin Ryle and his team. His team placed two telescopes at certain distances and by changing the distance between them and analyzing the results through computers, they received better and better resolving power.

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Major Works

In mid 1960s, they placed the two telescopes at a maximum distance of 1.6 km and found that a single telescope with 1.6 km diameter would give the same result. In 1967, Anthony Hewish and Jocelyn Bell of the Cambridge group used this principle to locate the first pulsar.

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Major Works