Antony Hewish(1924 — 2021)

Antony Hewish

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SciencesScientifique20th Century20th century, the golden age of post-war British radio astronomy, at the University of Cambridge.

Antony Hewish (1924-2021) was a British radio astronomer. He led the work that resulted in the discovery of pulsars in 1967 and received the Nobel Prize in Physics for it in 1974, shared with Martin Ryle.

Frequently asked questions

Antony Hewish was a British radio astronomer born in 1924 in Fowey, Cornwall. The key thing to remember is that he led the work that resulted in the discovery of pulsars in 1967 at the University of Cambridge, a breakthrough that earned him the Nobel Prize in Physics in 1974, shared with Martin Ryle. Less a personal award than a recognition of the team, this Nobel sparked controversy because the student Jocelyn Bell, who had spotted the first signal, was not honoured.

Key Facts

  • Born on 11 May 1924 in Fowey (Cornwall), died on 13 September 2021
  • Designs the radio telescope that made it possible to detect the first pulsars in 1967
  • The discovery of the first pulsar is made by his doctoral student Jocelyn Bell in 1967
  • Receives the Nobel Prize in Physics in 1974 with Martin Ryle, the first Nobel awarded for work in astronomy
  • Professor of radio astronomy at the University of Cambridge

Works & Achievements

Construction of the interplanetary scintillation radio telescope (1965-1967)

Design of a vast array of antennas to study quasars through scintillation. This instrument made the discovery of pulsars possible.

Discovery of pulsars (1967)

Identification of the first pulsar, a rotating neutron star emitting regular radio pulses. A revolution for astrophysics.

Observation of a Rapidly Pulsating Radio Source (Nature) (1968)

Landmark paper, co-authored with Jocelyn Bell and others, announcing the discovery to the scientific world.

Work on interplanetary scintillation (1960s)

Study of how the solar wind makes radio waves from distant sources scintillate. A new method for probing the interplanetary medium.

Nobel Lecture “Pulsars and High Density Physics” (1974)

Talk given upon receiving the Nobel Prize, retracing the discovery and its implications for high-density physics.

Research on radar countermeasures (Second World War) (1943-1945)

Participation in the development of airborne radar jamming systems. This experience steered him toward radio astronomy.

Anecdotes

In 1967, it was Antony Hewish's doctoral student, Jocelyn Bell, who spotted on the radio telescope's long paper strips a strange signal repeating every 1.3 seconds. Half-jokingly, the team at first nicknamed it “LGM-1”, for “Little Green Men”, so artificial did the regularity of the signal seem.

The radio telescope that made the discovery of pulsars possible had not been designed for that purpose at all: Hewish wanted to study the scintillation of quasars. The instrument was a vast field of more than a thousand wooden posts linked by wires, covering the equivalent of 57 tennis courts, which students had helped to plant by hand.

The 1974 Nobel Prize in Physics sparked controversy: it rewarded Hewish and Martin Ryle, but not Jocelyn Bell, even though she had been the first to notice the signal. The astronomer Fred Hoyle protested publicly, and this “Nobel scandal” has remained a textbook case in debates about the place of doctoral students in major discoveries.

During the Second World War, the young Hewish worked on airborne radar countermeasure and jamming devices, alongside Martin Ryle. It was this wartime experience with radio waves that later led him toward the emerging field of radio astronomy at Cambridge.

A pulsar is in fact a rotating neutron star, so dense that a teaspoon of its matter would weigh hundreds of millions of tonnes. Hewish received the Nobel for having been able to prove that this signal truly came from a compact celestial object, and not from an instrument fault or a distant civilization.

Primary Sources

Observation of a Rapidly Pulsating Radio Source, Nature (February 24, 1968)
Unusual signals from pulsating radio sources have been recorded at the Mullard Radio Astronomy Observatory. The radiation seems to come from local objects within the galaxy, and may be associated with oscillations of white dwarf or neutron stars.
Pulsars and High Density Physics — Antony Hewish's Nobel Lecture (December 12, 1974)
The discovery of pulsars was an unexpected result of a search for the scintillation of compact radio sources. The first indication that something unusual was happening came in August 1967.
Official Biography, The Nobel Prize in Physics 1974 (1974)
Antony Hewish received the Nobel Prize in Physics for his decisive role in the discovery of pulsars, shared with Martin Ryle for their pioneering research in radio astrophysics.

Key Places

Fowey, Cornwall

Small port town in southwest England where Antony Hewish was born in 1924. His seaside childhood left a lasting mark on his love of science.

University of Cambridge

University where Hewish studied and then spent his entire career. He became professor of radio astronomy there in 1977.

Mullard Radio Astronomy Observatory

Cambridge's radio astronomy observatory, located at Lord's Bridge. This is where the radio telescope that detected the first pulsar was housed.

Cavendish Laboratory

Famous physics laboratory at the University of Cambridge where Hewish joined Martin Ryle's team. A landmark of 20th-century British physics.

Cottenham, Cambridgeshire

Village near Cambridge where Antony Hewish lived and died in 2021 at the age of 97.

See also