Age, Biography and Wiki

Leslie H. Martin was born on 21 December, 1900 in Footscray, Victoria, is an Australian physicist. Discover Leslie H. Martin's Biography, Age, Height, Physical Stats, Dating/Affairs, Family and career updates. Learn How rich is he in this year and how he spends money? Also learn how he earned most of networth at the age of 82 years old?

Popular As N/A
Occupation N/A
Age 82 years old
Zodiac Sign Sagittarius
Born 21 December, 1900
Birthday 21 December
Birthplace Footscray, Victoria
Date of death 1 February, 1983
Died Place Camberwell, Victoria
Nationality Australia

We recommend you to check the complete list of Famous People born on 21 December. He is a member of famous with the age 82 years old group.

Leslie H. Martin Height, Weight & Measurements

At 82 years old, Leslie H. Martin height not available right now. We will update Leslie H. Martin's Height, weight, Body Measurements, Eye Color, Hair Color, Shoe & Dress size soon as possible.

Physical Status
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Dating & Relationship status

He is currently single. He is not dating anyone. We don't have much information about He's past relationship and any previous engaged. According to our Database, He has no children.

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Leslie H. Martin Net Worth

His net worth has been growing significantly in 2023-2024. So, how much is Leslie H. Martin worth at the age of 82 years old? Leslie H. Martin’s income source is mostly from being a successful . He is from Australia. We have estimated Leslie H. Martin's net worth, money, salary, income, and assets.

Net Worth in 2024 $1 Million - $5 Million
Salary in 2024 Under Review
Net Worth in 2023 Pending
Salary in 2023 Under Review
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Timeline

1851

Laby nominated him for an 1851 Research Fellowship and a free trip to England to study physics under Ernest Rutherford at the University of Cambridge's Cavendish laboratory.

1900

Sir Leslie Harold Martin, (21 December 1900 – 1 February 1983) was an Australian physicist.

Leslie Harold Martin was born in the Melbourne suburb of Footscray on 21 December 1900, to Henry Richard Martin, a railway worker, and his wife Esther (Ettie) Emily, née Tutty.

1917

He attended Flemington State School and won a Junior State Scholarship to Melbourne High School for his final years of secondary schooling in 1917 and 1918.

1918

His mathematics teacher, Miss Julia Flynn, encouraged him, and he won a Victorian Education Department Senior Government Scholarship in 1918.

1919

He entered the University of Melbourne on the scholarship in 1919, to study for a Bachelor of Science for Education, with the intention of becoming a maths teacher.

1921

In 1921, in his final year, he came top of his year with first class honours in Natural Philosophy (physics) and was awarded the Dixson Scholarship in Natural Philosophy.

1922

In 1922, he completed his Master of Science degree, writing his master's thesis on "The emission of X Rays" under the supervision of Professor T. H. Laby.

He was awarded first class honours and both the Dixson and Kernot Scholarships.

1923

Martin was awarded the Fred Knight Research Scholarship in 1923, which allowed him to continue his research with Laby.

He earned extra money as a demonstrator in the Department of Natural Philosophy, and he lectured in the evenings at the Working Men's College.

Before departing, he married Gladys Maude Elaine Bull, a Bachelor of Music student at the University of Melbourne, at St James's Church of England in Ivanhoe on 13 February 1923.

She did not complete her studies, but instead accompanied him to England, sailing on the SS Berrima.

1924

They had two sons; the first, Leon Henry Martin, born in Cambridge on 25 April 1924.

When Gladys became pregnant again, she decided to return to Australia to be with her parents.

1926

Their second son, Raymond Leslie Martin, was born on 3 February 1926.

Leon died on the return voyage to England on the SS Benalla in July 1926.

Martin enrolled at Trinity College, Cambridge, and continued his research into X-rays under Rutherford's supervision.

He completed his PhD in 1926.

The results of this work were published in the Proceedings of the Royal Society of London, and the Proceedings of the Cambridge Philosophical Society.

1927

He was awarded an International Research Fellowship by the Rockefeller Foundation, allowing him to stay on into 1927.

He later recalled that:"John Cockcroft and I worked in the same room at the Cavendish Laboratory. We designed a half-million-volt accelerator tube which was used with a powerful Tesla to produce fast electrons. The electric field around the H.T. electrode produced magnificent coloured discharges in vacuum tubes. These fascinated Rutherford. He loved to edge closer to the H.T. electrode holding a vacuum tube at arm's length in an attempt to increase the brilliance of the electrical display. These visitations scared us. Cockcroft ultimately passed a spark to earth through a lump of meat, boring a hole half an inch in diameter. This impressed Rutherford, who liked the direct approach but his visits became less frequent."

Martin applied for a position as a lecturer at the University of Melbourne in January 1927.

He was successful, and returned to Australia in August 1927.

His corner of the Cavendish Laboratory was taken over by Ernest Walton.

Martin continued his research into X-rays, working with Laby, J. C. Bower and F. F. H. Eggleston.

1934

He won the David Syme Research Prize in 1934, for his investigation of the Auger effect, the emission of electrons after ionisation by X-rays.

Work with the chemical element xenon gave important confirmation of Paul Dirac's quantum field theory.

1937

In 1937 he became an associate professor in Natural Philosophy, and second-in-charge of the Natural Philosophy Department.

1939

With the outbreak of the Second World War in September 1939, Martin commenced projects at the request of the Australian Defence Forces, investigating a proximity fuse for the Australian Army and an acoustic communications system for the Royal Australian Air Force (RAAF) that would allow an instructor and trainee pilot to converse with each other.

He led a team that built a prototype Height and Range

1941

Finder No. 3, Mark IV, for the Army, but the Army cancelled the order in August 1941 when the prototype was nearly complete.

1942

In January 1942, he was seconded to the Council for Scientific and Industrial Research's Radiophysics Laboratory in Sydney to develop secret valves for a Radio Direction Finder.

He teamed up with Eric Burhop to build a magnetron, producing a working prototype on 23 May 1942.

He then went on to build an original magnetron that generated 25 centimetre microwave radiation.

These magnetrons were used in radar equipment by the Army, RAAF, Royal Australian Navy (RAN), and United States Army Air Forces (USAAF).

1945

He was Professor of Physics at the University of Melbourne from 1945 to 1959, and Dean of the Faculty of Military Studies and Professor of Physics at the University of New South Wales at the Royal Military College, Duntroon, in Canberra from 1967 to 1970.

1948

He was the Defence Scientific Adviser and chairman of the Defence Research and Development Policy Committee from 1948 to 1968, and a member of the Australian Atomic Energy Commission from 1958 to 1968.

In this role he was an official observer at several British nuclear weapons tests in Australia.

1959

He was one of the 24 Founding Fellows of the Australian Academy of Science and had a significant influence on the structure of higher education in Australia as chairman of the Australian Universities Commission from 1959 until 1966.