Dan McKenzie (geophysicist)

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Dan McKenzie
Born (1942-02-21) 21 February 1942 (age 82)
NationalityBritish
Alma materKing's College, Cambridge, (BA 1963, PhD 1966)
AwardsA.G. Huntsman Award (1980)
Balzan Prize (1981)
Wollaston Medal (1983)
Japan Prize (1990)
Royal Medal (1991)
Copley Medal (2011)
William Bowie Medal (2001)
Crafoord Prize (2002)
Scientific career
FieldsGeophysics
InstitutionsUniversity of Cambridge
Thesis The shape of the earth  (1967)
Doctoral advisorTeddy Bullard

Dan Peter McKenzie

the Cambridge Department of Earth Sciences. He wrote the first paper defining the mathematical principles of plate tectonics on a sphere, and his early work on mantle convection
created the modern discussion of planetary interiors.

Early life

Born in

, London.

Education and career

McKenzie attended King's College, Cambridge where he read physics, obtaining a 2:1 in his final degree.[1]

As a graduate student, he worked with

Freeman Gilbert and Walter Munk. After eight months he returned to Cambridge, submitting his PhD in 1966. He has since said that nothing in his early life as a scientist had such a profound effect on him as those eight months in California.[2]

Plate tectonics

Spending time between Cambridge and a Fellowship held in

Caltech, McKenzie was invited, along with Teddy Bullard, to a conference in New York which initiated his revolutionary work on plate tectonics. After listening to separate talks from Fred Vine on plate tectonics,[3] looking at the thermal structure of oceanic plates as they formed and cooled.[1]

Following this, he published a seminal paper with

Euler's Fixed Point Theorem, in conjunction with magnetic anomalies and earthquakes to determine a precise mathematical theory on plate tectonics. This work was published some 3–4 months after the same work had been carried out by Jason Morgan at Princeton. Allegations were subsequently made suggesting that McKenzie was at Morgan's spring AGU talk where he presented his plate tectonics work.[1] Later in 1968 he went to Princeton where he found that he and Morgan had solved two or three problems using identical mathematics in exactly the same way – plate tectonics was one, another was the thermal structure of the oceans and another was looking at earthquake mechanisms in a different way to seismologists.[1]

Working with John Sclater, McKenzie determined the entire geological history of the Indian Ocean, the publication[5] of which eventually resulted in them both receiving Fellowships at the Royal Society.

Mantle convection and sedimentary basins

McKenzie was awarded a University position and took it up in 1969. At this point he decided to move away from plate tectonics, choosing instead to focus on the behavior of fluids below the plates. He studied cellular convection and motions in the mantle whilst at the same time pursuing yet another new avenue of research; the development of

sedimentary basins. It was from this work that he produced a classic paper[6] that has been widely accepted by oil companies as the "McKenzie Model of Sedimentary Basins."[1]

McKenzie was elected a Fellow of the Royal Society in 1976 aged just 34, and by 1978 was awarded a University Readership position.

Later career

McKenzie continues to work at the Bullard Laboratories in Cambridge where he is Professor of Earth Science. Most recently his research has provided new insights into the tectonic evolution of Mars and Venus. In 2002 he was awarded the prestigious

Member of the Order of the Companions of Honour in 2003, he brought the then current Cambridge membership of this elite group to four: Brenner, McKenzie, Hobsbawm and Hawking. He also served on the Physical Sciences jury for the Infosys Prize
from 2009 to 2011.

Selected bibliography

Awards

References

External links