Donald L. Turcotte

Last updated
Donald Turcotte
Born (1932-04-22) April 22, 1932 (age 90)
Alma mater Caltech (BS, 1954)
Cornell University (MAeroEng, 1955)
Caltech (PhD, 1958) [1]
Known for Geophysics
Awards Arthur L. Day Medal(1981), Charles A. Whitten Medal (1995), William Bowie Medal (2002)
Scientific career
Institutions Cornell
UC Davis
Thesis An Experimental Investigation of Flame Stabilization in a Heated Turbulent Boundary Layer
Doctoral advisor Frank E. Marble
Notable students Louise Kellogg, E Marc Parmentier, Bruce Malamud

Donald Lawson Turcotte (born 22 April 1932) is an American geophysicist most noted for his work on the boundary layer theory of mantle convection as part of the theory of plate tectonics. [2] He works at the University of California, Davis.

Contents

Education and career

Turcotte trained as an engineer, graduating with a PhD in aeronautics and physics from Caltech in 1958. After a year at the Naval Postgraduate School in Monterey, Turcotte took up a position at Cornell University, in the graduate school of Aeronautical Engineering. [3] In 1965, Turcotte took a sabbatical at the University of Oxford, in the engineering department. Here he met Ron Oxburgh, who had recently arrived in the Department of Geology, and they began a collaboration in which they developed ideas about convective flow in the Earth's mantle, and its links to the newly emerging ideas of plate tectonics. [4] In 1973, Turcotte moved to the geology department at Cornell where he worked for the next thirty years. After retiring from Cornell in 2003, Turcotte moved to University of California, Davis.

He has won awards including the Arthur L. Day Medal of the Geological Society of America, the William Bowie Medal [5] and the Charles A. Whitten Medal of the American Geophysical Union. He is a member of the National Academy of Sciences. [6]

In 2008, the American Geophysical Union's Nonlinear Geophysics committee established the Donald L. Turcotte Award, which is given annually to one honoree "in recognition of outstanding dissertation research that contributes directly to nonlinear geophysics." [7]

Books

Related Research Articles

<span class="mw-page-title-main">Plate tectonics</span> Movement of Earths lithosphere

Plate tectonics is the generally accepted scientific theory that considers the Earth's lithosphere to comprise a number of large tectonic plates which have been slowly moving since about 3.4 billion years ago. The model builds on the concept of continental drift, an idea developed during the first decades of the 20th century. Plate tectonics came to be generally accepted by geoscientists after seafloor spreading was validated in the mid to late 1960s.

<span class="mw-page-title-main">Geophysics</span> Physics of the Earth and its vicinity

Geophysics is a subject of natural science concerned with the physical processes and physical properties of the Earth and its surrounding space environment, and the use of quantitative methods for their analysis. The term geophysics classically refers to solid earth applications: Earth's shape; its gravitational, magnetic fields, and electromagnetic fields ; its internal structure and composition; its dynamics and their surface expression in plate tectonics, the generation of magmas, volcanism and rock formation. However, modern geophysics organizations and pure scientists use a broader definition that includes the water cycle including snow and ice; fluid dynamics of the oceans and the atmosphere; electricity and magnetism in the ionosphere and magnetosphere and solar-terrestrial physics; and analogous problems associated with the Moon and other planets.

<span class="mw-page-title-main">Lithosphere</span> Outermost shell of a terrestrial-type planet or natural satellite

A lithosphere is the rigid, outermost rocky shell of a terrestrial planet or natural satellite. On Earth, it is composed of the crust and the portion of the upper mantle that behaves elastically on time scales of up to thousands of years or more. The crust and upper mantle are distinguished on the basis of chemistry and mineralogy.

<span class="mw-page-title-main">Asthenosphere</span> Highly viscous, mechanically weak, and ductile region of Earths mantle

The asthenosphere is the mechanically weak and ductile region of the upper mantle of Earth. It lies below the lithosphere, at a depth between ~80 and 200 km below the surface, and extends as deep as 700 km (430 mi). However, the lower boundary of the asthenosphere is not well defined.

<span class="mw-page-title-main">Harry Hammond Hess</span> American geologist

Harry Hammond Hess was an American geologist and a United States Navy officer in World War II who is considered one of the "founding fathers" of the unifying theory of plate tectonics. He is best known for his theories on sea floor spreading, specifically work on relationships between island arcs, seafloor gravity anomalies, and serpentinized peridotite, suggesting that the convection of the Earth's mantle was the driving force behind this process.

Dan Peter McKenzie is a Professor of Geophysics at the University of Cambridge, and one-time head of the Bullard Laboratories of 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.

<span class="mw-page-title-main">Geothermal gradient</span> Rate of temperature increase with depth in Earths interior

Geothermal gradient is the rate of temperature change with respect to increasing depth in Earth's interior. As a general rule, the crust temperature rises with depth due to the heat flow from the much hotter mantle; away from tectonic plate boundaries, temperature rises in about 25–30 °C/km (72–87 °F/mi) of depth near the surface in most of the world. However, in some cases the temperature may drop with increasing depth, especially near the surface, a phenomenon known as inverse or negative geothermal gradient. The effects of weather, sun, and season only reach a depth of approximately 10-20 metres.

<span class="mw-page-title-main">Don L. Anderson</span> American geophysicist

Don Lynn Anderson was an American geophysicist who made significant contributions to the understanding of the origin, evolution, structure, and composition of Earth and other planets. An expert in numerous scientific disciplines, Anderson's work combined seismology, solid state physics, geochemistry and petrology to explain how the Earth works. Anderson was best known for his contributions to the understanding of the Earth's deep interior, and more recently, for the plate theory hypothesis that hotspots are the product of plate tectonics rather than narrow plumes emanating from the deep Earth. Anderson was Professor (Emeritus) of Geophysics in the Division of Geological and Planetary Sciences at the California Institute of Technology (Caltech). He received numerous awards from geophysical, geological and astronomical societies. In 1998 he was awarded the Crafoord Prize by the Royal Swedish Academy of Sciences along with Adam Dziewonski. Later that year, Anderson received the National Medal of Science. He held honorary doctorates from Rensselaer Polytechnic Institute and the University of Paris (Sorbonne), and served on numerous university advisory committees, including those at Harvard, Princeton, Yale, University of Chicago, Stanford, University of Paris, Purdue University, and Rice University. Anderson's wide-ranging research resulted in hundreds of published papers in the fields of planetary science, seismology, mineral physics, petrology, geochemistry, tectonics and the philosophy of science.

<span class="mw-page-title-main">Mantle convection</span> Gradual movement of the planets mantle

Mantle convection is the very slow creeping motion of Earth's solid silicate mantle as convection currents carrying heat from the interior to the planet's surface.

<span class="mw-page-title-main">Geodynamics</span> Study of dynamics of the Earth

Geodynamics is a subfield of geophysics dealing with dynamics of the Earth. It applies physics, chemistry and mathematics to the understanding of how mantle convection leads to plate tectonics and geologic phenomena such as seafloor spreading, mountain building, volcanoes, earthquakes, faulting. It also attempts to probe the internal activity by measuring magnetic fields, gravity, and seismic waves, as well as the mineralogy of rocks and their isotopic composition. Methods of geodynamics are also applied to exploration of other planets.

(Stanley) Keith Runcorn was a British physicist whose paleomagnetic reconstruction of the relative motions of Europe and America revived the theory of continental drift and was a major contribution to plate tectonics.

<span class="mw-page-title-main">Outline of geophysics</span> Topics in the physics of the Earth and its vicinity

The following outline is provided as an overview of and topical guide to geophysics:

<span class="mw-page-title-main">Earth's internal heat budget</span> Accounting of the energy flows at and below the planets crust

Earth's internal heat budget is fundamental to the thermal history of the Earth. The flow of heat from Earth's interior to the surface is estimated at 47±2 terawatts (TW) and comes from two main sources in roughly equal amounts: the radiogenic heat produced by the radioactive decay of isotopes in the mantle and crust, and the primordial heat left over from the formation of Earth.

<span class="mw-page-title-main">Geodynamics of Venus</span>

NASA's Magellan spacecraft mission discovered that Venus has a geologically young surface with a relatively uniform age of 500±200 Ma. The age of Venus was revealed by the observation of over 900 impact craters on the surface of the planet. These impact craters are nearly uniformly distributed over the surface of Venus and less than 10% have been modified by plains of volcanism or deformation. These observations indicate that a catastrophic resurfacing event took place on Venus around 500 Ma, and was followed by a dramatic decline in resurfacing rate. The radar images from the Magellan missions revealed that the terrestrial style of plate tectonics is not active on Venus and the surface appears to be immobile at the present time. Despite these surface observations, there are numerous surface features that indicate an actively convecting interior. The Soviet Venera landings revealed that the surface of Venus is essentially basaltic in composition based on geochemical measurements and morphology of volcanic flows. The surface of Venus is dominated by patterns of basaltic volcanism, and by compressional and extensional tectonic deformation, such as the highly deformed tesserae terrain and the pancake like volcano-tectonic features known as coronae. The planet's surface can be broadly characterized by its low lying plains, which cover about 80% of the surface, 'continental' plateaus and volcanic swells. There is also an abundance of small and large shield volcanoes distributed over the planet's surface. Based on its surface features, it appears that Venus is tectonically and convectively alive but has a lithosphere that is static.

David Gubbins is a British former geophysicist concerned with the mechanism of the Earth's magnetic field and theoretical geophysics, but his real passion is coaches. He is Emeritus Professor of Earth Sciences at Leeds University.

Maureen D. Long is an observational seismologist studying mantle and Mesosphere dynamics. She currently serves as a professor at Yale University within the Department of Geology and Geophysics.

Alik Ismail-Zadeh is a mathematical geophysicist known for his contribution to computational geodynamics and natural hazard studies, pioneering work on data assimilation in geodynamics as well as for outstanding service to the Earth and space science community. He is Senior Research Fellow at the Karlsruhe Institute of Technology in Germany.

Ridge push or sliding plate force is a proposed driving force for plate motion in plate tectonics that occurs at mid-ocean ridges as the result of the rigid lithosphere sliding down the hot, raised asthenosphere below mid-ocean ridges. Although it is called ridge push, the term is somewhat misleading; it is actually a body force that acts throughout an ocean plate, not just at the ridge, as a result of gravitational pull. The name comes from earlier models of plate tectonics in which ridge push was primarily ascribed to upwelling magma at mid-ocean ridges pushing or wedging the plates apart.

Claude Jaupart is a French geophysicist and a member of the French Academy of Sciences.

References

  1. <Donald L. Turcotte. geo.cornell.edu
  2. Gates, Alexander E. (2003). "Turcotte, Donald L. (1932)". A to Z of earth scientists. New York: Facts on File. pp. 265–266. ISBN   9781438109190.
  3. "Donald L. Turcotte".
  4. Turcotte, Donald L.; Oxburgh, E. Ronald (1969). "Continental drift". Physics Today. 22 (4): 30–39. Bibcode:1969PhT....22d..30T. doi:10.1063/1.3035524.
  5. "Bowie Medal Citation". www.agu.org. Retrieved 2016-07-28.
  6. "Donald Turcotte". www.nasonline.org. Retrieved 2016-07-22.
  7. "Donald L. Turcotte Award". www.agu.org. Retrieved 2016-08-06.