UC SANTA CRUZEarth & Planetary Sciences
About the DepartmentFacultyResearchGraduate ProgramUndergraduate ProgramCoursesNews & EventsSeminarsAlumni
UCSC A-Z IndexFind People

Earth & Planetary Sciences Faculty

Affiliated Faculty


Earth & Planetary Sciences Department
Earth & Marine Sci.
Santa Cruz, CA 95064
Phone: 831.459.4089
Fax: 831.459.3074
Maps & Directions


Other UCSC Links:
UCSC Home
Physical & Biological Sciences
Undergraduate Admissions
Graduate Admissions
Alumni Association

-- spacer
Quentin C. Williams  

QUENTIN C. WILLIAMS
Professor of Earth & Planetary Sciences
Mineral Physics, Experimental Geochemistry

Office: EMS A212
Phone: 831-459-3132
Fax: 831-459-3074
E-mail: qwilliams@es.ucsc.edu
Lab: C431/C483 x9-2596 x9-5355
 

For more information:
Website

Publications (PDF)


Education and Training
--

B.A., Princeton University
Ph.D., University of California, Berkeley

Research Interests --

The Earth's mantle and core comprise more than 99 percent of the mass of the planet. As such, the physical and chemical properties of these regions are critical in determining the processes by which the planet has evolved to its current state. Quentin Williams's research is centered on experimentally examining the structural and thermodynamic properties of minerals, melts, and fluids at both ambient and high pressures. In particular, the melting relations of deep Earth materials, the ability of deep Earth minerals (and melts) to retain water and carbon dioxide, the mineralogy of subduction zone materials, and the structural constraints that determine whether silicate magmas buoyantly rise or sink at different depths in the Earth are among his primary interests. Such properties not only control the thermal regime in the deep Earth (and thus the driving force of plate tectonics), but also are vital in determining the mechanisms and degree to which the planet has differentiated.

The principal tool Williams uses to study these problems is the high-temperature diamond anvil cell, a device by which pressures corresponding to those present throughout the deep Earth may be generated. Because of the transparency of diamond, probes such as Raman spectroscopy are used to examine the bonding properties of materials in situ at simultaneous high pressure and temperature. Such data yield insight into the local bonding environments of ions in crystals, melts, and solutions, and the changes in these environments with pressure and temperature.

Teaching Interests --

Evolution of the Earth | Thermochemistry of Geologic Systems | Comparative Planetology | Topics in Chemistry and Physics of the Earth

 

 
Home |  About the Department  | Faculty |  Research | Graduate |  Undergraduate | Courses |  News & Events | Seminars | Alumni
Copyright © University of California Santa Cruz. Last modified 12/1/06 by the  Earth & Planetary Sciences Webmaster.