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Professor Bernatowicz received his undergraduate degree from Edinboro University of Pennsylvania in 1974, and his Ph.D. from Washington University in 1980. He is now a member of the Washington University Physics Department, where he is a Professor of Physics. He has worked on a wide variety of problems in planetary geochemistry and geophysics, surface physics, and experimental nuclear physics, isotope geochemistry and astrophysics. He is a Fellow of the American Physical Society, a Fellow of the Meteoritical Society, a member of the American Astronomical Society and of the American Geophysical Union. He has served on a number of national committees, among them the National Research Council Associateship Program, the NASA Cosmochemistry Program Management Operations Working Group, and the NSF Meteorite Working Group. The graduate work of Prof. Bernatowicz included determination of average uranium content of lunar breccias by fission track methods; petrographic studies of lunar rocks; noble gas investigations of lunar fission Xe from the extinct isotope Pu-244; application of heavy noble gases to petrological problems, including the development of the first degassing models for the Earth using Xe isotopes. Professor Bernatowicz' post-graduate research has included: evaluations of the terrestrial inventory of Xe; development of techniques for using mass spectrometers to study adsorption of noble gases in very low surface coverage regimes; the study of adsorption and migration of Xe and Ar in the lunar regolith; determination of actinide element abundances in meteorites; experimental studies of the solubilities of noble gases in silicate melts; theoretical and laboratory studies of isotopic fractionation during equilibrium adsorption and very low energy ion implantation of noble gases; proof of the double beta decay of Te-128 and measurement of its half-life (8 x 10^24 yr - the longest half-life ever determined experimentally); determination of a strict upper limit on the Majorana mass of the electron neutrino (< 1.5 eV) from experimental double beta decay lifetimes of Te-128 and Te-130. |
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Research InterestsThe current research of Professor Bernatowicz focuses on detailed laboratory observations of presolar grains (literally ancient stardust) from meteorites to draw inferences about the physical conditions in ancient circumstellar environments and about the formation of dust in the Galaxy. His research utilizes isotope mass spectrometry and transmission electron microscopy (electron diffraction, electron energy loss spectrometry and energy dispersive X-ray spectrometry). Some of his contemporary publications on the topic of the laboratory study of ancient stardust include: Daulton T. L., Bernatowicz T. J., Lewis R. S., Messenger S.,
Stadermann F. J., and Amari S. (2002) Bernatowicz T. J., Messenger S., Pravdivtseva O., Swan P., and
Walker R. M. (2003) Croat T. K., Bernatowicz T., Amari S., Messenger S., and
Stadermann F. J. (2003) Daulton T. L., Bernatowicz T. J., Lewis R. S., Messenger S.,
Stadermann F. J., and Amari S. (2003) Croat T. K., Stadermann F. J., and Bernatowicz T. J. (2005) Bernatowicz T. J., Akande O. W., Croat T. K., and Cowsik R.
(2005) |
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Contact |
Thomas J Bernatowicz |
Phone: (314) 935-6274 |
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