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Fri, Oct 10th, 2008, @11:00am Astronomy Group Meeting |
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Erik H. Hauri
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In 2000 Erik Hauri received the F. G. Houtermans Medal from the European
Association of Geochemistry for his outstanding contributions to geochemistry
as a young researcher. That same year he was also awarded the James B.
Macelwane Medal by the American Geophysical Union.

Erik Hauri studies melt inclusions (tiny bits of melt
trapped in crystals) with the ion microprobe to determine the origins
of volatile elements in the Earth’s interior. This melt inclusion
is from mid-ocean-ridge magma from the Siqueiros Fracture Zone, Pacific
Ocean.
(Photo courtesy Alberto Saal, Brown University.)
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Material in the atmosphere, the oceans, and the interior of the Earth
circulates as a result of convection—the fluid motion that is driven
by temperature variations and gravity. Geochemist Erik Hauri studies the
movement of matter in planetary interiors and the origin and role of water
in volcanic systems on Earth and the other terrestrial planets. Analysis
of different atomic species, or isotopes, combined with numerical modeling
and seismic imaging techniques are revealing what goes on inside the rocky
planets and the timing of processes that occurred during planetary evolution.
Hauri uses high-precision, highly sensitive mass spectrometry and other
methods to analyze the composition of magma samples from Earth and meteorites
and determine their implication for the composition and evolution of solar
system bodies. He also directs the Carnegie-National Science Foundation
National Ion Microprobe Facility — a resource for scientists from
around the world to make in situ geochemical measurements at the micron
scale.
Plate tectonics powers the convective process in Earth’s
interior, and the presence of liquid water at the surface is thought to
be a primary factor in keeping this system active. By investigating magmas,
Hauri’s analyses have revealed that water plays a significant role
in magma generation and differentiation in a variety of planetary environments.
His work also sheds light on the primordial conditions under which the
Earth formed. When the Earth was accreting, it became a sea of molten
rock. The interior became partly depleted in the volatile elements —
hydrogen, carbon, nitrogen, and sulfur — a loss that continues today
through the eruption and outgassing from active volcanoes.
Venus has outgassed water, but atmospheric water has been
broken down by solar ultraviolet radiation and the hydrogen lost to space.
Water on Mars is believed to be partly frozen as ice and trapped in the
crust. The lack of active plate tectonics on the other terrestrial planets
and other factors have led scientists to believe that water from the Earth’s
surface is carried into the interior by plate subduction — the process
in which the edge of one plate descends below another — and serves
as the lubricant that facilitates continued plate motions. Water-rich
explosive volcanism occurring at subduction zones confirms that water
is carried down with the descending plate. But two major questions about
the water budget at subduction zones remain unanswered: How much of the
water that goes down into subduction zones comes back up at volcanic eruptions,
and how much water is left in the subducting plate? Hauri is currently
exploring these and related questions.
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SELECTED PUBLICATIONS
- Hauri, E. H. 2002. Osmium isotopes
and mantle convection, Phil. Trans. Roy. Soc.
London Ser. A 360, 2371-2382.
- Hauri, E. H. 2002. SIMS investigations of volatiles
in silicate glasses 2: abundances
and isotopes in Hawaiian melt inclusions, Chem. Geol. 183, 115-141.
- Saal, A., E. H. Hauri, C. H. Langmuir, and M. Perfit.
2002. Vapor undersaturation in
primitive mid-ocean ridge basalt and the volatile content of the Earth’s
upper mantle,
Nature 419, 451-455.
- Van Keken, P. E., E. H. Hauri, and C. J. Ballentine.
2002. Mantle mixing: generation,
preservation, and destruction of chemical heterogeneity, Annu. Rev.
Earth Planet. Sci. 30,
493-525.
- Hauri, E. H. 1996. Major element variability in the
Hawaiian mantle plume, Nature 382,
415-419.
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