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Stephen R. Sutton

Researcher at University of Chicago

Publications -  288
Citations -  10092

Stephen R. Sutton is an academic researcher from University of Chicago. The author has contributed to research in topics: Microprobe & XANES. The author has an hindex of 51, co-authored 287 publications receiving 9319 citations. Previous affiliations of Stephen R. Sutton include Argonne National Laboratory & Brookhaven National Laboratory.

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Comet 81P/Wild 2 under a microscope.

Donald E. Brownlee, +185 more
- 15 Dec 2006 - 
TL;DR: The Stardust spacecraft collected thousands of particles from comet 81P/Wild 2 and returned them to Earth for laboratory study, and preliminary examination shows that the nonvolatile portion of the comet is an unequilibrated assortment of materials that have both presolar and solar system origin.
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Structure of the Hydrated α-Al2O3 (0001) Surface

TL;DR: The physical and chemical properties of the hydrated α-Al2O3 (0001) surface are important for understanding the reactivity of natural and synthetic aluminum-containing oxides as mentioned in this paper.
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Advanced flat top laser heating system for high pressure research at GSECARS: application to the melting behavior of germanium

TL;DR: In this article, the flat top laser heating (FTLH) technique was used for in-situ high pressure high temperature studies into the physical and chemical properties of materials in the diamond anvil cell (DAC) and minerals at conditions relevant to the Earth's deep interior.
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Laser heated diamond cell system at the Advanced Photon Source for in situ x-ray measurements at high pressure and temperature

TL;DR: In this article, a double-sided laser heating system was used for in situ x-ray measurements at simultaneously ultrahigh pressures (to >150 GPa) and ultrahigh temperatures (to ∼4000 K) at the Advanced Photon Source.
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Elemental Compositions of Comet 81P/Wild 2 Samples Collected by Stardust

George J. Flynn, +79 more
- 15 Dec 2006 - 
TL;DR: The elements Cu, Zn, and Ga appear enriched in this Wild 2 material, which suggests that the CI meteorites may not represent the solar system composition for these moderately volatile minor elements.