<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>S. W. Ruff</dc:contributor>
  <dc:contributor>R.L. Fergason</dc:contributor>
  <dc:contributor>A.T. Knudson</dc:contributor>
  <dc:contributor>S. Anwar</dc:contributor>
  <dc:contributor>R. E. Arvidson</dc:contributor>
  <dc:contributor>J. L. Bandfield</dc:contributor>
  <dc:contributor>D.L. Blaney</dc:contributor>
  <dc:contributor>C. Budney</dc:contributor>
  <dc:contributor>W. M. Calvin</dc:contributor>
  <dc:contributor>T.D. Glotch</dc:contributor>
  <dc:contributor>M.P. Golombek</dc:contributor>
  <dc:contributor>N. Gorelick</dc:contributor>
  <dc:contributor>T.G. Graff</dc:contributor>
  <dc:contributor>V.E. Hamilton</dc:contributor>
  <dc:contributor>A. Hayes</dc:contributor>
  <dc:contributor>J. R. Johnson</dc:contributor>
  <dc:contributor>H.Y. McSween Jr.</dc:contributor>
  <dc:contributor>G.L. Mehall</dc:contributor>
  <dc:contributor>L.K. Mehall</dc:contributor>
  <dc:contributor>J.E. Moersch</dc:contributor>
  <dc:contributor>R.V. Morris</dc:contributor>
  <dc:contributor>A.D. Rogers</dc:contributor>
  <dc:contributor>M. D. Smith</dc:contributor>
  <dc:contributor>S. W. Squyres</dc:contributor>
  <dc:contributor>M.J. Wolff</dc:contributor>
  <dc:contributor>M.B. Wyatt</dc:contributor>
  <dc:creator>P. R. Christensen</dc:creator>
  <dc:date>2004</dc:date>
  <dc:description>The Miniature Thermal Emission Spectrometer (Mini-TES) on Spirit has studied the mineralogy and thermophysical properties at Gusev crater. Undisturbed soil spectra show evidence for minor carbonates and bound water. Rocks are olivine-rich basalts with varying degrees of dust and other coatings. Dark-toned soils observed on disturbed surfaces may be derived from rocks and have derived mineralogy (??5 to 10%) of 45% pyroxene (20% Ca-rich pyroxene and 25% pigeonite), 40% sodic to intermediate plagioclase, and 15% olivine (forsterite 45% ??5 to 10). Two spectrally distinct coatings are observed on rocks, a possible indicator of the interaction of water, rock, and airfall dust. Diurnal temperature data indicate particle sizes from 40 to 80 ??m in hollows to ???0.5 to 3 mm in soils.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1126/science.1100564</dc:identifier>
  <dc:language>en</dc:language>
  <dc:title>Initial results from the Mini-TES experiment in Gusev crater from the Spirit rover</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>