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Spectral properties of Titan's impact craters imply chemical weathering of its surface.

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Title: Spectral properties of Titan's impact craters imply chemical weathering of its surface.
Authors: Neish CD; Department of Physics and Space Sciences Florida Institute of Technology Melbourne Florida USA., Barnes JW; Department of Physics University of Idaho Moscow Idaho USA., Sotin C; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA., MacKenzie S; Department of Physics University of Idaho Moscow Idaho USA., Soderblom JM; Department of Earth, Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge Massachusetts USA., Le Mouélic S; Laboratoire de Planétologie et Géodynamique, LPGNantes, CNRS UMR 6112, Université de Nantes Nantes France., Kirk RL; United States Geological Survey, Astrogeology Science Center Flagstaff Arizona USA., Stiles BW; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA., Malaska MJ; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA., Le Gall A; Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin Paris France., Brown RH; Lunar and Planetary Laboratory University of Arizona Tucson Arizona USA., Baines KH; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA., Buratti B; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA., Clark RN; United States Geological Survey Denver Colorado USA., Nicholson PD; Department of Astronomy Cornell University Ithaca New York USA.
Source: Geophysical research letters [Geophys Res Lett] 2015 May 28; Vol. 42 (10), pp. 3746-3754. Date of Electronic Publication: 2015 May 26.
Publication Type: Journal Article
Journal Info: Publisher: American Geophysical Union Country of Publication: United States NLM ID: 9882887 Publication Model: Print-Electronic Cited Medium: Print ISSN: 0094-8276 (Print) Linking ISSN: 00948276 NLM ISO Abbreviation: Geophys Res Lett Subsets: PubMed not MEDLINE
Database: MEDLINE Ultimate
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  Data: Spectral properties of Titan's impact craters imply chemical weathering of its surface.
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  Data: <searchLink fieldCode="AU" term="%22Neish+CD%22">Neish CD</searchLink>; Department of Physics and Space Sciences Florida Institute of Technology Melbourne Florida USA.<br /><searchLink fieldCode="AU" term="%22Barnes+JW%22">Barnes JW</searchLink>; Department of Physics University of Idaho Moscow Idaho USA.<br /><searchLink fieldCode="AU" term="%22Sotin+C%22">Sotin C</searchLink>; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.<br /><searchLink fieldCode="AU" term="%22MacKenzie+S%22">MacKenzie S</searchLink>; Department of Physics University of Idaho Moscow Idaho USA.<br /><searchLink fieldCode="AU" term="%22Soderblom+JM%22">Soderblom JM</searchLink>; Department of Earth, Atmospheric and Planetary Sciences Massachusetts Institute of Technology Cambridge Massachusetts USA.<br /><searchLink fieldCode="AU" term="%22Le+Mouélic+S%22">Le Mouélic S</searchLink>; Laboratoire de Planétologie et Géodynamique, LPGNantes, CNRS UMR 6112, Université de Nantes Nantes France.<br /><searchLink fieldCode="AU" term="%22Kirk+RL%22">Kirk RL</searchLink>; United States Geological Survey, Astrogeology Science Center Flagstaff Arizona USA.<br /><searchLink fieldCode="AU" term="%22Stiles+BW%22">Stiles BW</searchLink>; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.<br /><searchLink fieldCode="AU" term="%22Malaska+MJ%22">Malaska MJ</searchLink>; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.<br /><searchLink fieldCode="AU" term="%22Le+Gall+A%22">Le Gall A</searchLink>; Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS) Université de Versailles Saint-Quentin Paris France.<br /><searchLink fieldCode="AU" term="%22Brown+RH%22">Brown RH</searchLink>; Lunar and Planetary Laboratory University of Arizona Tucson Arizona USA.<br /><searchLink fieldCode="AU" term="%22Baines+KH%22">Baines KH</searchLink>; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.<br /><searchLink fieldCode="AU" term="%22Buratti+B%22">Buratti B</searchLink>; Jet Propulsion Laboratory California Institute of Technology Pasadena California USA.<br /><searchLink fieldCode="AU" term="%22Clark+RN%22">Clark RN</searchLink>; United States Geological Survey Denver Colorado USA.<br /><searchLink fieldCode="AU" term="%22Nicholson+PD%22">Nicholson PD</searchLink>; Department of Astronomy Cornell University Ithaca New York USA.
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  Data: <searchLink fieldCode="JN" term="%229882887%22">Geophysical research letters</searchLink> [Geophys Res Lett] 2015 May 28; Vol. 42 (10), pp. 3746-3754. <i>Date of Electronic Publication: </i>2015 May 26.
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  Data: <i>Publisher: </i><searchLink fieldCode="PB" term="%22American+Geophysical+Union%22">American Geophysical Union </searchLink><i>Country of Publication: </i>United States <i>NLM ID: </i>9882887 <i>Publication Model: </i>Print-Electronic <i>Cited Medium: </i>Print <i>ISSN: </i>0094-8276 (Print) <i>Linking ISSN: </i><searchLink fieldCode="IS" term="%2200948276%22">00948276 </searchLink><i>NLM ISO Abbreviation: </i>Geophys Res Lett <i>Subsets: </i>PubMed not MEDLINE
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