Materials Map

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The Materials Map is an open tool for improving networking and interdisciplinary exchange within materials research. It enables cross-database search for cooperation and network partners and discovering of the research landscape.

The dashboard provides detailed information about the selected scientist, e.g. publications. The dashboard can be filtered and shows the relationship to co-authors in different diagrams. In addition, a link is provided to find contact information.

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The Materials Map is still under development. In its current state, it is only based on one single data source and, thus, incomplete and contains duplicates. We are working on incorporating new open data sources like ORCID to improve the quality and the timeliness of our data. We will update Materials Map as soon as possible and kindly ask for your patience.

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in Cooperation with on an Cooperation-Score of 37%

Topics

Publications (1/1 displayed)

  • 2020An orbital water-ice cycle on comet 67P from colour changes28citations

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Ciarniello, Mauro
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Raponi, Andrea
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Filacchione, Gianrico
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Mottola, Stefano
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De Sanctis, Maria Cristina
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2020

Co-Authors (by relevance)

  • Ciarniello, Mauro
  • Raponi, Andrea
  • Filacchione, Gianrico
  • Mottola, Stefano
  • De Sanctis, Maria Cristina
  • Formisano, Michelangelo
  • Mennella, Vito
  • Erard, Stèphane
  • Arnold, Gabriele
  • Capaccioni, Fabrizio
  • Longobardo, Andrea
  • Rinaldi, Giovanna
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article

An orbital water-ice cycle on comet 67P from colour changes

  • Ciarniello, Mauro
  • Raponi, Andrea
  • Filacchione, Gianrico
  • Mottola, Stefano
  • De Sanctis, Maria Cristina
  • Formisano, Michelangelo
  • Mennella, Vito
  • Erard, Stèphane
  • Arnold, Gabriele
  • Capaccioni, Fabrizio
  • Bockelèe-Morvan, Dominique
  • Longobardo, Andrea
  • Rinaldi, Giovanna
Abstract

Solar heating of a cometary surface provides the energy necessary to sustain gaseous activity, through which dust is removed<SUP>1,2</SUP>. In this dynamical environment, both the coma<SUP>3,4</SUP> and the nucleus<SUP>5,6</SUP> evolve during the orbit, changing their physical and compositional properties. The environment around an active nucleus is populated by dust grains with complex and variegated shapes<SUP>7</SUP>, lifted and diffused by gases freed from the sublimation of surface ices<SUP>8,9</SUP>. The visible colour of dust particles is highly variable: carbonaceous organic material-rich grains<SUP>10</SUP> appear red while magnesium silicate-rich<SUP>11,12</SUP> and water-ice-rich<SUP>13,14</SUP> grains appear blue, with some dependence on grain size distribution, viewing geometry, activity level and comet family type. We know that local colour changes are associated with grain size variations, such as in the bluer jets made of submicrometre grains on comet Hale-Bopp<SUP>15</SUP> or in the fragmented grains in the coma<SUP>16</SUP> of C/1999 S4 (LINEAR). Apart from grain size, composition also influences the coma's colour response, because transparent volatiles can introduce a substantial blueing in scattered light, as observed in the dust particles ejected after the collision of the Deep Impact probe with comet 9P/Tempel 1<SUP>17</SUP>. Here we report observations of two opposite seasonal colour cycles in the coma and on the surface of comet 67P/Churyumov-Gerasimenko through its perihelion passage<SUP>18</SUP>. Spectral analysis indicates an enrichment of submicrometre grains made of organic material and amorphous carbon in the coma, causing reddening during the passage. At the same time, the progressive removal of dust from the nucleus causes the exposure of more pristine and bluish icy layers on the surface. Far from the Sun, we find that the abundance of water ice on the nucleus is reduced owing to redeposition of dust and dehydration of the surface layer while the coma becomes less red....

Topics
  • impedance spectroscopy
  • surface
  • amorphous
  • Carbon
  • grain
  • grain size
  • Magnesium
  • Magnesium
  • laser emission spectroscopy
  • ion chromatography