| Autor: |
Blecka, M., Capaccioni, F., Filacchione, G., Raponi, A., Ciarnello, M., Arnold, Gabriele, De Sanctis, M.C., Erard, S., Bockelee-Morvan, D., Tosi, F., Capria, M. T., Piccioni, G., Palomba, E., Fonti, S., Longobardo, A, Drossart, P., Schmitt, B., Quirico, E., Rinaldi, G., Wawrzaszek, A. |
| Jazyk: |
angličtina |
| Rok vydání: |
2015 |
| Předmět: |
|
| Popis: |
The main subject of the paper is constraining the composition of the surface and possibly of the dust on the comet 67P/Churyumov-Gerasimenko by means of comparison between the data from the VIRTIS instrument onboard Rosetta and adopted model of the surface of asteroids [9]. As a first step we have taken into account the spectral range 2.0 - 4.0 μm. For our calculations Mie and Hapke’s models have been considered. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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