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Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
by
Colangeli, L
, Federico, C
, Leyrat, C
, Markus, K
, Barucci, M A
, Henry, F
, Combe, J-Ph
, Erard, S
, Politi, R
, Peter, G
, Filacchione, G
, Encrenaz, T
, Blanco, A
, Cartacci, M
, Longobardo, A
, Cicchetti, A
, Taylor, F
, Despan, D
, Magni, G
, Rinaldi, G
, Tozzi, G P
, Frigeri, A
, Jacquinod, S
, Langevin, Y
, Mennella, V
, McCord, T
, Ip, W H
, Beck, P
, Combi, M
, Jaumann, R
, Ciarniello, M
, Schmitt, B
, Semery, A
, Benkhoff, J
, Orofino, V
, De Sanctis, M C
, Piccioni, G
, Giuppi, S
, Blecka, M
, Bellucci, G
, Flamini, E
, Orosei, R
, Bockelee-Morvan, D
, Palumbo, P
, Tiphene, D
, Irwin, P
, Drossart, P
, Crovisier, J
, Ammannito, E
, Bonal, L
, Arnold, G
, Cerroni, P
, Mottola, S
, Carlson, R
, Capria, M T
, Carsenty, U
, Fink, U
, Grassi, D
, Bibring, J P
, Merlin, F
, Noschese, R
, Biver, N
, Fornasier, S
, Gudipati, M
, Hello, Y
, Coradini, A
, Stephan, K
, Fonti, S
, Quirico, E
, Reess, J M
, Schade, U
, Moroz, L
, Tosi, F
, Raponi, A
, Combes, M
, Capaccioni, F
, Kuehrt, E
, Palomba, E
2015
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Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
by
Colangeli, L
, Federico, C
, Leyrat, C
, Markus, K
, Barucci, M A
, Henry, F
, Combe, J-Ph
, Erard, S
, Politi, R
, Peter, G
, Filacchione, G
, Encrenaz, T
, Blanco, A
, Cartacci, M
, Longobardo, A
, Cicchetti, A
, Taylor, F
, Despan, D
, Magni, G
, Rinaldi, G
, Tozzi, G P
, Frigeri, A
, Jacquinod, S
, Langevin, Y
, Mennella, V
, McCord, T
, Ip, W H
, Beck, P
, Combi, M
, Jaumann, R
, Ciarniello, M
, Schmitt, B
, Semery, A
, Benkhoff, J
, Orofino, V
, De Sanctis, M C
, Piccioni, G
, Giuppi, S
, Blecka, M
, Bellucci, G
, Flamini, E
, Orosei, R
, Bockelee-Morvan, D
, Palumbo, P
, Tiphene, D
, Irwin, P
, Drossart, P
, Crovisier, J
, Ammannito, E
, Bonal, L
, Arnold, G
, Cerroni, P
, Mottola, S
, Carlson, R
, Capria, M T
, Carsenty, U
, Fink, U
, Grassi, D
, Bibring, J P
, Merlin, F
, Noschese, R
, Biver, N
, Fornasier, S
, Gudipati, M
, Hello, Y
, Coradini, A
, Stephan, K
, Fonti, S
, Quirico, E
, Reess, J M
, Schade, U
, Moroz, L
, Tosi, F
, Raponi, A
, Combes, M
, Capaccioni, F
, Kuehrt, E
, Palomba, E
in
2015
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Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
by
Colangeli, L
, Federico, C
, Leyrat, C
, Markus, K
, Barucci, M A
, Henry, F
, Combe, J-Ph
, Erard, S
, Politi, R
, Peter, G
, Filacchione, G
, Encrenaz, T
, Blanco, A
, Cartacci, M
, Longobardo, A
, Cicchetti, A
, Taylor, F
, Despan, D
, Magni, G
, Rinaldi, G
, Tozzi, G P
, Frigeri, A
, Jacquinod, S
, Langevin, Y
, Mennella, V
, McCord, T
, Ip, W H
, Beck, P
, Combi, M
, Jaumann, R
, Ciarniello, M
, Schmitt, B
, Semery, A
, Benkhoff, J
, Orofino, V
, De Sanctis, M C
, Piccioni, G
, Giuppi, S
, Blecka, M
, Bellucci, G
, Flamini, E
, Orosei, R
, Bockelee-Morvan, D
, Palumbo, P
, Tiphene, D
, Irwin, P
, Drossart, P
, Crovisier, J
, Ammannito, E
, Bonal, L
, Arnold, G
, Cerroni, P
, Mottola, S
, Carlson, R
, Capria, M T
, Carsenty, U
, Fink, U
, Grassi, D
, Bibring, J P
, Merlin, F
, Noschese, R
, Biver, N
, Fornasier, S
, Gudipati, M
, Hello, Y
, Coradini, A
, Stephan, K
, Fonti, S
, Quirico, E
, Reess, J M
, Schade, U
, Moroz, L
, Tosi, F
, Raponi, A
, Combes, M
, Capaccioni, F
, Kuehrt, E
, Palomba, E
2015
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Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
Journal Article
Cometary science. The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta
2015
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Overview
The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument on board the Rosetta spacecraft has provided evidence of carbon-bearing compounds on the nucleus of the comet 67P/Churyumov-Gerasimenko. The very low reflectance of the nucleus (normal albedo of 0.060 ± 0.003 at 0.55 micrometers), the spectral slopes in visible and infrared ranges (5 to 25 and 1.5 to 5% kÅ(-1)), and the broad absorption feature in the 2.9-to-3.6-micrometer range present across the entire illuminated surface are compatible with opaque minerals associated with nonvolatile organic macromolecular materials: a complex mixture of various types of carbon-hydrogen and/or oxygen-hydrogen chemical groups, with little contribution of nitrogen-hydrogen groups. In active areas, the changes in spectral slope and absorption feature width may suggest small amounts of water-ice. However, no ice-rich patches are observed, indicating a generally dehydrated nature for the surface currently illuminated by the Sun.
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