Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/26450
Titolo: | The Surface Composition and Thermal Properties of the Organic-Rich Surface of Comet 67P/Churyumov-Gerasimenko : VIRTIS/Rosetta Results (Invited) | Autori: | CAPACCIONI, FABRIZIO FILACCHIONE, GIANRICO Erard, S. Arnold, G. Drossart, P. DE SANCTIS, MARIA CRISTINA Bockelee-Morvan, D. CAPRIA, MARIA TERESA TOSI, Federico Leyrat, C. Schmitt, B. Quirico, E. CERRONI, PRISCILLA MENNELLA, Vito RAPONI, Andrea CIARNIELLO, Mauro Moroz, L. PALOMBA, Ernesto |
Data pubblicazione: | 2015 | Titolo del volume in cui è pubblicato il poster: | AOGS 12th Annual Meeting | Da pagina:: | PS02-D2-PM2-324-007 | Abstract: | The paper will describe the major results obtained by the instrument VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer), the dual channel spectrometer onboard Rosetta, on the surface composition and thermal properties of the nucleus of comet 67P/Churyumov-Gerasimenko. <P />VIRTIS is a dual channel spectrometer; VIRTIS-M (M for Mapper) is a hyper spectral imager covering a wide spectral range from 0.25 through 5μm. VIRTIS-M uses a slit and a scan mirror to generate images with spatial resolution of 250 μrad over a FOV of 3.7°. The second channel is VIRTIS-H (H for High-resolution), a point spectrometer with high spectral resolution (λ/∆λ=3000 @3μm) in the range 2-5 μm. The nucleus observations are performed in a wide range of conditions with spatial resolution varying from the initial 500m down to 2.5m. The surface temperature has been determined since the first distant observations when the nucleus filled one single VIRTIS-M pixel. On the mid of July 2014 from a distance of 15000km the mean surface temperature has been measured as 205±5K. This pointed to a surface structure largely covered by a porous crust, mainly devoid of water ice. Maximum temperature determined so far are as high as 230K on the subsolar point. The VIRTIS composition analysis has showed 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 μm), the spectral slopes in VIS and IR ranges (5-25 and 1.5-5 % kÅ-1) and the broad absorption feature in the 2.9-3.6 µm 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 C-H and/or O-H chemical groups, with little contribution of N-H. Authors acknowledge the support from national funding agencies. | Titolo del convegno: | AOGS 12th Annual Meeting | Luogo del convegno: | Singapore | Periodo del convegno: | 2-7 August, 2015 | URI: | http://hdl.handle.net/20.500.12386/26450 | URL: | https://www.meetmatt-svr3.net/aogs/aogs2015/mars2/pubViewAbs.asp?sMode=session&sId=3&submit=Browse+Abstracts https://www.asiaoceania.org/aogs2015/public.asp?page=home.htm |
Bibcode ADS: | 2015aogs.confE...3C | Fulltext: | open |
È visualizzato nelle collezioni: | 3.02 Abstract in Atti di convegno |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
AOGS 2015.pdf | 177.66 kB | Adobe PDF | Visualizza/apri | |
PS02-D2-PM2-324-007AOGS 2015.pdf | Abstract | 108.65 kB | Adobe PDF | Visualizza/apri |
Page view(s)
108
controllato il 11-set-2024
Download(s)
42
controllato il 11-set-2024
Google ScholarTM
Check
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.