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Communication Dans Un Congrès Année : 2015

Highlights of early VIRTIS/ROSETTA observations: 67P/Churyumov-Gerasimenko seen from orbit

Résumé

VIRTIS is the imaging spectrometer of the Rosetta mission, devoted to remote sensing studies of comet 67P/Churyumov-Gerasimenko (1). The instrument is made of a mapping channel covering the 0.3-5 mum range at moderate spectral resolution (VIRTIS-M), and of a cross-dispersion spectrometer covering the 2-5um range with resolution ~3000 (VIRTIS-H). The most recent results will be presented at the meeting; early ones are discussed here.The nucleus is observed from a wide range of illumination conditions and spatial resolution (down to 2.5 m). Albedo, spectral parameters, and compositional maps have been derived for areas out of the polar night. The nucleus surface appears to be extremely homogeneous and dark. The inferred normal albedo is 0.060 ± 0.003 at 0.55 mum (2), with distinct spectral slopes in the VIS and IR regions (5-25 and 1.5-5 % kÅ-1 respectively). The main spectral feature is a ubiquitous absorption in the 2.9-3.6 mum range, consistent with non-volatile organic macromolecular materials (2,3). The most likely absorbents include carboxylic groups, alcoholic OH, and possibly NH4 ions. However, the low albedo and marked slope suggest a mixture with opaque minerals (e.g. sulfides) or Fe-Ni alloys in the refractory crust. Ice is so far marginally detected in areas just emerging from shadow (4).The surface temperature is measured on the dayside as a function of local time and heliocentric distance. A maximum of 220K has been derived, with fast variations controlled by low thermal inertia. This is consistent with a surface covered by a porous crust, mainly devoid of water ice (5,6).Water vapor and carbon dioxide have been observed in the coma and their variability with altitude, geographic location and heliocentric distance has been studied. CO2/H2O ratio averages to 3-7%, but both species display different distributions. This suggests either different source regions, or seasonal variability (7).1- Coradini et al, SSR, 20072- Capaccioni et al., Science, 20153- Quirico et al, LPSC 20154- De Sanctis et al, LPSC 20155- Tosi et al, LPSC 20156- Leyrat et al, EGU 20157- Bockelée-Morvan et al, this meeting
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hal-03733694 , version 1 (21-07-2022)

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Stéphane Erard, Fabrizio Capaccioni, Gianrico Filacchione, Gabriele Arnold, Dominique Bockelée-Morvan, et al.. Highlights of early VIRTIS/ROSETTA observations: 67P/Churyumov-Gerasimenko seen from orbit. IAU General Assembly XXIX, Meeting #29, #2254766, Aug 2015, Honolulu, Hawaii, United States. ⟨hal-03733694⟩
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