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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Dotto, Elisabetta
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Topics
Publications (6/6 displayed)
- 2021Influence of the body composition on the evolution of ejecta in the Didymos-Dimorphos binary system
- 2018Rotationally resolved spectroscopy of Jupiter Trojans (624) Hektor and (911) Agamemnoncitations
- 2006Methanol Detection on the Surface of the TNO (55638) 2002 VE95
- 2004Heterogeneity/homogeneity on the TNO and Centaur surfaces
- 2003Unveiling the nature of 10199 Chariklo: near-infrared observations and modelingcitations
- 2002A portrait of the Centaur 10199 Chariklo
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document
A portrait of the Centaur 10199 Chariklo
Abstract
10199 Chariklo is the largest Centaur so far known. To investigate its surface composition and possible surface variations, spectroscopic observations have been carried out at the largest available telescopes. We obtained near-infrared spectra at ESO-VLT (Cerro Paranal, Chile) and TNG (La Palma, Spain) on April 2001 and March 2002, respectively. Considering all the available data from 0.38 micron to 2.45 micron we modeled the surface composition using geographical mixtures of different materials. A tentative model, composed by a mixture of amorphous carbon, titan tholins, olivines and some percentage of water ice, will be presented and discussed....