| People | Locations | Statistics |
|---|---|---|
| Naji, M. |
| |
| Motta, Antonella |
| |
| Aletan, Dirar |
| |
| Mohamed, Tarek |
| |
| Ertürk, Emre |
| |
| Taccardi, Nicola |
| |
| Kononenko, Denys |
| |
| Petrov, R. H. | Madrid |
|
| Alshaaer, Mazen | Brussels |
|
| Bih, L. |
| |
| Casati, R. |
| |
| Muller, Hermance |
| |
| Kočí, Jan | Prague |
|
| Šuljagić, Marija |
| |
| Kalteremidou, Kalliopi-Artemi | Brussels |
|
| Azam, Siraj |
| |
| Ospanova, Alyiya |
| |
| Blanpain, Bart |
| |
| Ali, M. A. |
| |
| Popa, V. |
| |
| Rančić, M. |
| |
| Ollier, Nadège |
| |
| Azevedo, Nuno Monteiro |
| |
| Landes, Michael |
| |
| Rignanese, Gian-Marco |
|
Zine, Sonia
Université Grenoble Alpes
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (10/10 displayed)
- 2018CONSERT probing of 67P/C-G nucleus during the ROSETTA mission, operations and results
- 2017 Interior of 67P/C-G comet as seen by CONSERT bistatic radar on Rosetta
- 2016Cosmochemical implications of CONSERT permittivity characterization of 67P/CG
- 2016Mineralogical implications of Consert permittivity characterization of 67P.
- 2016Cosmochemical implications of CONSERT permittivity characterization of 67P/C-G
- 2016Cosmochemical implications of CONSERT permittivity characterization of 67P/C-G
- 2016Mineralogical Implications of CONSERT Permittivity Characterization of 67P
- 2015Insights gained from Data Measured by the CONSERT Instrument during Philae's Descent onto 67P/C-G's surface
- 2015Properties of the 67P/Churyumov-Gerasimenko interior revealed by CONSERT radarcitations
- 2015The CONSERT Instrument during Philae's Descent onto 67P/C-G’s surface: Insights on Philae’s Attitude and the Surface Permittivity Measurements at the Agilkia-Landing-Site
Places of action
| Organizations | Location | People |
|---|
document
Mineralogical Implications of CONSERT Permittivity Characterization of 67P
Abstract
On 12 November 2014, after the descent and rebounds of the lander Philae, COmet Nucleus Sounding Experiment by Radio Transmission (CONSERT) restarted operating at 18h56 UTC and continued until 04h06 UTC, providing the first investigation of the internal structure of the nucleus of a comet. The analysis of the signal that propagated throughout the upper part of “head” of 67P allows us to estimate an average permittivity of approximately 1.27 (Kofman et al., 2015). This average permittivity induces constraints on the permittivity of the dust components versus volume fraction of dust and ices. We analyze constraints on dust permittivity using mixing formulas and ice composition models. Additional comparisons to laboratory measurements will allow us to discuss the implication on composition and mineralogy of the 67P dust particules.