Deciphering surface properties of the Jovian moons using radiative transfer modelling and NIR data

Guillaume Cruz Mermy; Frédéric Schmidt; François Andrieu; Thomas Cornet; Inès Belgacem

doi:https://doi.org/10.5194/egusphere-egu26-19686

[Back] [Session PS2.6]

EGU26-19686, updated on 14 Mar 2026

https://doi.org/10.5194/egusphere-egu26-19686

EGU General Assembly 2026

© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.

Deciphering surface properties of the Jovian moons using radiative transfer modelling and NIR data

Guillaume Cruz Mermy¹, Frédéric Schmidt², François Andrieu², Thomas Cornet¹, and Inès Belgacem¹

Guillaume Cruz Mermy et al.

¹European Space Agency (ESA), European Space Astronomy Centre (ESAC), Villanueva de la Cañada, Spain (guillaume.cruz-mermy@universite-paris-saclay.fr)
²Université Paris-Saclay, CNRS, GEOPS, 91405, Orsay, France

How to cite: Cruz Mermy, G., Schmidt, F., Andrieu, F., Cornet, T., and Belgacem, I.: Deciphering surface properties of the Jovian moons using radiative transfer modelling and NIR data, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19686, https://doi.org/10.5194/egusphere-egu26-19686, 2026.

This abstract has been withdrawn on 31 Mar 2026.