Preliminary estimation of the detection possibilities of Ganymede's water vapor environment with MAJIS. (15th October 2020)

• Record Type: Journal Article
• Authors: Plainaki, Christina; Sindoni, Giuseppe; Grassi, Davide; Cafarelli, Luigi; D'Aversa, Emiliano; Massetti, Stefano; Mura, Alessandro; Milillo, Anna; Filacchione, Gianrico; Piccioni, Giuseppe; Langevin, Yves; Poulet, Francois; Tosi, Federico; Migliorini, Alessandra; Altieri, Francesca
• Is Part Of: Planetary and space science. Volume 191(2020)
• Publication Date: 2020-10-15
• Subjects: Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2020.105004
• Languages: English
• ISSNs: 0032-0633

Abstract

Abstract: The exosphere of Ganymede is the interface region linking the moon's icy surface to Jupiter's magnetospheric environment. Its characterization is of key importance to achieve a full understanding of the ice alteration processes induced by the radiation environment. Several scientific instruments that will operate on board the upcoming Jupiter Icy Moons Explorer (JUICE) mission, selected by ESA in the context of its Cosmic Vision programme, have the potential to study Ganymede's exosphere. Among them, the Moons And Jupiter Imaging Spectrometer (MAJIS) will have the chance to investigate the composition of the moon's exospheric components and the emission of water molecules. The exospheric water density profile, as obtained from current models, is a crucial parameter for the estimation of the expected signal to noise ratio related to the actual measurement. In lack of an adequate number of Ganymede's observations from past missions, there is a general difficulty in constraining current exosphere models which are based, in general, on different scenarios and considerations and often show large discrepancies in the estimated spatial distribution of the neutral environment. In this work, we make a preliminary estimation of the expected IR emission from exospheric water molecules, using different modelled density profiles, and we speculate on the possibility of JUICE/MAJIS to detect it. An exercise on the potential plume detection capabilities of MAJIS is also performed. The first necessary step for performing these calculations is a rough comparison of the existing models of Ganymede's water vapor exosphere. We discuss the characteristics of the neutral environment as derived from different exospheric models available in literature, the role of the ion-surface interactions in the H2 O exosphere generation, and the related implications also in view of future observations. We then use the model outputs to estimate different scenarios for the expected non-Local Thermal Equilibrium (non-LTE) emission from these molecules. The results of this study can be of help during the JUICE observation planning phase. Highlights: JUICE/MAJIS has the necessary sensitivity to observe Ganymede's water exosphere. Current estimations provide a lower limit for future exosphere detection. Exosphere investigations with JUICE are important for speculating on weathering. JUICE will provide proof of the most realistic exosphere generation scenario.