Io and the Minor Jovian Moons – Prospects for JUICE
Tilmann Denk (Deutsches Zentrum für Luft- und Raumfahrt (DLR))
David A. Williams (School of Earth and Space Exploration)
Federico Tosi (Radio Observatory Medicina)
James F. Bell (School of Earth and Space Exploration)
Stefano Mottola (Deutsches Zentrum für Luft- und Raumfahrt (DLR))
Imke de Pater (TU Delft - Astrodynamics & Space Missions, University of California)
Valéry Lainey (Observatoire de Paris)
Philippa Molyneux (Southwest Research Institute)
Leonid I. Gurvits (TU Delft - Astrodynamics & Space Missions, Joint Institute for VLBI ERIC)
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Abstract
The Jupiter and Icy Moons Explorer (JUICE) mission of the European Space Agency (ESA) will investigate the Jovian system with multiple instruments over several years, beginning in early 2031. This paper describes the historical context and state of knowledge, as well as JUICE’s scientific goals and measurement techniques of the satellites that will not be encountered in close flybys. These include the large volcanically active moon Io, the four small inner moons Metis, Adrastea, Amalthea, and Thebe, and the numerous small Irregular (outer) moons. JUICE will provide multiple opportunities to observe Io from relatively remote distances of hundreds of thousands of kilometers. These observations will enable monitoring of Io’s surface for changes, and for the study of its neutral clouds and plasma torus. Io observations will be performed with the four optical remote sensing instruments and with the Particle Environment Package. For the small inner moons it is planned to obtain complete geographic longitude (scales up to 8 km/px), solar-phase and multi-color coverage, oblique polar views, and UV to near-IR spectra. Astrometric measurements will also be performed. The Irregular moons will mostly appear unresolved to the JUICE instruments. Nonetheless, long-duration disk-integrated lightcurves will be acquired to derive rotation periods, object dimensions, pole-axis orientations, and colors for most objects for the first time. From these data, convex-shape models will be generated and phase curves determined. Furthermore, the precision of the orbital elements will be improved via accurate astrometry. UV and near-IR measurements will be attempted for the largest of these objects.
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