<p>The <i>Jupiter and Icy Moons Explorer</i> (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.</p>

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Io and the Minor Jovian Moons – Prospects for JUICE

  • Tilmann Denk,
  • David A. Williams,
  • Federico Tosi,
  • James F. Bell III,
  • Stefano Mottola,
  • Imke de Pater,
  • Valéry Lainey,
  • Philippa Molyneux,
  • Klaus-Dieter Matz,
  • Paul Hartogh,
  • Rosaly M. Lopes,
  • Anezina Solomonidou,
  • Peter C. Thomas,
  • Hans Leo F. Huybrighs,
  • Leonid I. Gurvits,
  • Alessandro Mura,
  • Kurt D. Retherford,
  • Ladislav Rezac,
  • Thomas Roatsch,
  • Lorenz Roth,
  • Nico Haslebacher,
  • Cecilia Tubiana,
  • Alice Lucchetti,
  • Yves Langevin,
  • François Poulet,
  • Emmanuel Lellouch,
  • Fuminori Tsuchiya,
  • Claire Vallat,
  • Tim Van Hoolst,
  • Audrey Vorburger,
  • Peter Wurz,
  • Emiliano D’Aversa,
  • Randy Gladstone,
  • Thomas Greathouse,
  • Nicholas Schneider,
  • Francesca Zambon,
  • Nicolas Altobelli,
  • Pasquale Palumbo,
  • Ganna Portyankina,
  • Oded Aharonson,
  • Lorenzo Bruzzone,
  • John Carter,
  • Baptiste Cecconi,
  • Nick Cooper,
  • Marc Costa Sitjà,
  • Alfredo Escalante López,
  • Yoshifumi Futaana,
  • Elena Mazzotta Epifani,
  • Alessandra Migliorini,
  • William B. Moore,
  • Raphael Moreno,
  • Carl Murray,
  • Luca Penasa,
  • Giuseppe Piccioni,
  • Jürgen Schmidt,
  • Jan-Erik Wahlund,
  • Olivier Witasse

摘要

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.