English

Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer

Earth and Planetary Astrophysics 2023-10-27 v4 Instrumentation and Methods for Astrophysics

Abstract

ESA's Jupiter Icy Moons Explorer (JUICE) will provide a detailed investigation of the Jovian system in the 2030s, combining a suite of state-of-the-art instruments with an orbital tour tailored to maximise observing opportunities. We review the Jupiter science enabled by the JUICE mission, building on the legacy of discoveries from the Galileo, Cassini, and Juno missions, alongside ground- and space-based observatories. We focus on remote sensing of the climate, meteorology, and chemistry of the atmosphere and auroras from the cloud-forming weather layer, through the upper troposphere, into the stratosphere and ionosphere. The Jupiter orbital tour provides a wealth of opportunities for atmospheric and auroral science: global perspectives with its near-equatorial and inclined phases, sampling all phase angles from dayside to nightside, and investigating phenomena evolving on timescales from minutes to months. The remote sensing payload spans far-UV spectroscopy (50-210 nm), visible imaging (340-1080 nm), visible/near-infrared spectroscopy (0.49-5.56 μ\mum), and sub-millimetre sounding (near 530-625\,GHz and 1067-1275\,GHz). This is coupled to radio, stellar, and solar occultation opportunities to explore the atmosphere at high vertical resolution; and radio and plasma wave measurements of electric discharges in the Jovian atmosphere and auroras. Cross-disciplinary scientific investigations enable JUICE to explore coupling processes in giant planet atmospheres, to show how the atmosphere is connected to (i) the deep circulation and composition of the hydrogen-dominated interior; and (ii) to the currents and charged particle environments of the external magnetosphere. JUICE will provide a comprehensive characterisation of the atmosphere and auroras of this archetypal giant planet.

Keywords

Cite

@article{arxiv.2304.10229,
  title  = {Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer},
  author = {Leigh N. Fletcher and Thibault Cavalié and Davide Grassi and Ricardo Hueso and Luisa M. Lara and Yohai Kaspi and Eli Galanti and Thomas K. Greathouse and Philippa M. Molyneux and Marina Galand and Claire Vallat and Olivier Witasse and Rosario Lorente and Paul Hartogh and François Poulet and Yves Langevin and Pasquale Palumbo and G. Randall Gladstone and Kurt D. Retherford and Michele K. Dougherty and Jan-Erik Wahlund and Stas Barabash and Luciano Iess and Lorenzo Bruzzone and Hauke Hussmann and Leonid I. Gurvits and Ondřej Santolik and Ivana Kolmasova and Georg Fischer and Ingo Müller-Wodarg and Giuseppe Piccioni and Thierry Fouchet and Jean-Claude Gérard and Agustin Sánchez-Lavega and Patrick G. J. Irwin and Denis Grodent and Francesca Altieri and Alessandro Mura and Pierre Drossart and Josh Kammer and Rohini Giles and Stéphanie Cazaux and Geraint Jones and Maria Smirnova and Emmanuel Lellouch and Alexander S. Medvedev and Raphael Moreno and Ladislav Rezac and Athena Coustenis and Marc Costa},
  journal= {arXiv preprint arXiv:2304.10229},
  year   = {2023}
}

Comments

83 pages, 24 figures, accepted to Space Science Reviews special issue on ESA's JUICE mission

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