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Science goals and new mission concepts for future exploration of Titan’s atmosphere, geology and habitability: titan POlar scout/orbitEr and in situ lake lander and DrONe explorer (POSEIDON)

  • Sébastien Rodriguez
  • , Sandrine Vinatier
  • , Daniel Cordier
  • , Gabriel Tobie
  • , Richard K. Achterberg
  • , Carrie M. Anderson
  • , Sarah V. Badman
  • , Jason W. Barnes
  • , Erika L. Barth
  • , Bruno Bézard
  • , Nathalie Carrasco
  • , Benjamin Charnay
  • , Roger N. Clark
  • , Patrice Coll
  • , Thomas Cornet
  • , Athena Coustenis
  • , Isabelle Couturier-Tamburelli
  • , Michel Dobrijevic
  • , F. Michael Flasar
  • , Remco de Kok
  • Caroline Freissinet, Marina Galand, Thomas Gautier, Wolf D. Geppert, Caitlin A. Griffith, Murthy S. Gudipati, Lina Z. Hadid, Alexander G. Hayes, Amanda R. Hendrix, Ralf Jaumann, Donald E. Jennings, Antoine Jolly, Klara Kalousova, Tommi T. Koskinen, Panayotis Lavvas, Sébastien Lebonnois, Jean Pierre Lebreton, Alice Le Gall, Emmanuel Lellouch, Stéphane Le Mouélic, Rosaly M.C. Lopes, Juan M. Lora, Ralph D. Lorenz, Antoine Lucas, Shannon MacKenzie, Michael J. Malaska, Kathleen Mandt, Marco Mastrogiuseppe, Claire E. Newman, Conor A. Nixon, Jani Radebaugh, Scot C. Rafkin, Pascal Rannou, Ella M. Sciamma-O’Brien, Jason M. Soderblom, Anezina Solomonidou, Christophe Sotin, Katrin Stephan, Darrell Strobel, Cyril Szopa, Nicholas A. Teanby, Elizabeth P. Turtle, Véronique Vuitton, Robert A. West
  • Université Paris Diderot
  • Sorbonne Univ.
  • Univ. de Reims Champagne Ardenne
  • Université de Nantes
  • University of Maryland
  • NASA Goddard Space Flight Center
  • University of Leicester
  • University of Idaho
  • Southwest Research Institute
  • Université Paris-Saclay
  • Planetary Science Institute
  • Université de PARIS XII
  • European Space Agency
  • Aix-Marseille Université
  • Laboratoire d'Astrophysique de Bordeaux
  • Universiteit Utrecht
  • Imperial College London
  • AlbaNova University Center
  • University of Arizona
  • Science Division
  • Sorbonne Université
  • Cornell University
  • Free University of Berlin
  • Charles University
  • conventionnée avec l'Université d'Orléans
  • Yale University
  • Johns Hopkins University Applied Physics Laboratory
  • University of Rome
  • Aeolis Research
  • Brigham Young University
  • NASA Ames Research Center
  • Massachusetts Institute of Technology
  • California Institute of Technology
  • DLR
  • Johns Hopkins University
  • University of Bristol
  • Université Grenoble Alpes

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

In response to ESA’s “Voyage 2050” announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn’s largest moon Titan. Titan, a “world with two oceans”, is an organic-rich body with interior-surface-atmosphere interactions that are comparable in complexity to the Earth. Titan is also one of the few places in the Solar System with habitability potential. Titan’s remarkable nature was only partly revealed by the Cassini-Huygens mission and still holds mysteries requiring a complete exploration using a variety of vehicles and instruments. The proposed mission concept POSEIDON (Titan POlar Scout/orbitEr and In situ lake lander DrONe explorer) would perform joint orbital and in situ investigations of Titan. It is designed to build on and exceed the scope and scientific/technological accomplishments of Cassini-Huygens, exploring Titan in ways that were not previously possible, in particular through full close-up and in situ coverage over long periods of time. In the proposed mission architecture, POSEIDON consists of two major elements: a spacecraft with a large set of instruments that would orbit Titan, preferably in a low-eccentricity polar orbit, and a suite of in situ investigation components, i.e. a lake lander, a “heavy” drone (possibly amphibious) and/or a fleet of mini-drones, dedicated to the exploration of the polar regions. The ideal arrival time at Titan would be slightly before the next northern Spring equinox (2039), as equinoxes are the most active periods to monitor still largely unknown atmospheric and surface seasonal changes. The exploration of Titan’s northern latitudes with an orbiter and in situ element(s) would be highly complementary in terms of timing (with possible mission timing overlap), locations, and science goals with the upcoming NASA New Frontiers Dragonfly mission that will provide in situ exploration of Titan’s equatorial regions, in the mid-2030s.

langue originaleAnglais
Pages (de - à)911-973
Nombre de pages63
journalExperimental Astronomy
Volume54
Numéro de publication2-3
Les DOIs
étatPublié - 1 déc. 2022

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