ENCELADUS AS A POTENTIAL OASIS FOR LIFE: Science goals and investigations for future explorations A White paper submitted to ESA’S Voyage 2050 call Contact person: Gaël Choblet Address: Laboratoire de Planétologie et Géodynamique, UMR-CNRS 6112, Nantes Université 2, rue de la Houssinière, 44322 Nantes cedex, France Email: gaë
[email protected]; phone: +33 2 76 64 51 55 ENCELADUS AS A POTENTIAL OASIS FOR LIFE Core proposing team Gaël Choblet Arnaud Buch LPG, Univ. Nantes/CNRS, France CentraleSupélec, France Ondrej Cadek Eloi Camprubi-Casas Charles Univ. Prague, Czech Rep. Utrecht University, Netherlands Caroline Freissinet Matt Hedman LATMOS, UVSQ/CNRS, France University of Idaho, USA Geraint Jones Valery Lainey Mullard Space Science Lab, UK Obs. Paris, France Alice Le Gall Alice Lucchetti LATMOS, UVSQ/CNRS, France INAF-OAPD, Italy Shannon MacKenzie Giuseppe Mitri JHU-APL, USA IRSPS InGeo Univ. d’Annunzio, Italy Marc Neveu Francis Nimmo NASA Goddard Space Flight Ctr., USA University of California Santa Cruz, USA Karen Olsson-Francis Mark Panning Open University, UK JPL-Caltech, USA Joachim Saur Frank Postberg Univ. Köln, Germany Frei Univ. Berlin, Germany Jürgen Schmidt Takazo Shibuya Oulu University, Finland JAMSTEC, Japan Yasuhito Sekine Christophe Sotin ELSI, Japan JPL-Caltech, USA Gabriel Tobie Ondrej Soucek LPG, Univ. Nantes/CNRS, France Charles Univ. Prague, Czech Rep. Steve Vance Cyril Szopa JPL-Caltech, USA LATMOS, UVSQ/CNRS, France Laurie Barge Usui Tomohiro JPL-Caltech, USA ISAS/JAXA, Japan Marie Behounkova Tim Van Hoolst Charles Univ. Prague, Czech Rep. Royal Observatory, Belgium ENCELADUS AS A POTENTIAL OASIS FOR LIFE EXECUTIVE SUMMARY: Enceladus is the first planetary object for which direct sampling of a subsurface water reservoir, likely habitable, has been performed.