a1 Department of Chemistry and Biochemistry, LMU, Butenandtstrasse 5–13, 81377 Munich, Germany
a2 Physikalisches Institut, Space Research & Planetary Sciences, Siedlerstr. 5, 3012 Bern, Switzerland
a3 CNRS, Université de Nantes, Laboratoire de Planétologie et Géodynamique, UMR 6112, 2 rue de la Houssinière, Nantes, F-44000, France
a4 Institute for Astronomy, University of Vienna, Tuerkenschanzstr. 17, A-1180 Vienna, Austria
a5 Microbial Oceanography Research Centre, Department of Microbiology, School of Natural Sciences, National University of Ireland, Galway, Ireland
a6 Department of Astronomy, Stockholm University, AlbaNova University Center, Roslagstullsbacken 21, SE-106 91 Stockholm, Sweden
a7 Centre for Environmental Biology, Animal Biology Department, Faculdade de Ciências of the Universidade de Lisboa, Edifício C2, 5° piso, Campo Grande, 1749-016, Lisboa, Portugal
a8 IN+, Center for Innovation, Technology and Policy Research, Environment and Energy Scientific Area, Mechanical Engineering Department, Instituto Superior Técnico, Av. Rovisco Pais, 1, 1049-001, Lisboa, Portugal
a9 Faculty of Medicine, Autonomous University of Barcelona, Edifici M, Campus UAB. 08193 Bellaterra, Spain
a10 Planetary and Space Sciences Research Institute, The Open University, Walton Hall, Milton Keynes, UK
a11 Department of Chemistry, University of Leicester, University Road, Leicester, UK
a12 Institut de Physique de Rennes, Université de Rennes, Astrochimie expérimentale, Campus de Beaulieu, 35000 Rennes, France
a13 TU Dresden, Helmholtzstraße 10, 01069 Dresden, Germany
a14 Dipartimento di Astronomia e Scienza dello Spazio, Università di Firenze, Largo Enrico Fermi 2, 50125, Firenze, Italy
a15 Xiamen University, 361005 Fujian Province, China
a16 Université de Bordeaux, Laboratoire d'Astrophysique de Bordeaux (LAB), CNRS/INSU, UMR 5804, 33271 Floirac, France
a17 Institute of Communication Networks and Satellite Communications, Graz University of Technology, Inffeldgasse 12, 8010 Graz, Austria
Abstract
The HADES Europa mission concept aims to provide a framework for an astrobiological in-depth investigation of the Jupiter moon Europa, relying on existing technologies and feasibility. This mission study proposes a system consisting of an orbiter, lander and cryobot as a platform for detailed exploration of Europa. While the orbiter will investigate the presence of a liquid ocean and characterize Europa's internal structure, the lander will survey local dynamics of the ice layer and the surface environment. The lander releases a cryobot, that melts into the ice, will sample the pristine subsurface and is expected to provide data on organic and gaseous content and putative bio-signatures. In summary, we present the scientific objectives for an astrobiological investigation of Europa, resulting in a mission concept with a detailed evaluation of scientific instrumentation, mission sequences, basic design of the spacecraft, technology needs and cost estimations.
(Received July 20 2009)
(Accepted July 21 2009)
(Online publication August 26 2009)
Key Words:
Correspondence:
c1 e-mail: lucille.le-corre@univ-nantes.fr
Footnotes
# The authors contributed equally to the paper.