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The Emergence of Life
Authors:Camprubí   E.  de Leeuw  J. W.  House  C. H.  Raulin  F.  Russell  M. J.  Spang  A.  Tirumalai  M. R.  Westall  F.
Affiliation:1.Physikalisches Institut, University of Bern, Sidlerstr. 5, 3012, Bern, Switzerland
;2.Deutsches Zentrum für Luft- und Raumfahrt (DLR), RB-MUSC, Linder H?he 1, 51147, Cologne, Germany
;3.Deutsches Zentrum für Luft- und Raumfahrt (DLR), Institut für Planetenforschung, Asteroiden und Kometen, Rutherfordstra?e 2, 12489, Berlin, Germany
;4.LATMOS/IPSL, UVSQ (Université Paris-Saclay), UPMC (Sorbonne Univ.), CNRS, 11, boulevard D’Alembert, 78280, Guyancourt, France
;5.Institut für Geophysik und extraterrestrische Physik, Technische Universit?t Braunschweig, Mendelssohnstr. 3, 38106, Braunschweig, Germany
;6.ESA-ESTEC, Keplerlaan 1, 2200 AG, Noordwijk, The Netherlands
;7.Planetary and Space Sciences, School of Physical Sciences, The Open University, Milton Keynes, MK7 6AA, UK
;8.Institute for Astronomy, Royal Observatory, University of Edinburgh, Edinburgh, EH9 3HJ, UK
;
Abstract:

The Rosetta observations have greatly advanced our knowledge of the cometary nucleus and its immediate environment. However, constraints on the mission (both planned and unplanned), the only partially successful Philae lander, and other instrumental issues have inevitably resulted in open questions. Surprising results from the many successful Rosetta observations have also opened new questions, unimagined when Rosetta was first planned. We discuss these and introduce several mission concepts that might address these issues. It is apparent that a sample return mission as originally conceived in the 1980s during the genesis of Rosetta would provide many answers but it is arguable whether it is technically feasible even with today’s technology and knowledge. Less ambitious mission concepts are described to address the suggested main outstanding scientific goals.

Keywords:
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