The Philae lander mission and science overview

Author:

Boehnhardt Hermann1,Bibring Jean-Pierre2,Apathy Istvan3,Auster Hans Ulrich4,Ercoli Finzi Amalia5,Goesmann Fred1,Klingelhöfer Göstar6ORCID,Knapmeyer Martin7,Kofman Wlodek8,Krüger Harald1,Mottola Stefano7,Schmidt Walter9,Seidensticker Klaus7,Spohn Tilman7,Wright Ian10

Affiliation:

1. Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany

2. Institut d'Astrophysique Spatiale (IAS), 91405 Orsay, France

3. Atomic Energy Research Institute, PO Box 49, 1525 Budapest, Hungary

4. Institute for Geophysics and Extraterrestrial Physics, Technical University Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, Germany

5. Politecnico di Milano, via La Masa 34, 20156 Milano, Italy

6. Institute for Inorganic and Analytical Chemistry, Johannes Gutenberg University, Staudinger Weg 9, 55099 Mainz, Germany

7. Institute of Planetary Research, Deutsches Zentrum für Luft- und Raumfahrt, Rutherfordstr. 2, 12489 Berlin, Germany

8. UGA-Grenoble CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble, UMR 5274, 38058 Grenoble, France

9. Space Research Division, Finnish Meteorological Institute, 00560 Helsinki, Finland

10. Planetary and Space Science Research Institute, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK

Abstract

The Philae lander accomplished the first soft landing and the first scientific experiments of a human-made spacecraft on the surface of a comet. Planned, expected and unexpected activities and events happened during the descent, the touch-downs, the hopping across and the stay and operations on the surface. The key results were obtained during 12–14 November 2014, at 3 AU from the Sun, during the 63 h long period of the descent and of the first science sequence on the surface. Thereafter, Philae went into hibernation, waking up again in late April 2015 with subsequent communication periods with Earth (via the orbiter), too short to enable new scientific activities. The science return of the mission comes from eight of the 10 instruments on-board and focuses on morphological, thermal, mechanical and electrical properties of the surface as well as on the surface composition. It allows a first characterization of the local environment of the touch-down and landing sites. Unique conclusions on the organics in the cometary material, the nucleus interior, the comet formation and evolution became available through measurements of the Philae lander in the context of the Rosetta mission. This article is part of the themed issue ‘Cometary science after Rosetta’.

Funder

Max-Planck Society and by the German Space Agency

CNES, CNRS, University Joseph Fourier (UIF) Grenoble

Deutsches Zentrum för Luft- und Raumfahrt DLR

Science and Technology Facilities Council, UK

UK Space Agency

Publisher

The Royal Society

Subject

General Physics and Astronomy,General Engineering,General Mathematics

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