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The Philae lander reveals low-strength primitive ice inside cometary boulders.
O'Rourke, Laurence; Heinisch, Philip; Blum, Jürgen; Fornasier, Sonia; Filacchione, Gianrico; Van Hoang, Hong; Ciarniello, Mauro; Raponi, Andrea; Gundlach, Bastian; Blasco, Rafael Andrés; Grieger, Björn; Glassmeier, Karl-Heinz; Küppers, Michael; Rotundi, Alessandra; Groussin, Olivier; Bockelée-Morvan, Dominique; Auster, Hans-Ulrich; Oklay, Nilda; Paar, Gerhard; Perucha, Maria Del Pilar Caballo; Kovacs, Gabor; Jorda, Laurent; Vincent, Jean-Baptiste; Capaccioni, Fabrizio; Biver, Nicolas; Parker, Joel Wm; Tubiana, Cecilia; Sierks, Holger.
Afiliação
  • O'Rourke L; European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain. lorourke@esa.int.
  • Heinisch P; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Blum J; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Fornasier S; LESIA, Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, Meudon, France.
  • Filacchione G; Institut Universitaire de France (IUF), Paris, France.
  • Van Hoang H; Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
  • Ciarniello M; LESIA, Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, Meudon, France.
  • Raponi A; Université Grenoble Alpes, CNRS, Institut de Planétologie et Astrophysique de Grenoble (IPAG), UMR, Grenoble, France.
  • Gundlach B; Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
  • Blasco RA; Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
  • Grieger B; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Glassmeier KH; Telespazio Vega UK Ltd for the European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain.
  • Küppers M; Aurora Technology BV for the European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain.
  • Rotundi A; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Groussin O; European Space Agency (ESA), European Space Astronomy Centre (ESAC), Madrid, Spain.
  • Bockelée-Morvan D; Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
  • Auster HU; Dipartimento di Scienze e Tecnologie, Universitá degli Studi di Napoli Parthenope, Naples, Italy.
  • Oklay N; Aix Marseille Université, CNRS, CNES, LAM, Marseille, France.
  • Paar G; LESIA, Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, Meudon, France.
  • Perucha MDPC; Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany.
  • Kovacs G; Independent researcher, Berlin, Germany.
  • Jorda L; Joanneum Research Forschungsgesellschaft, Graz, Austria.
  • Vincent JB; Joanneum Research Forschungsgesellschaft, Graz, Austria.
  • Capaccioni F; Department of Mechatronics, Optics and Engineering Informatics, Budapest University of Technology and Economics, Budapest, Hungary.
  • Biver N; Aix Marseille Université, CNRS, CNES, LAM, Marseille, France.
  • Parker JW; DLR Institute of Planetary Research, Berlin, Germany.
  • Tubiana C; Istituto Nazionale di Astrofisica, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
  • Sierks H; LESIA, Observatoire de Paris, Université PSL, CNRS, Université de Paris, Sorbonne Université, Meudon, France.
Nature ; 586(7831): 697-701, 2020 10.
Article em En | MEDLINE | ID: mdl-33116289
ABSTRACT
On 12 November 2014, the Philae lander descended towards comet 67P/Churyumov-Gerasimenko, bounced twice off the surface, then arrived under an overhanging cliff in the Abydos region. The landing process provided insights into the properties of a cometary nucleus1-3. Here we report an investigation of the previously undiscovered site of the second touchdown, where Philae spent almost two minutes of its cross-comet journey, producing four distinct surface contacts on two adjoining cometary boulders. It exposed primitive water ice-that is, water ice from the time of the comet's formation 4.5 billion years ago-in their interiors while travelling through a crevice between the boulders. Our multi-instrument observations made 19 months later found that this water ice, mixed with ubiquitous dark organic-rich material, has a local dust/ice mass ratio of [Formula see text], matching values previously observed in freshly exposed water ice from outbursts4 and water ice in shadow5,6. At the end of the crevice, Philae made a 0.25-metre-deep impression in the boulder ice, providing in situ measurements confirming that primitive ice has a very low compressive strength (less than 12 pascals, softer than freshly fallen light snow) and allowing a key estimation to be made of the porosity (75 ± 7 per cent) of the boulders' icy interiors. Our results provide constraints for cometary landers seeking access to a volatile-rich ice sample.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Ano de publicação: 2020 Tipo de documento: Article