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Krypton isotopes and noble gas abundances in the coma of comet 67P/Churyumov-Gerasimenko.
Rubin, Martin; Altwegg, Kathrin; Balsiger, Hans; Bar-Nun, Akiva; Berthelier, Jean-Jacques; Briois, Christelle; Calmonte, Ursina; Combi, Michael; De Keyser, Johan; Fiethe, Björn; Fuselier, Stephen A; Gasc, Sebastien; Gombosi, Tamas I; Hansen, Kenneth C; Kopp, Ernest; Korth, Axel; Laufer, Diana; Le Roy, Léna; Mall, Urs; Marty, Bernard; Mousis, Olivier; Owen, Tobias; Rème, Henri; Sémon, Thierry; Tzou, Chia-Yu; Waite, Jack H; Wurz, Peter.
  • Rubin M; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Altwegg K; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Balsiger H; Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, CH-3012 Bern, Switzerland.
  • Bar-Nun A; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Berthelier JJ; Department of Geophysics, Tel Aviv University, Ramat-Aviv, Tel Aviv, Israel.
  • Briois C; Laboratoire Atmosphères, Milieux, Observations Spatiales, Institut Pierre Simon Laplace, CNRS, Université Pierre et Marie Curie, 4 Place Jussieu, 75252 Paris Cedex 05, France.
  • Calmonte U; Laboratoire de Physique et Chimie de l'Environnement et de l'Espace, UMR 6115 CNRS-Université d'Orléans, Orléans, France.
  • Combi M; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • De Keyser J; Department of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.
  • Fiethe B; Koninklijk Belgisch Instituut voor Ruimte-Aeronomie-Institut Royal Belge d'Aéronomie Spatiale, Ringlaan 3, B-1180 Brussels, Belgium.
  • Fuselier SA; Institute of Computer and Network Engineering, Technische Universität Braunschweig, Hans-Sommer-Straße 66, D-38106 Braunschweig, Germany.
  • Gasc S; Space Science Directorate, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA.
  • Gombosi TI; University of Texas at San Antonio, San Antonio, TX 78249, USA.
  • Hansen KC; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Kopp E; Department of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.
  • Korth A; Department of Climate and Space Sciences and Engineering, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA.
  • Laufer D; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Le Roy L; Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.
  • Mall U; Department of Geophysics, Tel Aviv University, Ramat-Aviv, Tel Aviv, Israel.
  • Marty B; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
  • Mousis O; Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.
  • Owen T; Centre de Recherches Pétrographiques et Géochimiques, CNRS, Université de Lorraine, 15 rue Notre Dame des Pauvres, BP 20, 54501 Vandoeuvre lès Nancy, France.
  • Rème H; Laboratoire d'Astrophysique de Marseille, CNRS, Aix-Marseille Université, 13388 Marseille, France.
  • Sémon T; Institute for Astronomy, University of Hawaii, Honolulu, HI 96822, USA.
  • Tzou CY; Institut de Recherche en Astrophysique et Planétologie, CNRS, Université Paul Sabatier, Observatoire Midi-Pyrénées, 9 Avenue du Colonel Roche, 31028 Toulouse Cedex 4, France.
  • Waite JH; Centre National d'Études Spatiales, 2 Place Maurice Quentin, 75001 Paris, France.
  • Wurz P; Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland.
Sci Adv ; 4(7): eaar6297, 2018 07.
Article en En | MEDLINE | ID: mdl-29978041
The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis mass spectrometer Double Focusing Mass Spectrometer on board the European Space Agency's Rosetta spacecraft detected the major isotopes of the noble gases argon, krypton, and xenon in the coma of comet 67P/Churyumov-Gerasimenko. Earlier, it was found that xenon exhibits an isotopic composition distinct from anywhere else in the solar system. However, argon isotopes, within error, were shown to be consistent with solar isotope abundances. This discrepancy suggested an additional exotic component of xenon in comet 67P/Churyumov-Gerasimenko. We show that krypton also exhibits an isotopic composition close to solar. Furthermore, we found the argon to krypton and the krypton to xenon ratios in the comet to be lower than solar, which is a necessity to postulate an addition of exotic xenon in the comet.