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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00006463naa a2200817 4500
001oai:DiVA.org:ri-13620
003SwePub
008160930s2016 | |||||||||||000 ||eng|
024a https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-136202 URI
024a https://doi.org/10.1038/nature193202 DOI
040 a (SwePub)ri
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Fray, Nicolasu CNRS, France; Paris Diderot University, France4 aut
2451 0a High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko
264 c 2016-09-07
264 1b Nature Publishing Group,c 2016
338 a print2 rdacarrier
520 a The presence of solid carbonaceous matter in cometary dust was established by the detection of elements such as carbon, hydrogen, oxygen and nitrogen in particles from comet 1P/Halley1, 2. Such matter is generally thought to have originated in the interstellar medium3, but it might have formed in the solar nebula—the cloud of gas and dust that was left over after the Sun formed4. This solid carbonaceous material cannot be observed from Earth, so it has eluded unambiguous characterization5. Many gaseous organic molecules, however, have been observed6, 7, 8, 9; they come mostly from the sublimation of ices at the surface or in the subsurface of cometary nuclei8. These ices could have been formed from material inherited from the interstellar medium that suffered little processing in the solar nebula10. Here we report the in situ detection of solid organic matter in the dust particles emitted by comet 67P/Churyumov–Gerasimenko; the carbon in this organic material is bound in very large macromolecular compounds, analogous to the insoluble organic matter found in the carbonaceous chondrite meteorites11, 12. The organic matter in meteorites might have formed in the interstellar medium and/or the solar nebula, but was almost certainly modified in the meteorites’ parent bodies11. We conclude that the observed cometary carbonaceous solid matter could have the same origin as the meteoritic insoluble organic matter, but suffered less modification before and/or after being incorporated into the comet.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a Asteroids
653 a comets
653 a Kuiper belt
700a Bardyn, Anaïsu CNRS, France; Paris Diderot University, France; University of Orléans, France4 aut
700a Cottin, Hervéu CNRS, France; Paris Diderot University, France4 aut
700a Altwegg, Kathrinu University of Bern, Switzerland4 aut
700a Baklouti, Doniau CNRS, France; University of Paris-Sud, France4 aut
700a Briois, Christelleu CNRS, France; University of Orléans, France4 aut
700a Colangeli, Luigiu ESTEC European Space Research and Technology Centre, The Netherlands4 aut
700a Engrand, Cécileu CNRS, France; University of Paris-Saclay, France; University of Paris-Sud, France4 aut
700a Fischer, Henningu Max Planck Institute for Solar System Research, Germany4 aut
700a Glasmachers, Albrechtu University of Wuppertal, Germany4 aut
700a Grün, Eberhardu Max Planck Institute for Nuclear Physics, Germany4 aut
700a Haerendel, Gerhardu Max Planck Institute for Extraterrestrial Physics, Germany4 aut
700a Henkel, Hartmutu Von Hoerner und Sulger GmbH, Germany4 aut
700a Höfner, Herwigu Max Planck Institute for Extraterrestrial Physics, Germany4 aut
700a Hornung, Klausu Universität der Bundeswehr, Germany4 aut
700a Jessberger, Elmar K.u University of Münster, Germany4 aut
700a Koch, Andreasu Von Hoerner und Sulger GmbH, Germany4 aut
700a Krüger, Haraldu Max Planck Institute for Solar System Research, Germany4 aut
700a Langevin, Yvesu CNRS, France; University of Paris-Sud, France4 aut
700a Lehto, Harryu University of Turku, Finland4 aut
700a Lehto, Kirsiu University of Turku, Finland4 aut
700a Le Roy, Lénau University of Bern, Switzerland4 aut
700a Merouane, Sihaneu Max Planck Institute for Solar System Research, Germany4 aut
700a Modica, Paolau CNRS, France; Paris Diderot University, France; University of Orléans, France4 aut
700a Orthous-Daunay, François-Régisu CNRS, France; Université Grenoble Alpes, France4 aut
700a Paquette, Johnu Max Planck Institute for Solar System Research, Germany4 aut
700a Raulin, Françoisu CNRS, France; Paris Diderot University, France4 aut
700a Rynö, Jouniu Finnish Meteorological Institute, Finland4 aut
700a Schulz, Ritau ESA European Space Agency, The Netherlands4 aut
700a Silén, Johanu Finnish Meteorological Institute, Finland4 aut
700a Siljeström, Sandrau RISE,Medicinteknik4 aut0 (Swepub:ri)SandraSi@ri.se
700a Steiger, Wolfgangu RC Seibersdorf Research GmbH Business Field Aerospace Technology, Austria4 aut
700a Stenzel, Oliveru Max Planck Institute for Solar System Research, Germany4 aut
700a Stephan, Thomasu University of Chicago, USA4 aut
700a Thirkell, Laurentu CNRS, France; University of Orléans, France4 aut
700a Thomas, Rogeru CNRS, France; University of Orléans, France4 aut
700a Torkar, Klausu Austrian Academy of Sciences, Austria4 aut
700a Varmuza, Kurtu Vienna University of Technology, Austria4 aut
700a Wanczek, Karl-Peteru University of Bremen, Germany4 aut
700a Zaprudin, Borisu University of Turku, Finland4 aut
700a Kissel, Jochenu Max Planck Institute for Solar System Research, Germany4 aut
700a Hilchenbach, Martinu Max Planck Institute for Solar System Research, Germany4 aut
710a CNRS, France; Paris Diderot University, Franceb CNRS, France; Paris Diderot University, France; University of Orléans, France4 org
773t Natured : Nature Publishing Groupg 538:7623, s. 72-74q 538:7623<72-74x 0028-0836x 1476-4687
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-13620
8564 8u https://doi.org/10.1038/nature19320

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