Sökning: WFRF:(Roger Sandra) > High-molecular-weig...
Fältnamn | Indikatorer | Metadata |
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000 | 06463naa a2200817 4500 | |
001 | oai:DiVA.org:ri-13620 | |
003 | SwePub | |
008 | 160930s2016 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-136202 URI |
024 | 7 | a https://doi.org/10.1038/nature193202 DOI |
040 | a (SwePub)ri | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Fray, Nicolasu CNRS, France; Paris Diderot University, France4 aut |
245 | 1 0 | a High-molecular-weight organic matter in the particles of comet 67P/Churyumov–Gerasimenko |
264 | c 2016-09-07 | |
264 | 1 | b 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 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
653 | a Asteroids | |
653 | a comets | |
653 | a Kuiper belt | |
700 | 1 | a Bardyn, Anaïsu CNRS, France; Paris Diderot University, France; University of Orléans, France4 aut |
700 | 1 | a Cottin, Hervéu CNRS, France; Paris Diderot University, France4 aut |
700 | 1 | a Altwegg, Kathrinu University of Bern, Switzerland4 aut |
700 | 1 | a Baklouti, Doniau CNRS, France; University of Paris-Sud, France4 aut |
700 | 1 | a Briois, Christelleu CNRS, France; University of Orléans, France4 aut |
700 | 1 | a Colangeli, Luigiu ESTEC European Space Research and Technology Centre, The Netherlands4 aut |
700 | 1 | a Engrand, Cécileu CNRS, France; University of Paris-Saclay, France; University of Paris-Sud, France4 aut |
700 | 1 | a Fischer, Henningu Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Glasmachers, Albrechtu University of Wuppertal, Germany4 aut |
700 | 1 | a Grün, Eberhardu Max Planck Institute for Nuclear Physics, Germany4 aut |
700 | 1 | a Haerendel, Gerhardu Max Planck Institute for Extraterrestrial Physics, Germany4 aut |
700 | 1 | a Henkel, Hartmutu Von Hoerner und Sulger GmbH, Germany4 aut |
700 | 1 | a Höfner, Herwigu Max Planck Institute for Extraterrestrial Physics, Germany4 aut |
700 | 1 | a Hornung, Klausu Universität der Bundeswehr, Germany4 aut |
700 | 1 | a Jessberger, Elmar K.u University of Münster, Germany4 aut |
700 | 1 | a Koch, Andreasu Von Hoerner und Sulger GmbH, Germany4 aut |
700 | 1 | a Krüger, Haraldu Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Langevin, Yvesu CNRS, France; University of Paris-Sud, France4 aut |
700 | 1 | a Lehto, Harryu University of Turku, Finland4 aut |
700 | 1 | a Lehto, Kirsiu University of Turku, Finland4 aut |
700 | 1 | a Le Roy, Lénau University of Bern, Switzerland4 aut |
700 | 1 | a Merouane, Sihaneu Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Modica, Paolau CNRS, France; Paris Diderot University, France; University of Orléans, France4 aut |
700 | 1 | a Orthous-Daunay, François-Régisu CNRS, France; Université Grenoble Alpes, France4 aut |
700 | 1 | a Paquette, Johnu Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Raulin, Françoisu CNRS, France; Paris Diderot University, France4 aut |
700 | 1 | a Rynö, Jouniu Finnish Meteorological Institute, Finland4 aut |
700 | 1 | a Schulz, Ritau ESA European Space Agency, The Netherlands4 aut |
700 | 1 | a Silén, Johanu Finnish Meteorological Institute, Finland4 aut |
700 | 1 | a Siljeström, Sandrau RISE,Medicinteknik4 aut0 (Swepub:ri)SandraSi@ri.se |
700 | 1 | a Steiger, Wolfgangu RC Seibersdorf Research GmbH Business Field Aerospace Technology, Austria4 aut |
700 | 1 | a Stenzel, Oliveru Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Stephan, Thomasu University of Chicago, USA4 aut |
700 | 1 | a Thirkell, Laurentu CNRS, France; University of Orléans, France4 aut |
700 | 1 | a Thomas, Rogeru CNRS, France; University of Orléans, France4 aut |
700 | 1 | a Torkar, Klausu Austrian Academy of Sciences, Austria4 aut |
700 | 1 | a Varmuza, Kurtu Vienna University of Technology, Austria4 aut |
700 | 1 | a Wanczek, Karl-Peteru University of Bremen, Germany4 aut |
700 | 1 | a Zaprudin, Borisu University of Turku, Finland4 aut |
700 | 1 | a Kissel, Jochenu Max Planck Institute for Solar System Research, Germany4 aut |
700 | 1 | a Hilchenbach, Martinu Max Planck Institute for Solar System Research, Germany4 aut |
710 | 2 | a CNRS, France; Paris Diderot University, Franceb CNRS, France; Paris Diderot University, France; University of Orléans, France4 org |
773 | 0 | t Natured : Nature Publishing Groupg 538:7623, s. 72-74q 538:7623<72-74x 0028-0836x 1476-4687 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:ri:diva-13620 |
856 | 4 8 | u https://doi.org/10.1038/nature19320 |
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