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Title:
Interstellar and interplanetary solids in the laboratory
Authors:
Dartois, Emmanuel; Alata, Ivan; Engrand, Cécile; Brunetto, Rosario; Duprat, Jean; Pino, Thomas; Quirico, Eric; Remusat, Laurent; Bardin, Noémie; Mostefaoui, Smail; Morinaud, Gilles; Crane, Bruno; Szwec, Nicolas; Delauche, Lucie; Jamme, Frédéric; Sandt, Christophe; Dumas, Paul
Affiliation:
AA(Institut d'Astrophysique Spatiale, UMR8617 CNRS-Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, Univ. Paris-Sud, 91405 Orsay, France), AB(ISMO, UMR 8214-CNRS Université Paris Sud, bât 210, 91405 Orsay Cedex, France), AC(Centre de Sciences Nucléaires et de Sciences de la Matière, UMR8609 CNRS/IN2P3-Univ. Paris-Sud, Université Paris-Saclay, Bât. 104, 91405 Orsay, France), AD(Institut d'Astrophysique Spatiale, UMR8617 CNRS-Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, Univ. Paris-Sud, 91405 Orsay, France), AE(Centre de Sciences Nucléaires et de Sciences de la Matière, UMR8609 CNRS/IN2P3-Univ. Paris-Sud, Université Paris-Saclay, Bât. 104, 91405 Orsay, France), AF(ISMO, UMR 8214-CNRS Université Paris Sud, bât 210, 91405 Orsay Cedex, France), AG(IPAG, UJF-Grenoble 1/CNRS-INSU, UMR 5274, 38041 Grenoble, France), AH(IMPMC, UMR 7590 CNRS, UPMC, IRD, MNHN, 61 rue Buffon, 75005 Paris, France), AI(Centre de Sciences Nucléaires et de Sciences de la Matière, UMR8609 CNRS/IN2P3-Univ. Paris-Sud, Université Paris-Saclay, Bât. 104, 91405 Orsay, France), AJ(IMPMC, UMR 7590 CNRS, UPMC, IRD, MNHN, 61 rue Buffon, 75005 Paris, France), AK(Institut d'Astrophysique Spatiale, UMR8617 CNRS-Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, Univ. Paris-Sud, 91405 Orsay, France), AL(Institut d'Astrophysique Spatiale, UMR8617 CNRS-Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, Univ. Paris-Sud, 91405 Orsay, France), AM(Institut d'Astrophysique Spatiale, UMR8617 CNRS-Univ. Paris-Sud, Université Paris-Saclay, Bât. 121, Univ. Paris-Sud, 91405 Orsay, France), AN(Centre de Sciences Nucléaires et de Sciences de la Matière, UMR8609 CNRS/IN2P3-Univ. Paris-Sud, Université Paris-Saclay, Bât. 104, 91405 Orsay, France), AO(Synchrotron SOLEIL, BP48, Saint Aubin, 91192 Gif sur Yvette, France), AP(Synchrotron SOLEIL, BP48, Saint Aubin, 91192 Gif sur Yvette, France), AQ(Synchrotron SOLEIL, BP48, Saint Aubin, 91192 Gif sur Yvette, France)
Publication:
Astronomy in Focus, as presented at the IAU XXIX General Assembly, 2015. Proceedings of the IAU, Volume 29B, 2016, pp. 416-419
Publication Date:
00/2016
Origin:
CUP
Keywords:
ISM: dust, extinction, ISM: lines and bands, interplanetary medium, comets: general, Kuiper Belt, Oort Cloud,
Abstract Copyright:
(c) 2016: Copyright © International Astronomical Union 2016
DOI:
10.1017/S1743921316005688
Bibliographic Code:
2016IAUFM..29B.416D

Abstract

The composition of interstellar matter is driven by environmental parameters and results from extreme interstellar medium physico-chemical conditions. Astrochemists must rely on remote observations to monitor and analyze the interstellar solids composition. They bring additional information from the study of analogues produced in the laboratory, placed in simulated space environments. Planetologists and cosmochemists access and spectroscopically examine collected extraterrestrial material in the laboratory. Diffuse interstellar medium and molecular clouds observations set constraints on the composition of organic solids that can then be compared with collected extraterrestrial materials analyses, to shed light on their possible links.
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