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Interstellar and interplanetary solids in the laboratory

  • Emmanuel Dartois (a1), Ivan Alata (a2), Cécile Engrand (a3), Rosario Brunetto (a1), Jean Duprat (a3), Thomas Pino (a2), Eric Quirico (a4), Laurent Remusat (a5), Noémie Bardin (a3), Smail Mostefaoui (a5), Gilles Morinaud (a1), Bruno Crane (a1), Nicolas Szwec (a1), Lucie Delauche (a3), Frédéric Jamme (a6), Christophe Sandt (a6) and Paul Dumas (a6)...

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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Copyright

Corresponding author

emmanuel.dartois@ias.u-psud.fr, to whom correspondence should be addressed

References

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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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