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The ORGANIC experiment on EXPOSE-R on the ISS: Flight sample preparation and ground control spectroscopy

  • K. L. Bryson*
  • , Z. Peeters
  • , F. Salama
  • , B. Foing
  • , P. Ehrenfreund
  • , A. J. Ricco
  • , E. Jessberger
  • , A. Bischoff
  • , M. Breitfellner
  • , W. Schmidt
  • , F. Robert
  • *Corresponding author for this work
  • Bay Area Environmental Research Institute
  • NASA Ames Research Center
  • Carnegie Institution of Washington
  • European Space Research and Technology Centre (ESTEC)
  • Leiden University
  • Space Policy Institute
  • University of Münster
  • European Space Astronomy Centre
  • Institut für PAH-Forschung
  • Muséum national d'histoire naturelle

Research output: Contribution to journalArticlepeer-review

15 Citations (Scopus)

Abstract

In March of 2009, the ORGANIC experiment integrated into the European multi-user facility EXPOSE-R, containing experiments dedicated to Astrobiology, was mounted through Extra Vehicular Activity (EVA) externally on the International Space Station (ISS). The experiment exposed organic samples of astronomical interest for a duration of 97 weeks (∼22 months) to the space environment. The samples that were returned to Earth in spring 2011, received a total UV radiation dose during their exposure including direct solar irradiation of >2500 h, exceeding the limits of laboratory simulations. We report flight sample preparation and pre-flight ultraviolet-visible (UV-Vis) characterization of the ORGANIC samples, which include 11 polycyclic aromatic hydrocarbons (PAHs) and three fullerenes. The corresponding time-dependent ground control monitoring experiments for ORGANIC measured over ∼19 months are presented and the results anticipated upon return of the samples are discussed. We present the first UV-Vis spectrum of solid circobiphenyl (C 38 H 16 ). Further, we present the first published UV-Vis spectra of diphenanthro[9,10-b′,10′-d]thiophene (C 28 H 16 S), dinaphtho[8,1,2-abc,2′,1′,8′-klm]coronene (C 36 H 16 ), tetrabenzo[de,no,st,c′d′]heptacene (C 42 H 22 ), and dibenzo[jk,a′b′]octacene (C 40 H 22 ) in solid phase and in solution. The results of the ORGANIC experiment are expected to enhance our knowledge of the evolution and degradation of large carbon-containing molecules in space environments.

Original languageEnglish
Pages (from-to)1980-1996
Number of pages17
JournalAdvances in Space Research
Volume48
Issue number12
DOIs
Publication statusPublished - 15 Dec 2011
Externally publishedYes

Keywords

  • Astrobiology
  • EXPOSE-R
  • ISS
  • PAHS

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