Literature DB >> 19827851

Chemical characterization of Titan's tholins: solubility, morphology and molecular structure revisited.

N Carrasco1, I Schmitz-Afonso, J-Y Bonnet, E Quirico, R Thissen, Odile Dutuit, A Bagag, O Laprévote, A Buch, A Giulani, Gilles Adandé, F Ouni, E Hadamcik, C Szopa, G Cernogora.   

Abstract

In this work Titan's atmospheric chemistry is simulated using a capacitively coupled plasma radio frequency discharge in a N(2)-CH(4) stationnary flux. Samples of Titan's tholins are produced in gaseous mixtures containing either 2 or 10% methane before the plasma discharge, covering the methane concentration range measured in Titan's atmosphere. We study their solubility and associated morphology, their infrared spectroscopy signature and the mass distribution of the soluble fraction by mass spectrometry. An important result is to highlight that the previous Titan's tholin solubility studies are inappropriate to fully characterize such a heterogeneous organic matter and we develop a new protocol to evaluate quantitatively tholins solubility. We find that tholins contain up to 35% in mass of molecules soluble in methanol, attached to a hardly insoluble fraction. Methanol is then chosen as a discriminating solvent to characterize the differences between soluble and insoluble species constituting the bulk tholins. No significant morphological change of shape or surface feature is derived from scanning electron microscopy after the extraction of the soluble fraction. This observation suggests a solid structure despite an important porosity of the grains. Infrared spectroscopy is recorded for both fractions. The IR spectra of the bulk, soluble, and insoluble tholins fractions are found to be very similar and reveal identical chemical signatures of nitrogen bearing functions and aliphatic groups. This result confirms that the chemical information collected when analyzing only the soluble fraction provides a valuable insight representative of the bulk material. The soluble fraction is ionized with an atmospheric pressure photoionization source and analyzed by a hybrid mass spectrometer. The congested mass spectra with one peak at every mass unit between 50 and 800 u confirm that the soluble fraction contains a complex mixture of organic molecules. The broad distribution, however, exhibits a regular pattern of mass clusters. Tandem collision induced dissociation analysis is performed in the negative ion mode to retrieve structural information. It reveals that (i) the molecules are ended by methyl, amine and cyanide groups, (ii) a 27 u neutral moiety (most probably HCN) is often released in the fragmentation of tholin anions, and (iii) an ubiquitous ionic fragment at m/z 66 is found in all tandem spectra. A tentative structure is proposed for this negative ion.

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Year:  2009        PMID: 19827851     DOI: 10.1021/jp904735q

Source DB:  PubMed          Journal:  J Phys Chem A        ISSN: 1089-5639            Impact factor:   2.781


  3 in total

1.  Formation of amino acids and nucleotide bases in a Titan atmosphere simulation experiment.

Authors:  S M Hörst; R V Yelle; A Buch; N Carrasco; G Cernogora; O Dutuit; E Quirico; E Sciamma-O'Brien; M A Smith; A Somogyi; C Szopa; R Thissen; V Vuitton
Journal:  Astrobiology       Date:  2012-08-23       Impact factor: 4.335

2.  Structural Study of Analogues of Titan's Haze by Trapped Ion Mobility Coupled with a Fourier Transform Ion Cyclotron Mass Spectrometer.

Authors:  Christopher P Rüger; Julien Maillard; Johann Le Maître; Mark Ridgeway; Christopher J Thompson; Isabelle Schmitz-Afonso; Thomas Gautier; Nathalie Carrasco; Melvin A Park; Pierre Giusti; Carlos Afonso
Journal:  J Am Soc Mass Spectrom       Date:  2019-05-07       Impact factor: 3.109

3.  The Role of Ultrahigh Resolution Fourier Transform Mass Spectrometry (FT-MS) in Astrobiology-Related Research: Analysis of Meteorites and Tholins.

Authors:  Árpád Somogyi; Roland Thissen; Francois-Régis Orthous-Daunay; Véronique Vuitton
Journal:  Int J Mol Sci       Date:  2016-03-24       Impact factor: 5.923

  3 in total

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