Characterization of aromaticity in analogues of titan's atmospheric aerosols with two-step laser desorption ionization mass spectrometry
Ahmed Mahjoub, Martin Schwell, Nathalie Carrasco, Yves Benilan, Guy, Cernogora, Cyril Szopa, Marie-Claire Gazeau

TL;DR
This study uses advanced laser mass spectrometry to identify aromatic compounds, including PAHs and PANHs, in Titan's aerosol analogues, revealing their presence and potential astrobiological relevance.
Contribution
It demonstrates the application of Two-Step Laser Desorption Ionization Mass Spectrometry to detect aromatic molecules in Titan's aerosol analogues, including nitrogen-containing PAHs and biologically relevant molecules.
Findings
Detection of small PAHs with 1-3 aromatic rings in Titan's aerosol analogues.
Identification of nitrogen-containing PAHs (PANHs) in the analogues.
Presence of molecules relevant to astrobiology, such as adenine.
Abstract
The role of polycyclic aromatic hydrocarbons (PAH) and Nitrogen containing PAH (PANH) as intermediates of aerosol production in the atmosphere of Titan has been a subject of controversy for a long time. An analysis of the atmospheric emission band observed by the Visible and Infrared Mapping Spectrometer (VIMS) at 3.28 micrometer suggests the presence of neutral polycyclic aromatic species in the upper atmosphere of Titan. These molecules are seen as the counter part of negative and positive aromatics ions suspected by the Plasma Spectrometer onboard the Cassini spacecraft, but the low resolution of the instrument hinders any molecular speciation. In this work we investigate the specific aromatic content of Titan's atmospheric aerosols through laboratory simulations. We report here the selective detection of aromatic compounds in tholins, Titan's aerosol analogues, produced with a…
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