Integration of LIBS instruments in the rover used for planetary exploration in an attempt to get multi-elemental
information from rocks, minerals, and soils is a reality. Its great effectiveness has been demonstrated in many
works from the research teams participating in the mission Mars Science Laboratory (MSL). However, the detection
and discrimination by LIBS of organic compounds can be complex since, among other aspects; this technique is
very sensitive to environmental conditions, such as the atmosphere composition and pressure [1-3].
The objective of this investigation is to assess the effect of the surrounding atmosphere (CO2) on the formation of
emitting species in laser-induced plasmas of C-containing compounds in order to identify the possible both
inorganic and organic sources. Moreover, the influence of molecular structures on the intensity of C, C2, CN, H, N
and O emissions has been analyzed (Fig. 1). Four organic compounds (adenine, glycine, pyrene, and urea) were
selected for their interest as possible indicators or precursors of life. A laboratory LIBS system coupled to a
pressure chamber for simulating Martian environment was used for the analysis of pellet-shaped samples.
Formation pathways of species coexisting in the plasma plume (C, C2 and CN, mainly) generated in air and in CO2
atmosphere have been considered. The ablation thresholds and the limits of detection of the organic molecules on
inorganic matrices (CaCO3 and CaSO4 2H2O) have been established
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