Oil shale, a sedimentary rock containing organic matter and a variety of inorganic minerals including carbonates and
kerogens, serves as a significant source of organic material on Earth [1]. Kerogen, the most abundant form of organic
matter, differs in chemical composition based on the microorganisms that contributed to its formation [2]. Laser-induced
breakdown spectroscopy (LIBS) is a powerful analytical technique used on the Mars rover, allowing elemental
characterization of Martian rocks, soils, and sediments.
This study presents the first-ever detection of natural organic matter in oil shale using LIBS under simulated Martian
conditions. Through an analysis of emitting species including CN and C2, LIBS successfully identifies the presence of
organic compounds in this sedimentary rock. The ability to detect and characterize natural organic matter in oil shale,
known for its potential to suggest the existence of ancient life, holds significant relevance in astrobiology. Furthermore,
this information contributes to the identification of biosignatures and aids in the development of planetary exploration
strategies.
Oil shale samples were analyzed using LIBS under simulated Martian conditions after being crushed, pressed into
pellets, and subjected to pyrolysis to remove organic matter. The analysis revealed significant changes in the infrared
spectra, confirming the absence of aliphatic hydrocarbons after pyrolysis [3]. The LIBS results demonstrated the
presence of molecular species associated with hydrocarbons, such as CN and C2, through distinct spectral emissions.
The absence of these emissions in the pyrolyzed sample further supported the detection of organic matter originating
from kerogen.