Tokyo Tech News

Tracing the Origins of Organic Matter in Martian Sediments


Published: May 14, 2024

Organic matter on Mars may have been formed due to atmospheric processes rather than have biological origin suggests researchers at Tokyo Tech. Using photolysis experiments and theoretical considerations, researchers demonstrate that the organic matter in sediments is formed from carbon monoxide, which originates from the photodissociation of carbon dioxide in the atmosphere. This process results in organic matter with low amounts of carbon-13 isotope, as observed in sediments from the Gale crater on Mars.

Decoding Martian Organic Matter Origins:  Insights from Isotopic Analysis

Although Mars presents a barren, dusty landscape with no signs of life so far, its geological features such as deltas, lakebeds, and river valleys strongly suggest a past where water once flowed abundantly on its surface. To explore this possibility, scientists examine sediments preserved near these formations. The composition of these sediments holds clues about the early environmental conditions, the processes that shaped the planet over time, and even potential signs of past life.

In one such analysis, sediments collected by the Curiosity rover from Gale Crater, believed to be an ancient lake formed approximately 3.8 billion years ago due to an asteroid impact, revealed organic matter. However, this organic matter had a significantly lower amount of the carbon-13 isotope (13C) relative to carbon-12 isotopes (12C) compared to what is found on Earth, suggesting different processes of organic matter formation on Mars.

Now, a study published in the journal Nature Geoscience on May 9, 2024, elucidates this discrepancy. A research team, led by Professor Yuichiro Ueno from Tokyo Institute of Technology and Professor Matthew Johnson from the University of Copenhagen, found that the photodissociation of carbon dioxide (CO2) in the atmosphere to carbon monoxide (CO) and subsequent reduction result in organic matter with depleted 13C content.

"On measuring the stable isotope ratio between 13C and 12C, the Martian organic matter has a 13C abundance of 0.92% to 0.99% of the carbon that makes it up. This is extremely low compared to Earth's sedimentary organic matter, which is about 1.04%, and atmospheric CO2, around 1.07%, both of which are biological remnants, and are not similar to the organic matter in meteorites, which is about 1.05%," explains Ueno.

Early Mars had an atmosphere rich in CO2 containing both 13C and 12C isotopes. The researchers simulated different conditions of the Martian atmosphere's composition and temperature in laboratory experiments. They found that when 12CO2 is exposed to solar ultraviolet (UV) light, it preferentially absorbs UV radiation, leading to its dissociation into CO depleted in 13C, leaving behind CO2 enriched in 13C.

This isotopic fractionation (separation of isotopes) is also observed in the upper atmospheres of Mars and Earth, where UV irradiation from the Sun causes CO2 to dissociate into CO with depleted 13C content. In a reducing Martian atmosphere, CO transforms into simple organic compounds such as formaldehyde and carboxylic acids. During the early Martian era, with surface temperatures close to the freezing point of water and not exceeding 300 K (27°C), these compounds may have dissolved in water and settled in sediments.

Using model calculations, the researchers found that in an atmosphere with a CO2 to CO ratio of 90:10, a 20% conversion of CO2 to CO would lead to sedimentary organic matter with δ13CVPDB values of -135‰. Also, the remaining CO2 would be enriched in 13C with δ13CVPDB values of +20‰. These values closely matche those seen in sediments analyzed by the Curiosity rover and estimated from a Martian meteorite. This finding points to an atmospheric process rather than a biological one as the main source of organic matter formation on early Mars.

"If the estimation in this research is correct, there may be an unexpected amount of organic material present in Martian sediments. This suggests that future explorations of Mars might uncover large quantities of organic matter," says Ueno.


Authors :
Yuichiro Ueno1,2,3,*, Johan A. Schmidt4,9, Matthew S. Johnson4, Xiaofeng Zang1, Alexis Gilbert1,2, Hiroyuki Kurokawa2,5, Tomohiro Usui2,6, Shohei Aoki7,8
Title :
Synthesis of 13C-depleted organic matter from CO in a reducing early Martian atmosphere
Journal :
Nature Geoscience
Affiliations :

1 Department of Earth and Planetary Sciences, Tokyo Institute of Technology, Tokyo, Japan

2 Earth-Life Science Institute, Tokyo Institute of Technology, Japan

3 Japan Agency for Marine-Earth Science and Technology (JAMSTEC), Japan

4 Department of Chemistry, University of Copenhagen, Denmark

5 Department of Earth Science and Astronomy, The University of Tokyo, Japan

6 Japan Aerospace Exploration Agency, Japan

7 Department of Complexity Science and Engineering, The University of Tokyo, Japan

8 Royal Belgian Institute for Space Aeronomy, Belgium

9 Present address: Devlabs ApS, Denmark

* Corresponding author's email:

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Professor Yuichiro Ueno

School of Science, Tokyo Institute of Technology



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