New Pathway to Hydrogen Cyanide on Early Earth Unveiled

What the research is about

Hydrogen cyanide (HCN) is widely known as a toxic gas. However, in studies on the origin of life, it is considered one of the most important molecules because it can serve as a starting material for producing the building blocks of life, including DNA, RNA, amino acids, and lipids.

Since the famous Miller-Urey experiment in the 1950s, scientists have generally believed that HCN on early Earth was produced from methane (CH4) in the atmosphere. Later studies, however, suggested that methane may not have been as abundant on early Earth as previously thought. This raised a major question: if methane was scarce, where did the HCN needed for life come from?

To explore this question, a research team led by Professor Ryuhei Nakamura of Institute of Science Tokyo (Science Tokyo) focused on amino acids, which are thought to have been abundant on early Earth. The team examined 38 different minerals, including minerals found in deep-sea hydrothermal vent deposits ("chimneys") and minerals originating from meteorites.

The researchers discovered that manganese dioxide (MnO2), a common mineral, helps oxidize amino acids, producing HCN as a reaction product. Remarkably, the reaction proceeded in mild aqueous environments without oxygen gas-conditions similar to those on Earth before life emerged.

The study also showed that not only glycine, the simplest amino acid, but also various other amino acids and short peptides could react with MnO2 to produce HCN. In other words, amino acids themselves-already considered important ingredients for life-may also have helped generate another key ingredient for life.

Why this matters

This study suggests that even if methane levels were low on early Earth, chemical reactions needed to produce the building blocks of life could still have taken place. Previous studies showed that amino acids could break down into substances such as ammonia (NH3) and carbon dioxide (CO2), but they rarely produced HCN. In other experiments using electricity, scientists detected cyanide groups (-CN) attached to the surfaces of gold or platinum electrodes. However, these surface-bound molecules were not the "free" HCN needed to react with other molecules and help build the chemistry of life.

In the new study, MnO2 played a special role. The research team carefully investigated whether the detected HCN truly came from amino acids and which part of the amino acid molecule was transformed into HCN. The team focused on glycine (NH2CH2COOH), the simplest amino acid, which contains two carbon atoms. By labeling each carbon atom and tracking the reaction, the researchers found that the carbon in the CH2 group was converted into HCN. This result revealed a previously unknown reaction pathway in which MnO2 specifically interacts with the CH2 part of amino acids.

What's next

This research addresses one of science's biggest questions: how did life begin? The discovery of an HCN formation pathway that does not depend on methane could provide new clues not only about early Earth, but also about the possibility of life-forming chemistry on other planets such as Mars.

The findings may also have practical applications. HCN is an important industrial chemical used in metal extraction and chemical synthesis. In the future, this reaction could contribute to technologies that convert plant-derived amino acids into useful chemicals, as well as more sustainable methods for resource mining.

Comment from the researcher

The Miller-Urey experiment has had a major influence on origin-of-life research for nearly 70 years. However, questions remained about whether methane was actually abundant on early Earth. Our discovery could significantly change this long-standing view. While this study explores the origin of life, it may also contribute to future advances in chemistry and environmental technologies.

(Ryuhei Nakamura, Professor, Earth-Life Science Institute (ELSI), Institute of Future Science, Institute of Science Tokyo)

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