Frozen hydrogen cyanide may have sparked life on Earth

A new study suggests that hydrogen cyanide, a highly poisonous chemical, could have played a key role in the origins of life by forming reactive ice crystals in extreme cold. Computer simulations show these crystals promote unusual chemical reactions that produce building blocks for life. The findings highlight the chemical potential of frozen environments, including those beyond Earth.

Hydrogen cyanide, known for its toxicity to humans, freezes into crystals at low temperatures, creating surfaces that are unusually reactive. Researchers used computer modeling to examine these crystals, revealing that they can drive chemical processes typically impossible in frigid conditions. The study, published in ACS Central Science, indicates that such reactions might have initiated the formation of life's fundamental components.

The team, led by Martin Rahm, modeled a hydrogen cyanide crystal resembling a 450-nanometer-long cylinder with a rounded base and multifaceted top, akin to earlier observations of "cobweb" formations. Their simulations identified two pathways converting hydrogen cyanide to the more reactive hydrogen isocyanide, occurring in minutes to days depending on temperature. This compound on crystal surfaces could facilitate the creation of complex prebiotic molecules.

"We may never know precisely how life began, but understanding how some of its ingredients take shape is within reach. Hydrogen cyanide is likely one source of this chemical complexity, and we show that it can react surprisingly quickly in cold places," Rahm stated.

Hydrogen cyanide is common in space, detected on comets and in atmospheres like that of Saturn's moon Titan. Interacting with water, it forms polymers, amino acids, and nucleobases—essentials for proteins and DNA. The researchers, Marco Cappelletti, Hilda Sandström, and Rahm, propose lab tests, such as crushing crystals with water to expose surfaces and observe molecule formation in cold settings.

Funded by the Swedish Research Council and Sweden's National Academic Infrastructure for Supercomputing, the work underscores that icy worlds may be more chemically active than previously assumed, with implications for prebiotic chemistry on early Earth and elsewhere.

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ETH Zurich scientists with single-atom indium catalyst converting CO2 to methanol in a high-tech lab reactor, sustainable energy theme.
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Scientists develop single-atom catalyst for CO2-to-methanol conversion

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Researchers at ETH Zurich have engineered a catalyst using isolated indium atoms on hafnium oxide to convert CO2 and hydrogen into methanol more efficiently than previous methods. This single-atom design maximizes metal use and enables clearer study of reaction mechanisms. The breakthrough could support sustainable chemical production if powered by renewables.

Scientists suggest that asteroid impacts created hot, chemical-rich environments that could have kick-started life on Earth. A new review led by recent Rutgers graduate Shea Cinquemani highlights impact-generated hydrothermal systems as potential cradles for life's building blocks. These systems may have persisted for thousands of years, providing ideal conditions for early biology.

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Researchers at ETH Zurich have discovered that Earth formed with just the right amount of oxygen during its core development, keeping essential phosphorus and nitrogen accessible for life. Too much or too little oxygen would have trapped or lost these elements. The finding highlights a chemical 'Goldilocks zone' critical for habitability.

Scientists have found that the 2022 eruption of an underwater volcano in the South Pacific triggered a chemical process that removed significant amounts of methane from the atmosphere. The discovery, detailed in a new study, shows how volcanic ash and seawater combined to break down the potent greenhouse gas.

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University of Utah researchers report that iron-rich hemozoin crystals inside the malaria parasite Plasmodium falciparum move through the parasite’s digestive compartment because reactions involving hydrogen peroxide at the crystal surface generate chemical propulsion. The work, published in Proceedings of the National Academy of Sciences, links a long-observed phenomenon to peroxide chemistry and could point to new antimalarial drug strategies and ideas for engineered micro- and nanoscale devices.

New research indicates that hidden oceans on icy moons around outer planets may boil due to tidal heating, explaining unusual surface features. The study, published in Nature Astronomy, focuses on smaller moons like Enceladus, Mimas, and Miranda. Lead author Max Rudolph from UC Davis highlights the processes shaping these worlds over millions of years.

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Researchers at Michigan State University have developed a computer simulation showing that gravitational collapse can naturally produce double-lobed, snowman-like structures in the outer solar system. These contact binaries make up about 10 percent of planetesimals in the Kuiper Belt beyond Neptune. The findings, published in the Monthly Notices of the Royal Astronomical Society, explain a long-standing puzzle in astronomy.

 

 

 

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