In the 1950s, biochemist Stanley Miller performed a series of experiments to demonstrate that organic compounds could be created under conditions mimicking the primordial Earth. Some unused samples from Miller’s research were recently uncovered by a team of scientists, including Jim Cleaves, of Carnegie’s Geophysical Laboratory. Their findings, carried out using modern techniques and published online March 21 by Proceedings of the National Academy of Sciences, indicate the possible importance of volcanoes and sulfur in the formation of amino acids, and possibly life, on Earth.
Miller’s experiments were the first to demonstrate that subjecting hydrogen-rich gases to an electric spark could create the basic molecules of life. The set of samples used in this research was created in 1958.
In the years since Miller’s initial experiments, scientists have come to believe that the atmosphere of primitive Earth wasn’t made up of the same gases that he used in his initial study. But volcanic eruptions were likely very common during the early history of the planet and these volcanoes could have emitted clouds rich in hydrogen, methane and H2S, which would create conditions similar to Miller’s experiments in limited geographic areas. The spark could have been supplied by lightning, which is commonly associated with volcanic clouds.
“Preserved samples from one of Miller’s experiments in 1958 using hydrogen sulfide were found in his archived collection. They had been collected, catalogued, and stored, but never analyzed,” Cleaves said. “The techniques he used in the 1950s were only capable of detecting a few amino acids, but today’s equipment is much more sophisticated.”
The team was able to identify 23 types of amino acid, some of which are the building blocks of proteins and necessary for life, including the sulfur-containing amino acid methionine, as well as four other types of organic compounds known as amines. The structures of several of the amino acids indicate that they were clearly synthesized in the experiment and not contaminants, although traces of contamination from fifty years of storage were also evident. The results showed the first known synthesis of sulfur-containing amino acids using the spark method developed by Miller.
The team checked their work by comparing the amino acids created by Miller in the presence of hydrogen sulfide, to organic compounds found in carbonaceous chondrites, a type of organic-rich meteorite. They found the greatest similarity between the experiments with H2S and the carbonaceous chondrites, indicating that hydrogen sulfide may have played a role in the creation of the meteorite amino acids.
“Our results demonstrate the earliest example of the synthesis of sulfur-containing organic compounds in an experiment to mimic primitive Earth conditions,” Cleaves said.
For copies of the papers, contact the PNAS news office at pnasnews@nas.edu or +202-334-1310, or contact the author.
The Mandeville Special Collections in the University of California, San Diego, Geisel Library provided assistance with archiving and retrieving Miller’s original laboratory notebooks. Funding support was provided by the NASA Astrobiology Institute and the Goddard Center for Astrobiology. Some of the researchers were supported by the NASA Postdoctoral Program administered by Oak Ridge Associated Universities. Assistance with data analysis and figure preparation was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
The Carnegie Institution for Science (http://carnegiescience.edu) is a private, nonprofit organization headquartered in Washington, D.C., with six research departments throughout the U.S. Since its founding in 1902, the Carnegie Institution has been a pioneering force in basic scientific research. Carnegie scientists are leaders in plant biology, developmental biology, astronomy, materials science, global ecology, and Earth and planetary science.
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