Findings confirm that adding UV light helps to form guanine of RNA

Atlanta-- In attempting to understand the origin of the building blocks of RNA, one of the four bases of RNA — guanine (G) — has proven to be a particular challenge. While the other three bases of RNA — adenine (A), cytosine (C) and uracil (U) — could be created by heating a simple precursor compound in the presence of certain naturally occurring catalysts, guanine had not been observed as a product of the same reactions. By adding ultraviolet (UV) light to a model prebiotic reaction, researchers from the Georgia Institute of Technology and Sapienza University have discovered a route that could have formed the missing guanine.

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Atlanta-- In attempting to understand the origin of the building blocks of RNA, one of the four bases of RNA — guanine (G) — has proven to be a particular challenge. While the other three bases of RNA — adenine (A), cytosine (C) and uracil (U) — could be created by heating a simple precursor compound in the presence of certain naturally occurring catalysts, guanine had not been observed as a product of the same reactions. By adding ultraviolet (UV) light to a model prebiotic reaction, researchers from the Georgia Institute of Technology and Sapienza University have discovered a route that could have formed the missing guanine.

Recent efforts to understand the prebiotic formation of the building blocks of RNA have focused on the chemical formamide (H2NCOH) as a potential starting material to create the RNA bases because it contains the four required elements — carbon, hydrogen, oxygen and nitrogen — and because of its stability, reactivity and low volatility compared to water. Previous reports have shown that these nucleic acid components — with the exception of guanine — can be synthesized by heating formamide to 160°C in the presence of mineral catalysts.

The findings were reported in the June 14 issue of the journal ChemBioChem. This collaborative work is supported by the National Science Foundation (NSF), the National Aeronautics and Space Administration and the European Space Agency. The NSF funding is provided through the Center for Chemical Evolution at Georgia Tech. In their ChemBioChem paper, the researchers show for the first time that guanine can be produced by subjecting a solution of formamide to UV radiation during heating. The trace guanine yield was greatly enhanced when minerals and photons were used together. In addition, production of adenine and a related molecule called hypoxanthine increased when UV light was added to the heating process — a 15-fold increase was seen in adenine yield.

“These results potentially relax some of the requirements and reactions necessary to get life started, because formamide molecules would not have had to be in contact with a particular type of rock when heated on the prebiotic Earth, if the formamide was exposed to direct sunlight during heating,” said Nicholas Hud, a professor in the Georgia Tech School of Chemistry and Biochemistry.

The study demonstrated that guanine, adenine and hypoxanthine can be produced at lower temperatures than previously reported, even in the absence of minerals, as long as photons are added.

“For these experiments, we built a very simple reaction chamber with an inexpensive 254-nm photon source to simulate conditions that could have been present on early Earth,” explained Thomas Orlando, also a professor in Georgia Tech’s School of Chemistry and Biochemistry. “We didn’t need extremely sophisticated experimental systems or expensive lasers; however, we did use sophisticated mass spectrometers to analyze the resulting complex chemical mixtures.”

Georgia Tech and Sapienza University researchers showed for the first time that guanine can be produced by subjecting a solution of formamide to ultraviolet radiation during heating. Their study also demonstrated that guanine, adenine and hypoxanthine can be produced at lower temperatures than previously reported, even in the absence of minerals, as long as photons are added. (Image courtesy Gary Meek)

The Hud and Orlando laboratories conducted experiments by heating formamide to 130°C — 30 degrees cooler than previous experiments — and shining UV light onto it.

The authors suggest that aqueous pools containing small amounts of formamide may have existed on the early Earth. During hot and dry periods, water evaporation could have given rise to concentrated solutions of formamide and exposed mineral surfaces coated with formamide. By conducting additional experiments at 100°C with solutions of formamide and water, the researchers confirmed that this “drying pool” model could give rise to solutions of formamide capable of producing the compounds found in their earlier experiments.

“While there is still a lot of chemistry required for us to better understand the formation of biological molecules needed for life, these one-pot reactions that occur due to the synergy of thermal and photochemical processes tell us that the chemical and environmental requirements to produce life are probably less restrictive than we once thought,” added Hud.

Sapienza University professor of molecular biology Ernesto Di Mauro, and Georgia Tech chemistry graduate students Hannah Barks and Ragan Buckley and research scientist Gregory Grieves also contributed to this work.

This project is supported by the National Science Foundation (NSF) (Award No. CHE-0739189) and the National Aeronautics and Space Administration (NASA) (Award Nos. NNG05GP20G and NNX08AO14G).

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