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Ancient proteins offer new clues about origin of life on Earth

By simulating early Earth conditions in the lab, researchers have found that without specific amino acids, ancient proteins would not have known how to evolve into everything alive on the planet today — including plants, animals, and humans.

The findings, which detail how amino acids shaped the genetic code of ancient microorganisms, shed light on the mystery of how life began on Earth.

“You see the same amino acids in every organism, from humans to bacteria to archaea, and that’s because all things on Earth are connected through this tree of life that has an origin, an organism that was the ancestor to all living things,” said Stephen Fried, a Johns Hopkins chemist who co-led the research with scientists at Charles University in the Czech Republic. “We’re describing the events that shaped why that ancestor got the amino acids that it did.”

The findings are newly published in the Journal of the American Chemical Society.

In the lab, the researchers mimicked primordial protein synthesis of 4 billion years ago by using an alternative set of amino acids that were highly abundant before life arose on Earth.

They found ancient organic compounds integrated the amino acids best suited for protein folding into their biochemistry. In other words, life thrived on Earth not just because some amino acids were available and easy to make in ancient habitats but because some of them were especially good at helping proteins adopt specific shapes to perform crucial functions.

“Protein folding was basically allowing us to do evolution before there was even life on our planet,” Fried said. “You could have evolution before you had biology, you could have natural selection for the chemicals that are useful for life even before there was DNA.”

Even though the primordial Earth had hundreds of amino acids, all living things use the same 20 of these compounds. Fried calls those compounds “canonical.” But science has struggled to pinpoint what’s so special — if anything — about those 20 amino acids.

In its first billion years, Earth’s atmosphere consisted of an assortment of gases like ammonia and carbon dioxide that reacted with high levels of ultraviolet radiation to concoct some of the simpler canonical amino acids. Others arrived via special delivery by meteorites, which introduced a mixed bag of ingredients that helped life on Earth complete a set of 10 “early” amino acids.

How the rest came to be is an open question that Fried’s team is trying to answer with the new research, especially because those space rocks brought much more than the “modern” amino acids.

“We’re trying to find out what was so special about our canonical amino acids,” Fried said. “Were they selected for any particular reason?”

Scientists estimate Earth is 4.6 billion years old, and that DNA, proteins, and other molecules didn’t begin to form simple organisms until 3.8 billion years ago. The new research offers new clues into the mystery of what happened during the time in between.

“To have evolution in the Darwinian sense, you need to have this whole sophisticated way of turning genetic molecules like DNA and RNA into proteins. But replicating DNA also requires proteins, so we have a chicken-and-egg problem,” Fried said. “Our research shows that nature could have selected for building blocks with useful properties before Darwinian evolution.”

Scientists have spotted amino acids in asteroids far from Earth, suggesting those compounds are ubiquitous in other corners of the universe. That’s why Fried thinks the new research could also have implications for the possibility of finding life beyond Earth.

“The universe seems to love amino acids,” Fried said. “Maybe if we found life on a different planet, it wouldn’t be that different.”

This research is supported by the Human Frontier Science Program grant HFSP-RGY0074/2019 and the NIH Director’s New Innovator Award (DP2-GM140926).

Authors include Anneliese M. Faustino, of Johns Hopkins; Mikhail Makarov, Alma C. Sanchez Rocha, Ivan Cherepashuk, Robin Krystufek, and Klara Hlouchova, of Charles University; Volha Dzmitruk, Tatsiana Charnavets, and Michal Lebl, of the Czech Academy of Sciences; and Kosuke Fujishima, of Tokyo Institute of Technology.

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