How many different molecules can be created when you release one of the universe's most reactive substances, hydrogen cyanide, in the lab? A question scientists are asking because hydrogen cyanide seems to have played a role in creating some of life's building blocks. Hydrogen cyanide is an organic compound and it is found in large quantities in the universe. It may have helped in producing amino acids and DNA bases, some of life's basic molecules. If hydrogen cyanide can lead to the formation of amino acids, can it also contribute to the formation of other essential compounds? Can hydrogen cyanide help explain how life originated on Earth? And how it can arise on other planets?
"Chemical reactions can be organized into a self-replicating system, a so-called autocatalytic cycle. Being able to copy itself is one of life's most basic characteristics, so for us who study the origin of life, there is obviously great interest in exploring what it takes for a chemical reaction to copy itself. So far the identification of these cycles has been much more complicated", explains Martin Hanczyc, who will present the work at the European Conference on Artificial Life in Taormina, Italy this week.
Preliminary studies have shown that hydrogen cyanide can contribute to the formation of amino acids. This discovery required month-long experiments in the laboratory, where scientists painstakingly monitored the reactions and continuously manipulated the experiment to keep it on track.
According to associate professor Daniel Merkle at the Department of Mathematics and Computer Science a novel approach can in a matter of hours or a day spot all the thousands of different molecules that can be formed during the reaction of hydrogen cyanide in the laboratory - even if the experiment has not been manipulated along the way and is allowed to evolve chaotically.
When Hanczyc and Merkle tested their methods on a hydrogen cyanide reaction in the laboratory they found that many of the molecules that had previously been identified as particularly interesting – for example the DNA base adenine, was automatically discovered.
"In our study we found that our approaches identified the right molecules. This confirms to us that these novel methods can be used as an effective and reliable tool in chemical analyzes in the future", says Hanczyc.
The composite image above from NASA's Spitzer Space Telescope and NASA's Chandra X-ray Observatory shows the remnant of one such explosion. The remnant, called N132D, is the wispy pink shell of gas at the center of this image. The pinkish color reveals a clash between the explosion's high-energy shockwaves and surrounding dust grains. In the background, small organic molecules called polycyclic aromatic hydrocarbons are shown as tints of green. The blue spots represent stars in our galaxy along this line of sight. N132D is located 163,000 light-years away in a neighboring galaxy called, the Large Magellanic Cloud.
The Daily Galaxy via University of Southern Denmark
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