Astronomers have found a friendly molecule in deep space.
New research shows how a simple molecule called ortho-benzene helps form more complex organic molecules deep inside a frigid gas cloud. The team says it plays a small but critical role in creating chemically rich building blocks that will eons later form young stars and planets.
In the last few years, astronomers have discovered a bunch of complex organic molecules in rapid succession inside the dense Taurus Molecular Cloud-1 (TMC-1), which is a stellar nursery in the constellation Taurus located some 440 light-years from Earth.
Forming large molecules requires heat, which is in short supply in TMC-1. The cloud’s temperatures dip as low as minus 440 degrees Fahrenheit (minus 263 degrees Celsius), so astronomers have struggled to explain how complex molecules with lengthy names like 1-ethynyl cyclopentadiene came to be in the gas cloud in surprising abundance.
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“Researchers kept detecting these molecules in TMC-1, but their origin was unclear,” study lead author Jordy Bouwman, a cosmochemist and professor at the University of Colorado Boulder, said in a statement (opens in new tab).
Now, research by Bouwman’s team found that ortho-benzene, which was discovered inside TMC-1 only in August 2021, drives complex chemical reactions and is at least partly responsible for the presence of large molecules inside the gas cloud.
Unlike most elements, researchers say ortho-benzene is one of the “extroverts of the chemistry world” because it does not require a lot of heat for chemical reactions, so it bonds easily with other molecules. This way, it serves a critical role in improving the chemical complexity of cold stellar nurseries like TMC-1.
“We’re only at the start of truly understanding how we go from these small building blocks to larger molecules,” Bouwman said in the same statement. “I think we’ll find that this chemistry is so much more complex than we thought, even at the earliest stages of star formation.”
The team made the new observations using a technique (also with a lengthy name) called photoelectron photoion coincidence spectroscopy. Essentially, the process allowed researchers to learn the outcomes of various chemical reactions, and they found that ortho-benzene and methyl radicals — another frequent sighting in molecular clouds — can easily combine to form larger, more complex organic compounds.
Currently, there are two leading theories about how abundant hydrocarbons and other ringed compounds materialized in gas clouds. One posits that carbon-bearing molecules called polycyclic aromatic hydrocarbons (PAHs) — which are thought to be important precursors to more complex molecules — were inherited and broken down from earlier stages of cloud evolution. The second theory suggests that large molecules built up in-situ from smaller, simpler elements. The latest findings add evidence for the latter idea, researchers say.
Bouwman’s team used an astrochemical model to see how ortho-benzene reactions form bigger molecules (like those with long names) in deep space. They simulated reactions happening in TMC-1 by plugging in the amounts of different elements gathered from recent observations targeting the gas cloud.
According to the study, these simulations with ortho-benzene as the prime candidate were an “excellent reproduction” of complex compounds like 1-ethynyl cyclopentadiene, and in similar concentrations spotted by astronomers in TMC-1 using telescopes.
“Our findings may just change the view on what ingredients we have in the first place to form new stars and new planets,” Bouwman said.
The research is described in a paper (opens in new tab) published Feb. 6 in the journal Nature Astronomy.
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