Nav: Home

Method of tracking reactions between air and carbon-based compounds established

February 26, 2018

By being the first to fully track the changing chemistry of carbon molecules in the air, a Virginia Tech professor could change the way we study pollutants, smog, and emissions to the atmosphere.

Gabriel Isaacman-VanWertz, lead scientist on a new study published in Nature Chemistry and assistant professor in Virginia Tech's department of civil and environmental engineering, has established a method of tracking reactions between air and carbon-based compounds -- a feat that has been previously elusive to researchers.

This new finding could allow researchers to study pollution, smog, and haze in a comprehensive way, backed by data that accurately depicts a compound's behavior over time.

"There are tens of thousands of different compounds in the atmosphere," Isaacman-VanWertz said. "In general, the focus of my work is to study the chemistry of how those tens of thousands of compounds interact with each other and change with time."

When a certain compound is introduced into the atmosphere, it chemically reacts to form other compounds and molecules over time, explains Isaacman-VanWertz, who began this research as a post-doctoral research fellow at the Massachusetts Institute of Technology with study co-author Jesse Kroll.

Isaacman-VanWertz is particularly focused on studying the way the atmosphere interacts with organic compounds -- the carbon-containing compounds that make up all living things. Large amounts of these compounds are emitted from natural sources and human activities.

Anything with a scent emits organic compounds: citrus, vinegar, nail polish remover, and gasoline, for example. Once these emitted compounds enter the atmosphere, they change in complex ways to form hundreds or thousands of other compounds.

Previously, tracking the way the carbon changes once it enters the atmosphere has been a challenge. Thanks to tools developed in the past decade, this study found that complete measurement of carbon in the atmosphere is now possible, though it still requires state-of-the-art instruments and careful analysis.

For this project, Isaacman-VanWertz studied the smell of pine, which is made of an organic compound known as pinene.

Isaacman-VanWertz and his collaborators at MIT used five spectrometers -- advanced pieces of equipment that classify chemicals by their masses and the atoms they contain -- to measure the characteristics of carbon inside a Teflon bag the height of a person in a climate-controlled, blacklight-outfitted room.

When they turned on the blacklights, it was like turning on the sun, Isaacman-VanWertz said. The light of the "sun" spurred the chemistry of the pinene inside the chamber and simulated the reactions that would occur in the atmosphere.

Each spectrometer was tasked with collecting a certain set of data throughout the elapsed reaction, like tracking specific ranges of chemical compounds. One of the hardest parts of this experiment was putting all of these measurements on the same scale, Isaacman-VanWertz said. Understanding the specific details and measurements of each instrument can be so complex, he said, there are doctoral students writing entire theses on these topics.

Isaacman-VanWertz and his collaborators were able to, for the first time, fully track the carbon in the pinene molecules from start to finish as they underwent chemical changes as they would in the atmosphere. The carbon atoms in pinene do not disappear after their initial introduction to the atmosphere -- they turn into hundreds of different compounds through a cascade of chemical reactions.

Although the initial mixture of compounds formed from reactions of pinene is very complex, all the carbon was found to end up in "reservoirs" that are relatively stable and won't react further in the atmosphere.

What's more, the process is likely similar for other carbon-based compounds. Isaacman-VanWertz picked pinene because it has been extensively studied, so he could use previous work to make sense of his observations.

Though pinene is naturally emitted, its behavior is comparable enough to better anticipate the way other compounds, like those in pollutants, smog, and haze, will react in the air. Understanding this helps "paint a big picture of the atmosphere," Isaacman-VanWertz said.

For example, these results will help other researchers understand how pollutants from a power plant might transform in the atmosphere and impact a downwind community.

"If you can understand how the chemistry happens, then you can understand what sorts of pollutants will be in the atmosphere based on how far from a polluting source you are," Isaacman-VanWertz explained.

Isaacman-VanWertz hopes other researchers will build upon the results of this study. He wants to know whether the tendency of emitted compounds to end up as long-lived atmospheric components is generally applicable to other compounds and how this process might coexist or compete with other processes occurring in the atmosphere.
-end-


Virginia Tech

Related Atmosphere Articles:

Physics: An ultrafast glimpse of the photochemistry of the atmosphere
Researchers at Ludwig-Maximilians-Universitaet (LMU) in Munich have explored the initial consequences of the interaction of light with molecules on the surface of nanoscopic aerosols.
Using lasers to visualize molecular mysteries in our atmosphere
Molecular interactions between gases and liquids underpin much of our lives, but difficulties in measuring gas-liquid collisions have so far prevented the fundamental exploration of these processes.
The atmosphere of a new ultra hot Jupiter is analyzed
The combination of observations made with the CARMENES spectrograph on the 3.5m telescope at Calar Alto Observatory (Almería), and the HARPS-N spectrograph on the National Galileo Telescope (TNG) at the Roque de los Muchachos Observatory (Garafía, La Palma) has enabled a team from the Instituto de Astrofísica de Canarias (IAC) and from the University of La Laguna (ULL) to reveal new details about this extrasolar planet, which has a surface temperature of around 2000 K.
An exoplanet loses its atmosphere in the form of a tail
A new study, led by scientists from the Instituto de Astrofísica de Canarias (IAC), reveals that the giant exoplanet WASP-69b carries a comet-like tail made up of helium particles escaping from its gravitational field propelled by the ultraviolet radiation of its star.
Iron and titanium in the atmosphere of an exoplanet
Exoplanets can orbit close to their host star. When the host star is much hotter than our sun, then the exoplanet becomes as hot as a star.
More Atmosphere News and Atmosphere Current Events

Best Science Podcasts 2019

We have hand picked the best science podcasts for 2019. Sit back and enjoy new science podcasts updated daily from your favorite science news services and scientists.
Now Playing: TED Radio Hour

Erasing The Stigma
Many of us either cope with mental illness or know someone who does. But we still have a hard time talking about it. This hour, TED speakers explore ways to push past — and even erase — the stigma. Guests include musician and comedian Jordan Raskopoulos, neuroscientist and psychiatrist Thomas Insel, psychiatrist Dixon Chibanda, anxiety and depression researcher Olivia Remes, and entrepreneur Sangu Delle.
Now Playing: Science for the People

#537 Science Journalism, Hold the Hype
Everyone's seen a piece of science getting over-exaggerated in the media. Most people would be quick to blame journalists and big media for getting in wrong. In many cases, you'd be right. But there's other sources of hype in science journalism. and one of them can be found in the humble, and little-known press release. We're talking with Chris Chambers about doing science about science journalism, and where the hype creeps in. Related links: The association between exaggeration in health related science news and academic press releases: retrospective observational study Claims of causality in health news: a randomised trial This...