August 12, 2008
Strange molecule in the sky cleans acid rain, scientists discoverWEST LAFAYETTE, Ind. -
It's the unusual chemistry facilitated by this molecule, however, that will attract the most attention from scientists.
Marsha Lester, the University of Pennsylvania's Edmund J. Kahn Distinguished Professor, and Joseph Francisco, William E. Moore Distinguished Professor of Chemistry at Purdue University, found the molecule, which had puzzled and eluded scientists for more than 40 years.
A technical paper describing the molecule is published this week in a special edition of the Proceedings of the National Academy of Science.
Somewhat like a human body metabolizing food, the Earth's atmosphere has the ability to "burn," or oxidize pollutants, especially nitric oxides emitted from sources such as factories and automobiles. What doesn't get oxidized in the atmosphere falls back to Earth in the form of acid rain.
"The chemical details of how the atmosphere removes nitric acid have not been clear," Francisco says. "This gives us important insights into this process. Without that knowledge we really can't understand the conditions under which nitric acid is removed from the atmosphere."
Francisco says the discovery will allow scientists to better model how pollutants react in the atmosphere and to predict potential outcomes.
"This becomes important in emerging industrial nations such as China, India and Brazil where there are automobiles and factories that are unregulated," Francisco says. "This chemistry will give us insight into the extent that acid rain will be a future concern."
Lester says the molecule had been theorized by atmospheric chemists for 40 years and that she and Francisco had pursued it for the past several years.
"We've speculated about this unusual atmospheric species for many years, and then to actually see it and learn about its properties was very exciting," she says.
What makes the molecule so unusual is its two hydrogen bonds, which are similar to those found in water.
Chemists know that although water is one of the most common substances found on the planet, it has unusual properties. For example, the solid form - ice - is lighter than the liquid form and floats. Water also boils at a much higher temperature than would be expected from its chemical structure.
The cause of these strange behaviors are weak hydrogen bonds that hold water molecules together.
The new atmospheric molecule has two hydrogen bonds, which allows it to form a six-sided ring structure. Hydrogen bonds are usually weaker than the normal bonds between atoms in a molecule, which are known as covalent bonds. In fact, covalent bonds are 20 times stronger than hydrogen bonds. But in this case, these two hydrogen bonds are strong enough to affect atmospheric chemistry, Francisco says.
Lester says the new molecule exhibits its own unusual properties.
"The reaction involving this molecule proceeds faster as you go to lower temperatures, which is the opposite of most chemical reactions," she says. "The rate of reaction also changes depending on the atmospheric pressure, and most reactions don't depend on external pressure. The molecule also exhibits unusual quantum properties."
Lester says the unusual properties prevented scientists from being able to model the reaction for so long.
"This is not how we explain chemistry to high school students," she says.
Francisco says that this discovery will be used in areas other than atmospheric chemistry.
"Here's a situation where we were studying this purely environmental problem, but, because the findings are so fundamental, it may have broader ramifications to biological systems that depend on hydrogen bonds," he says.
The breakthrough was enabled by laser-based laboratory techniques at the University of Pennsylvania and the supercomputing resources available at Purdue, Francisco says. The computation was done on an SGI Altix supercomputer operated by the Office of Information Technology at Purdue.
"The key is knowing where to look and how to identify new chemical entities, and with the computing resources we have at Purdue we can help identify processes to within experimental uncertainty," he says. "We couldn't have done this without the supercomputing power that we have available."
Writer: Steve Tally, (765) 494-9809, email@example.com
Sources: Joseph Francisco, (765) 494-7851, firstname.lastname@example.org
Marsha Lester, (215) 898-4640, email@example.com
Purdue News Service: (765) 494-2096; firstname.lastname@example.org
Note to Journalists: The citation for the PNAS paper is Bridget A. O'Donnell, Eunice X. J. Li, Marsha I. Lester and Joseph S. Francisco Special Feature: Spectroscopic identification and stability of the intermediate in the OH + HONO2 reaction, doi:10.1073/pnas.0800320105. A copy is available from Steve Tally, (765) 494-9809, email@example.com
A publication-quality image is available at http://news.uns.purdue.edu/images/+2008/ozonemodel.jpg
Spectroscopic Identification and Stability of the Intermediate in OH + HONO2 Reaction
Bridget A. O'Donnell, Eunice X.J. Li*, and Marsha Lester, Dept. of Chemistry, University of Pennsylvania, Philadelphia, PA 19104-6323Joseph S. Francisco, Dept. of Chemistry, Purdue University, West Lafayette, IN 47907-2084
The reaction of nitric acid with the hydroxyl radical controls the residence time of HONO2 in the lower atmosphere. Prior studies [Brown, S.S., Burkholder, J.B., Talukdar, R.K., & Ravishankara, A.R. (2001) Reaction of hydroxyl radical with nitric acid: Insights into its mechanism. J. Phys. Chem. A 105, 1605-1614] have revealed unusual kinetic behavior for this reaction including negative temperature dependence, pressure dependence, and an overall reaction rate strong affected by isotopic substitution. This suggested that the reaction occurs through an intermediate, theoretically predicted to be a hydrogen-bonded OH-HONO2 complex in a six-membered ringlike configuration. In this study, the intermediate is generated directly by the association of photolytically generated OH radicals with HONO2 and stabilized in a pulsed supersonic expansion. Infrared action spectroscopy is used to identify the intermediate via OH radical stretch (v1) and OH stretch of nitric acid (v2) in the OH-HONO2 complex. Two vibrational features are attributed to OH-HONO2: a rotationally structured v1 band at 3516.8 cm-1 and an extensively broadened v2 feature at 3260 cm-1, both shifted from their respective monomers. These same transitions are identified for OD-DONO2. Assignments of the features are based on their vibrational frequencies, analysis of rotational band structure, and comparison with complementary high level ab initio calculations. In addition, the OH (v=0) product state distributions resulting from v1 and v2 excitation are used to determine the binding energy of OH-HONO2, D0< 5.3 kcal mol-1, which is in good accord with ab initio predictions.
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