A New Way to Analyze Ancient Atmospheres
Their discovery also provides a simple chemical explanation for the unusual carbonate inclusions found in a meteorite from Mars that was once thought by some scientists to be evidence of ancient martian life.
“We never knew before how the atmosphere could be trapped in carbonate,” said Mark Thiemens, dean of UC San Diego’s Division of Physical Sciences who headed the team of scientists that detailed its discovery in this week’s early online edition of the Journal of the Proceedings of the National Academy of Sciences. “This chemical reaction, which takes place on the surface of aerosols in the atmosphere, not only provides us with an understanding of how these carbonates can form on the Earth and Mars. It gives us a new tool to better understand climate change, as our planet warms and becomes more dusty.”
Robina Shaheen, a postdoctoral researcher in Thiemens’ laboratory, discovered the chemical reaction and detailed its importance in the Earth’s atmosphere after four years of painstaking experiments in which she found a higher than expected proportion of oxygen 17 isotopes in the carbonates found on dust grains, aerosols and dirt from various parts of the world.
Martian meteorites, such as ALH84001, which was once thought to exhibit evidence of extraterrestrial life, have carbonates with similarly high oxygen 17 anomalies. Scientists have long attributed those anomalies to photochemical processes involving ozone and carbon dioxide in the thin atmosphere on Mars, which is bathed by intense ultraviolet radiation. But after finding similar anomalies on terrestrial carbonates formed in atmospheric aerosols, Shaheen surmised they might be the result of another chemical process more common to both planets.
“What she found is that the tiny little layer on the outside of the grain is where this chemistry all happens,” said Thiemens. “It’s the ozone in the atmosphere mixing with water and carbon dioxide that drives a completely different kind of chemistry, one that’s not in any of the models.”
While current models of atmospheric processes assume that the mixing of large volumes of gases drives the chemistry of the Earth’s atmosphere, the UCSD chemists think their discovery may force a rethinking of this idea, particularly as the Earth’s atmosphere becomes warmer and more dusty, providing more opportunities for this sort of chemistry to take place on aerosols.
“You can do chemistry on a grain that’s a lot quicker and easier in many respects than is possible in other atmospheric processes,” said Thiemens.
Shaheen, who analyzed the carbonates in the martian meteorite ALH84001 and found that they could have been formed on aerosols in ancient martian atmosphere, said that NASA’s Phoenix lander recently detected carbonates associated with particulates in the dusty atmosphere of Mars. “We think it might be this same mechanism that is operating,” she added.
“We’ve found a new way to measure the Earth’s atmosphere for time periods when we previously could not do it,” said Thiemens. “What happened to ozone and oxygen levels 65 million years ago during the Cretaceous-Tertiary period when the dinosaurs and many other forms of life were killed in a mass extinction? Who died first? Did the food chain disappear before the dinosaurs? What happened 251 million years ago during the Permian-Triassic period, the most severe extinction of life on Earth, when 85 percent of life disappeared and no one knows why? There’s no record of what happened in the atmosphere. But if you can find a record of what happened to oxygen levels, you can answer questions like that.”
Other researchers at UCSD involved in the study in Thiemens’ laboratory were undergraduates Anna Abramian and John Horn. The research was partially supported by grants from National Aeronautics and Space Administration, the National Science Foundation and the UC San Diego Chancellor’s Associates.