New findings challenge a theory that a meteor explosion or impact thousands of years ago caused catastrophic fires over much of North America and Europe and triggered an abrupt global cooling period, called the Younger Dryas. Whereas proponents of the theory have offered “carbonaceous spherules” and nanodiamonds — both of which they claimed were formed by intense heat — as evidence of the impact, a new study concludes that those supposed clues are nothing more than fossilized balls of fungus, charcoal, and fecal pellets. Moreover, these naturally-occurring organic materials, some of which had likely been subjected to normal cycles of wildfires, date from a period of thousands of years both before and after the time that the Younger Dryas period began — further suggesting that there was no sudden impact event.
“People get very excited about the idea of a major impact causing a catastrophic fire and the abrupt climate change in that period, but there just isn’t the evidence to support it,” says Andrew C. Scott of the Department of Earth Sciences at Royal Holloway, University of London, who led the research.
The findings by Scott and his colleagues have been accepted for publication in Geophysical Research Letters, a journal of the American Geophysical Union (AGU). The research team included scientists from England, Switzerland, and the United States.
The Younger Dryas impact event theory holds that a very large meteor struck Earth or exploded in the atmosphere about 12,900 years ago, causing a vast fire over most of North America, which contributed to extinctions of most of large animals on the continent and triggered a thousand-year-long cold period. While there is much previous evidence for the abrupt onset of a cooling period at that time, other researchers have theorized that the climatic change resulted from increased freshwater in the ocean, changes in ocean and atmospheric circulation patterns, or other causes unrelated to impacts.
The impact-theory proponents point to a charred layer of sediment filled with organic material that they say is unique to that period as evidence of such an event. These researchers described carbon spheres, carbon cylinders, and charcoal pieces that they conclude are melted and charred organic matter created in the intense heat of a widespread fire.
Scott and his fellow researchers analyzed sediment samples to determine the origins of the carbonaceous particles. After comparing the fossil particles with modern fungal ones exposed to low to moderate heat (less than 500 degrees Celsius, or 932 degrees Fahrenheit), Scott’s group concludes that the particles are actually balls of fungal material and other ordinary organic particles, such as fecal pellets from insects, plant or fungal galls, and wood, some of which may have been exposed to regularly-occurring low-intensity wildfires.
The researchers used microscopic analysis of particles from the Pleistocene-Holocene sediments collected from the California Channel Islands and compared them with modern soil samples that had been subjected to wildfires, as well as balls of stringy fungal material, called sclerotia, some of which were also subjected to a range of temperatures in a laboratory. Many soil and plant fungi produce sclerotia — tough balls of cells that are usually 0.5 millimeter to 2 millimeters in size (0.02 inch to 0.08 inch) — as a way to survive periods of harsh conditions. Their shape can vary from spherical to elongated, and their internal structures, which can take on a spongy or honeycomb pattern, matches the descriptions given by Dryas- impact event proponents.
Further, the group studied the amount of light reflected by the fossil spherules and wood charcoal from the sediment layers that included the Dryas period. The researchers used the reflectance of the organic material to determine the amount of heat to which it had been subjected. They found that the fossilized matter was unlikely to have been exposed to temperatures above 450 degrees Celsius (842 degrees Fahrenheit). Radiocarbon dating also showed that the particles, taken from several layers, ranged in age from 16,821 to 11,467 years ago. Proponents of the impact theory had reported that the spherules they found in the Younger Dryas sediment layer dated to a very narrow time period of 12,900 to 13,000 years before present.
“There is a long history of fire in the fossil record, and these fungal samples are common everywhere, from ancient times to the present,” Scott says. “These data support our conclusion that there wasn’t one single intense fire that triggered the onset of the cold period.”
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Funding for this research was provided by the National Geographic Society, the National Science Foundation, the Royal Society of London, the Royal Holloway strategy fund, the Natural Environmental Research Council, and the Integrated Infrastructure Initiative on Synchrotrons and Free Electron Lasers.
As of the date of this press release, the paper by Scott et al. is still “in press” (i.e., not yet published). Journalists and public information officers (PIOs) of educational and scientific institutions who have registered with AGU can download a PDF copy of this paper in press by clicking on this link: http://www.agu.org/journals/pip/gl/2010GL043345-pip.pdf
Or, you may order a copy of the paper by emailing your request to Kathleen O’Neil at koneil@agu.org. Please provide your name, the name of your publication, and your phone number.
Title: “Fungus, not comet or catastrophe, accounts for carbonaceous spherules in the Younger Dryas ‘impact layer'”
Authors: Andrew C. Scott and Margaret E. Collinson, Department of Earth Sciences, Royal Holloway University of London, Egham, UK Nicholas Pinter, Department of Geology, Southern Illinois University, Carbondale, Illinois Mark Hardiman, Department of Geography, Royal Holloway University of London, Department of Geography, Egham, Surrey, UK R. Scott Anderson, School of Earth Sciences & Environmental Sustainability, Northern Arizona University, Flagstaff, Arizona Anthony P.R. Brain, Centre for Ultrastructural Imaging, King’s College London, London, UK Selena Y. Smith, Museum of Paleontology and Department of Geological Sciences, University of Michigan, Ann Arbor, Michigan Federica Marone, Swiss Light Source, Paul Scherrer Institut, Villigen, Switzerland Marco Stampanoni, Swiss Light Source, Paul Scherrer Institut, Villigen, Switzerland; and Institute for Biomedical Engineering, University and ETH Zurich, Zurich, Switzerland
