In a new analysis of a lunar model collected by Apollo 17, researchers have detected and dated carbon on the moon in the form of graphite -- the sooty stuff of pencil lead which survived from around 3.8 billion years ago, when the moon was greatly bombarded by meteorites. Up to now, scientists thought the trace amounts of carbon formerly detected on the surface of the moon came from the solar wind.

Some of the graphite exposed by the new study appeared in a rare rolled form known as "graphite whiskers," which scientists consider formed in the very high-temperature reactions initiated by a meteorite impact. The discovery also means that the moon potentially holds a record of the carbon input by meteors into the Earth-moon system when life was just beginning to appear on Earth. The research is published in the July 2 concern of the journal Science.

"The solar system was chaotic, with countless colliding objects 3.9 billion years ago," explained lead author Andrew Steele, based at the Carnegie Institution for Science in Washington, D.C. "Volatiles -- compounds like water and rudiments like carbon were vaporized under that heat and shock. These materials were critical to the creation of life on Earth."

"Materials that fell on the early Earth fell on the moon as well, because the two bodies essentially share the same gravity well," said Marc Fries, a planetary scientist who conducted the research while working at NASA's Jet Propulsion Laboratory, Pasadena, Calif., and is now based at the Planetary Science Institute in Tucson, Ariz. "This sample is like a immaculate page from Earth's past, before plate tectonics and other forces erased the history of this ancient carbon material on Earth."

While the sample from the Mare Serenitatis area came back to Earth in 1972, the research team, led by scientists at the Geophysical Laboratory of the Carnegie Institution for Science, used a innovative technique known as Raman spectroscopy on the sample. Previous techniques enabled scientists to get a sense of the composition, but this kind of spectroscopy is more sensitive and also allows scientists to produce an image of the minerals. The graphite whiskers appeared to be a few micrometers in diameter and up to about 10 microns long.

Scientists were astonished at the finding of graphite and graphite whiskers.

"It shows that modern spatially determined techniques could be used to discover further surprises in the now 40-year-old Apollo collection," said co-author Mihaela Glamoclija, based at the Carnegie Institution.

The scientists ruled out the opportunity that the graphite was a result of contamination, because graphite whiskers, in particular, form under very hot conditions, between 1,830 and 6,500 degrees Fahrenheit (1,273 to 3,900 Kelvin). They also ruled out the solar wind as the source, because the graphite and graphite whiskers were much superior to carbon implanted by the solar wind, and while contamination occurred throughout the sample, the graphite was restricted to a discrete blackened area of the sample.

"We believe that the carbon we detected either came from the object that made the impact basin, or it strong from the carbon-rich gas that was released during impact," said co-author Francis McCubbin, of the Carnegie Institution.

The research was partly funded by the NASA Astrobiology, Mars Fundamental Research, and the Lunar Advanced Science and Exploration Research programs in NASA's Planetary Division in Washington. The California Institute of Technology manages JPL for NASA.

For More Information Visit http://www.jpl.nasa.gov/news/news.cfm?release=2010-220

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