for National Geographic News
Science has a better understanding of how and when the moon came to be thanks to a team of German geochemists who compared ratios of trace elements in rocks from the Earth, the moon, Mars, and meteorites.
Most astronomers subscribe to the so-called "cratering" theory to explain the moon's creation: Billions of years ago, a Mars-sized body slammed into Earth, projecting a mixture of rocky debris into space, some of which lumped together to form the moon. The remaining debris rained back down on Earth.
But until recently, scientists debated how much lunar material originally came from the Earth and how much came from the celestial body that impacted it. Estimates ranged from 1 to 90 percent.
The rock comparison work of Carsten Münker, a geochemist at Germany's University of Münster, and his colleagues places the upper limit of impactor material at 65 percent. Their work also dates the moon to be at least 4.53 billion years old.
Jay Melosh, a geophysicist at the University of Arizona in Tucson and an expert on the impact-origin theory of the moon, said the limit on the amount of impactor material in the moon proposed by Münker and colleagues is reasonable.
"It will generate more smiles among the cratering community than gasps of horror," he said. Melosh said the German research team's estimates syncs up with that of another researcher team that has yet to be published.
The research by Münker and colleagues appeared in the July 4 issue of Science, the research journal of the American Association for the Advancement of Science, based in Washington, D.C.
The German geochemists' findings are based on an analysis of the ratio of the elements niobium to tantalum. Niobium is a metal commonly found in alloy steels. Tantalum is a metal resistant to acid corrosion commonly used in chemical, dental, and surgical instruments.
Both niobium and tantalum are nearly geochemical twins in magmatic systems like Earth's core, where the elements are barely separated from each other, said Münker. As such, scientists thought that Earth and moon shared the same niobium to tantalum ratio.
Recent studies have shown that niobium is attracted to iron at high pressures. Tantalum is not. When the Earth's iron core separated from our planet's rocky mantle, high pressure caused by Earth's gravity caused the two metals to separate, with the niobium going to the iron core.
Analysis of rock samples by scientists lead them to believe that the only instance when pressures would be large enough to force such a separation between the elements niobium and tantalum is at the time when the Earth formed. Other celestial bodies, such as the moon, Mars, and meteorites are too small to generate such high gravitational pressure.
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