Meteorites key to the story of Earth's layers
The team measured the amount of the rare elements hafnium and lutetium in the mineral zircon in a meteorite that originated early in the solar system.
"Meteorites that contain zircons are rare. We had been looking for an old meteorite with large zircons, about 50 microns long, that contained enough hafnium for precise analysis," said Dr Yuri Amelin, from The Australian National University (ANU) Research School of Earth Sciences.
"By chance we found one for sale from a dealer. It was just what we wanted. We believe it originated from the asteroid Vesta, following a large impact that sent rock fragments on a course to Earth."
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Dr Yuri Amelin [Credit: Stuart Hay] |
Determining how and when the layers formed relies on knowing the composition of the original material that formed into the Earth, before differentiation, said Dr Amelin.
"Meteorites are remnants of the original pool of material that formed all the planets," he said.
"But they have not had planetary-scale forces changing their composition throughout their five billion years orbiting the sun."
The team accurately measured the ratio of the isotopes hafnium-176 and hafnium-177 in the meteorite, to give a starting point for the Earth's composition.
The team were then able to compare the results with the oldest rocks on Earth, and found that the chemical composition had already been altered, proving that a crust had already formed on the surface of the Earth around 4.5 billion years ago.
Source: Australian National University [April 13, 2015]
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