April 4, 2012
New Isotope Measurement Could Alter History Of Early Solar System
The early days of our solar system might look quite different than previously thought, according to research at the U.S. Department of Energy´s (DOE) Argonne National Laboratory published in Science. The study used more sensitive instruments to find a different half-life for samarium, one of the isotopes used to chart the evolution of the solar system.
“It shrinks the chronology of early events in the solar system, like the formation of planets, into a shorter time span,” said Argonne physicist Michael Paul. “It also means some of the oldest rocks on Earth would have formed even earlier – as early as 120 million years after the solar system formed, in one case of Greenland rocks.”
According to current theory, everything in our solar system formed from star dust several billion years ago. Some of this dust was formed in giant supernovae explosions which supplied most of our heavy elements. One of these is the isotope samarium-146.
Samarium-146, or Sm-146, is unstable and occasionally emits a particle, which changes the atom into a different element. Using the same technique as radiocarbon dating, scientists can calculate how long it´s been since the Sm-146 was created. Because Sm-146 decays extremely slowly–on the order of millions of years–many models use it to help determine the age of the solar system.
The number of years it takes for an isotope to decrease by half is called its half-life. Since Sm-146 emits particles so rarely, it takes a sophisticated instrument to measure this half-life.
The Argonne Tandem Linac Accelerator System, or ATLAS, is a DOE national user facility for the study of nuclear structure and astrophysics, and is just such an instrument. “It´s easy for the ATLAS, used as a mass spectrometer, to pick out one Sm-146 atom in tens of billions of atoms,” said physicist Richard Pardo, who manages the facility and participated in the study.
By counting Sm-146 atoms with ATLAS and tracking the particles that the sample emits, the team came up with a new calculation for its half-life: just 68 million years.
This is significantly shorter than the previously used value of 103 million years.
The new value patches some holes in current understanding, according to Paul. “The new time scale now matches up with a recent, precise dating taken from a lunar rock, and is in better agreement with dates obtained with other chronometers,” Paul said.
The study, “A Shorter 146Sm Half-Life Measured and Implications for 146Sm-142Nd Chronology in the Solar System”, was published in Science. Argonne scientists Catherine Deibel, Brad DiGiovine, John Greene, Dale Henderson, Cheng-Lie Jiang, Scott Marley, K. Ernst Rehm, Robert Scott, and Richard Vondrasek also participated in the study.
The work was supported by the DOE Office of Science and the Japan Society for the Promotion of Science.
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