From: Hiroshima University
Posted: Thursday, August 4, 2016
New experiments provide insight into how Earth-type planets form when giant asteroids or planetesimals collide and how the interiors of such planets develop. Researchers at Hiroshima University, Osaka University, Ehime University, University of Tokyo, and the Chiba Institute of Technology collaborated to publish their research in the August 3, 2016 issue of Science Advances.
"Our results provide a better understanding how impact-generated magmas evolve and allow us to model Earth-type planets' inner structures. Collisions at these extreme temperatures and pressures created our own Earth and may have also formed the mantles of other Super Earth planets, for example CoRoT-7b and Kepler-10b," said Toshimori Sekine, Ph.D., first author of the research paper and Professor at Hiroshima University.
These powerful collisions cause chemical reactions within the giant rocks and knowing what types of reactions occur under what conditions gives researchers a better understanding of the development of planets too far away for satellites to explore. Many of the rocks include forsterite, a representative mineral that makes up much of the matter in space. Forsterite, known to scientists as Mg2SiO4, is a combination of Magnesium, Silicone, and Oxygen and is the most abundant constituent of Earth's mantle, the layer between the surface crust and molten core.
The research team of geophysicists and engineers successfully measured the melting of forsterite. However, replicating the intense collisions that can turn minerals into magma in Earth-based experiments was a challenge.
"The laser shock technique was first used in the 1990s, but the results were not precise. Recent technical advances enable us to measure precisely the laser-shocked states," said Sekine.
The laser shock technique uses a high-power laser to irradiate a target, which was a block of forsterite in the experiments by Sekine's team. The energy of the irradiation causes an abrupt expansion of the target's molecules and the inertia of this expansion generates a shock wave. The energy from the shock wave can create heat and light that melts and reflects off of the forsterite.
Previous studies without the laser shock technique only measured the properties of forsterite at shock pressures below 200 Giga Pascals (GPa). The new experiments put forsterite crystals under pressures between approximately 250 and 970 GPa. For comparison, the pressure at the center of Earth is estimated to be 360 GPa.
Researchers measured the pressure, temperature, density, and reflectivity of laser-shocked forsterite. These parameters did not increase at a constant rate as the pressure steadily increased, revealing that both energy producing and energy absorbing reactions occur in shocked forsterite melt at pressures between 250 GPa and 344 GPa.
Earlier research has connected magnesium oxide, one of the minerals that is formed from forsterite, to the reactions necessary for a planet to develop a magnetic field that persists for a long geological time, such as the magnetic field of Earth. With these new details of forsterite's melting behavior, researchers may be able to predict how minerals separate into different layers of magma and which minerals may be close enough to react.
"Our results can support the possibility that violent, large-scale collisions between space bodies containing enough forsterite and moving faster than about 13 kilometers per second (8.1 miles per second) could lead to chemical layering in the mantels of massive terrestrial planets. Melting forsterite may have produced a sufficiently high concentration of magnesium oxide in early Earth's core to power a magnetic field around the planet," said Sekine.
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This work was supported in part by JSPS KAKENHI Grant Numbers 22224012, JSPS core to core program on International Alliance for Material Science in Extreme States with High Power Laser and XFEL, and X-ray Free Electron Laser Priority Strategy Program (MEXT).
Citation Details for the Research Paper:
Sekine T, Ozaki N, Miyanishi K, Asaumi Y, Kimura T, Albertazzi, Yuya Sato, Sakawa Y, Sano T, Sugita S, Matsui T, Kodama R. 3 August 2016. Shock compression response of forsterite above 250 GPa. Science Advances.
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