A University of Arkansas researcher and his colleagues have used magnesium isotopes to determine the temperature at which rocks form, which will allow scientists to better study the formation of the earth’s crust and mantle as well as the formation of meteorites.
Fang-Zhen Teng, professor of geosciences, and Wang-Ye Li, Yilin Xiao and Jian Huang of the University of Science and Technology of China report their findings in Earth and Planetary Science Letters.
“Knowing the temperature of rock formations is important to understanding the earth’s evolution,” Teng said. “We also can study extraterrestrial samples to know more about how meteorites formed and evolved.”
Of course, most rocks on earth have been rocks for millions and millions of years, making it difficult to determine their thermal history.
“We have to study the formation temperature of rocks indirectly,” Teng said. Several methods for doing so exist, but most do not give accurate readings at the high temperatures where rocks form. “How the temperature varies at depth within the earth’s crust and mantle is still uncertain,” Teng said.
The researchers studied magnesium isotope fractionation in eclogite, a metamorphic rock that contains the minerals omphacite and garnet, found in a mountain range in China. Eclogites form at high temperatures and pressures and often form from subducted ocean floor basalts that are drawn below the earth’s crust, and are brought to the surface during mountain-building processes.
Isotopes have the same chemical properties, but different weights, so some processes cause what looks like the same material to behave differently. In this case, the researchers looked at isotope fractionation, or the separation of isotopes into different areas within the rock. The magnesium isotope fractionation within a rock depends upon the temperature at which the atoms stopped moving within it, which is the time that the rock has formed.
The scientists found that the fractionation of magnesium isotopes is big at high temperatures, which allows researchers to then study it accurately. The researchers looked at other isotopes, but found the fractionation to be too small to measure precisely. The light magnesium isotopes move quickly to a low energy state (i.e., garnet), whereas the heavy isotopes prefer a high-energy state (i.e., omphacite). The proportion of light and heavy isotopes in each state in a given rock determines the temperature at which the rock formed. Using this magnesium isotope fractionation, the researchers can determine the temperature of rock formation to a higher precision. For example, if previous isotope “thermometers” only determined the temperature to a precision of within 50 degrees Celsius, then the magnesium thermometer can reach a precision of within 20 degrees Celsius.By knowing the temperature of the rock formation, scientists will be able to determine the cooling rate of rocks at different depths within the earth’s crust and mantle. This will help them learn more about how the rocks cool down.
“This will help us determine how mountains were built. If we know the ‘cooking’ history, we can determine how fast the mountains were built and how the plates collide and evolve,” Teng said.
The researchers plan to collect samples from mountain building areas to further use this new tool.CONTACTS:
Fang-Zhen Teng | Newswise Science News
NASA examines Peru's deadly rainfall
24.03.2017 | NASA/Goddard Space Flight Center
Steep rise of the Bernese Alps
24.03.2017 | Universität Bern
Astronomers from Bonn and Tautenburg in Thuringia (Germany) used the 100-m radio telescope at Effelsberg to observe several galaxy clusters. At the edges of these large accumulations of dark matter, stellar systems (galaxies), hot gas, and charged particles, they found magnetic fields that are exceptionally ordered over distances of many million light years. This makes them the most extended magnetic fields in the universe known so far.
The results will be published on March 22 in the journal „Astronomy & Astrophysics“.
Galaxy clusters are the largest gravitationally bound structures in the universe. With a typical extent of about 10 million light years, i.e. 100 times the...
Researchers at the Goethe University Frankfurt, together with partners from the University of Tübingen in Germany and Queen Mary University as well as Francis Crick Institute from London (UK) have developed a novel technology to decipher the secret ubiquitin code.
Ubiquitin is a small protein that can be linked to other cellular proteins, thereby controlling and modulating their functions. The attachment occurs in many...
In the eternal search for next generation high-efficiency solar cells and LEDs, scientists at Los Alamos National Laboratory and their partners are creating...
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are less stable. Now researchers at the Technical University of Munich (TUM) have, for the first time ever, produced a composite material combining silicon nanosheets and a polymer that is both UV-resistant and easy to process. This brings the scientists a significant step closer to industrial applications like flexible displays and photosensors.
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are...
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to simulate these confined natural conditions in artificial vesicles for the first time. As reported in the academic journal Small, the results are offering better insight into the development of nanoreactors and artificial organelles.
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to...
20.03.2017 | Event News
14.03.2017 | Event News
07.03.2017 | Event News
24.03.2017 | Materials Sciences
24.03.2017 | Physics and Astronomy
24.03.2017 | Physics and Astronomy