Asteroid impact in slow motion
Researchers at the University of Jena and the German Electron Synchrotron DESY solve a 60-year-old mystery with a high-pressure study
Large asteroid impacts can melt significant amounts of material from Earth's crust (artist's impression).
- Research
Published: | By: Till Mundzeck
For the first time, researchers have recorded live and in atomic detail what happens to the material in an asteroid impact. The team of Falko Langenhorst from the University of Jena and Hanns-Peter Liermann from DESY simulated an asteroid impact with the mineral quartz in the lab and pursued it in slow motion in a diamond anvil cell, while monitoring it with DESY's X-ray source PETRA III. The observation reveals an intermediate state in quartz that solves a decades-old mystery about the formation of characteristic lamellae in material hit by an asteroid. Quartz is ubiquitous on the Earth's surface, and is, for example, the major constituent of sand. The analysis helps to better understand traces of past impacts, and may also have significance for entirely different materials. The researchers present their findings in the journal Nature Communications.
Asteroid impacts are catastrophic events that create huge craters and sometimes melt parts of Earth's berock. “Nevertheless, craters are often difficult to detect on Earth, because erosion, weathering and plate tectonics cause them to disappear over millions of years,” Langenhorst explains. Therefore, minerals that undergo characteristic changes due to the force of the impact often serve as evidence of an impact. For example, quartz sand (which chemically is silicon dioxide, SiO2) is gradually transformed into glass by such an impact, with the quartz grains then being crisscrossed by microscopic lamellae. This structure can only be explored in detail under an electron microscope. It can be seen in material from the relatively recent and prominent Barringer crater in Arizona, USA, for example.
Barringer crater in Arizona was formed about 50 000 years ago by an approximately 50-meter iron meteorite.
“For more than 60 years, these lamellar structures have served as an indicator of an asteroid impact, but no one knew until now how this structure was formed in the first place,” Liermann says. “We have now solved this decades-old mystery.” To do so, the researchers had spent years modifying and advancing techniques that allow materials to be studied under high pressure in the lab. In these experiments, samples are usually compressed between two small diamond anvils in a so-called diamond anvil cell (DAC). It allows extreme pressures – as prevalent in Earth's interior or in an asteroid impact – to be generated in a controlled manner.
Charactersitic lamellae
For its experiments, the team used a dynamic diamond anvil cell (dDAC) in which the pressure can be changed very quickly during the measurement. With this device, the scientists compressed small quartz single crystals stronger and stronger, while shining PETRA III's intense X-ray light through them to investigate changes to their crystal structure. “The trick is to let the simulated asteroid impact proceed slowly enough to be able to follow it with the X-ray light, but not too slowly, so that the effects typical of an asteroid impact can still occur,” Liermann says. Experiments on the scale of seconds proved to be the right duration.
“We observed that at a pressure of about 180,000 atmospheres, the quartz structure suddenly transformed into a more tightly packed transition structure, which we call rosiaite-like,” reports first author Christoph Otzen, who is writing his doctoral thesis on these studies. “In this crystal structure, the quartz shrinks by a third of its volume. The characteristic lamellae form exactly where the quartz changes into this so-called metastable phase, which no one has been able to identify in quartz before us.” Rosiaite is an oxidic mineral and the namesake for the crystal structure that is known from various materials. It does not consist of silica, but is a lead antimonate (a compound of lead, antimony and oxygen).
Collapse into disorder
“The higher the pressure rises, the larger the ratio of silica with a rosiaite-like structure in the sample,” Otzen explains. “But when the pressure drops again, the rosiaite-like lamellae do not transform back into the original quartz structure, but collapse into glass lamellae with a disordered structure. We also see these lamellae in quartz grains from deposits of asteroid impacts.”
Quantity and orientation of the lamellae allow conclusions to be drawn about the impact. For instance, they indicate how high the impact pressure has been. “For decades, such lamellae have been used to detect and analyze asteroid impacts,” Langenhorst points out. “But only now can we accurately explain and understand their formation."
For the study, the researchers did not use the highest pressures technically feasible. “In the range of the highest pressures, so much heat is generated that the material melts or vaporizes,” explains Langenhorst. “Molten material that solidifies back into rock doesn't give us much useful information for now. What is important, however, is precisely the pressure range in which minerals undergo characteristic changes in the solid state, and that's what we studied in this case.”
The simulated asteroid impact creates tiny glass lamellae in the quartz crystals studied, only tens of nanometers wide, which are only visible under the electron microscope.
Model for glass formation?
The results could have significance beyond the study of asteroid impacts. “What we observed could be a model study for the formation of glass in completely different materials such as ice,” Langenhorst points out. “It might be the generic path that a crystal structure transforms into a metastable phase in an intermediate step during rapid compression, which then transforms into the disordered glass structure. We plan to investigate this further, because it could be of great importance for materials research.”
With the planned transformation of PETRA III at DESY into the world's best X-ray microscope, PETRA IV, such studies will be even more realistically possible in the future. “A 200 times higher X-ray intensity will allow us to run these experiments 200 times faster, so we can simulate an asteroid impact even more realistically,” says Liermann.
Information
Original publication
Evidence for a rosiaite-structured high-pressure silica phase and its relation to lamellar amorphization in quartz; Christoph Otzen, Hanns-Peter Liermann, Falko Langenhorst; „Nature Communications“, 2023; https://doi.org/10.1038/s41467-023-36320-7External link
Falko Langenhorst, Prof. Dr