A team led by Paul Asimow (MS ’93, PhD ’97), professor of geology and geochemistry at Caltech, may have uncovered one of the reasons for that scarcity, demonstrating in laboratory experiments that quasicrystals could arise from collisions between rocky bodies in the asteroid belt with unusual chemical compositions.
A paper on their findings was published on June 13 in the advance online edition of the sciences/” title=”View all articles about Proceedings of the National Academy of Sciences here”>Proceedings of the National Academy of Sciences.
At an atomic level, crystals are both ordered and periodic, meaning that they have a defined geometric structure, with that structure repeating itself over and over. To grow such a repeating structure without the original organization breaking down, the crystal can only exhibit one of four types of rotational symmetry: two-fold, three-fold, four-fold, or six-fold.
The number refers to how many times an object will look exactly the same within a full 360-degree rotation about an axis. For example, an object with two-fold symmetry appears the same twice, or every 180 degrees; an object with three-fold symmetry appears the same three times, or every 120 degrees; and an object with four-fold symmetry appears the same four times, or every 90 degrees.
Prior to 1984, it was believed that it would be impossible for a crystal to grow with any other type of symmetry; no examples of crystals with other symmetries had been discovered in nature or grown in a lab. In that year, however, Princeton physicist Paul Steinhardt (BS ’74) theorized a set of conditions under which other types of symmetry could potentially exist and Dan Shechtman of the Israel Institute of Technology published a paper announcing the creation of a crystal-like structure with a five-fold rotational symmetry.
These structures were ordered enough to produce recognizable diffraction patterns when shot with high-energy beams of electrons and X-rays—unlike disordered structures, which produce no patterns. However, the crystal-like structures were not periodic—that is, their organization shifted and changed as they grew. The materials were dubbed “quasiperiodic crystals,” or “quasicrystals” for short.
Over the next few decades, researchers figured out how to manufacture more than 100 different varieties of quasicrystals by melting and homogenizing certain elements and then cooling them at very specific rates in the lab. Still, though, no naturally existing quasicrystals were known. Indeed, researchers suspected their formation would be impossible. That is because most lab-grown quasicrystals were metastable, meaning that the same combination of elements could arrange themselves into a crystalline structure using less energy.
Everything changed in the late 2000s, when Steinhardt and colleague Luca Bindi from the Museum of Natural History at the University of Florence (currently in the Faculty of the Department of Earth Sciences of the same University) found a tiny grain of an aluminum, copper, and iron mineral that exhibited five-fold symmetry. The grain came from a small sample of the Khatyrka meteorite, an extraterrestrial object known only from a few pieces found in Russia‘s Koryak Mountains. Steinhardt and his collaborators found a second natural quasicrystal from the same meteorite in 2015, confirming that the natural existence of quasicrystals was possible, just very rare.
A microscopic analysis of the meteorite indicated that it had undergone a major shock at some point in its lifetime before crashing to Earth – likely from a collision with another rocky body in space. Such collisions are common in the asteroid belt and release high amounts of energy.
Asimow and colleagues hypothesized that the energy released by the shock could have caused the quasicrystal’s formation by triggering a rapid cycle of compression, heating, decompression, and cooling.
To test the hypothesis, Asimow simulated the collision between two asteroids in his lab. He took thin slices of minerals found in the Khatyrka meteorite and sandwiched them together in a sample case that resembles a steel hockey puck. He then screwed the “puck” to the muzzle of a four-meter-long, 20-mm-bore single-stage propellant gun, and blasted it with a projectile at nearly one kilometer per second, about equal to the speed of the fastest rifle-fired bullets.
It is important to note that those minerals included a sample of a metallic copper-aluminum alloy, which has only been found in nature in the Khatyrka meteorite.
After the sample was shocked with the propellant gun, it was sawed open, polished, and examined. The impact smashed the sandwiched elements together and, in several spots, created microscopic quasicrystals.
Armed with this experimental evidence, Asimow says he is confident that shocks are the source of naturally formed quasicrystals. “We know that the Khatyrka meteorite was shocked. And now we know that when you shock the starting materials that were available in that meteorite, you get a quasicrystal.”
Sarah Stewart (PhD ’02)—a planetary collision expert from the University of California, Davis, and reviewer of the PNAS paper—admits she was surprised by the findings. “If you had called me before the study and asked if this would work I would have said ‘no way.’ The astounding thing is that they did it so easily,” she says. “Nature is crazy.”
Asimow acknowledges that the experiments leave many questions unanswered. For example, it is unclear at what point the quasicrystal formed during the shock’s pressure and temperature cycle. A bigger mystery, Asimow says, is the origin of the copper-aluminum alloy in the meteorite, which has never been seen elsewhere in nature.
Next, Asimow plans to shock various combinations of minerals to see what key ingredients are necessary for natural quasicrystal formation.
These results are published in a paper titled “Shock synthesis of quasicrystals with implications for their origin in asteroid collisions.” In addition to Asimow, Steinhardt, and Bindi, other coauthors on the paper are Chi Ma, director of analytical facilities in the Geological and Planetary Sciences division at Caltech; Lincoln Hollister (PhD ’66) and Chaney Lin from Princeton University; and Oliver Tschauner from the University of Nevada, Las Vegas. Their work was supported by the National Science Foundation (NSF), the University of Florence, and the NSF-Materials Research Science & Engineering Centers Program through New York University and the Princeton Center for Complex Materials.