Researchers simulate conditions inside 'super-Earths'

By aiming intense X-ray beams at iron samples, scientists have discovered what may lie at the core of "super-Earths," rocky planets triple the mass of Earth orbiting far-distant stars.

The team, led by scientists from Johns Hopkins and Princeton universities, was the first to simulate—if only for the briefest of moments—the deep interiors of these exoplanets, offering insight into what previously had been limited to extrapolations and theoretical calculations.

The results, which also mark the highest-pressure diffraction data ever recorded, were published by the journal Science Advances.

Super-Earths—which are larger than Earth, though substantially less massive than the giant planets orbiting farthest from our sun—have no direct analogues in our solar system. Scientists hope that learning more about their potential structure and composition will lead to insights into types of planetary architecture that may exist in our galaxy. But there are two key obstacles. First, scientists don't have direct measurements of our own planetary core from which to extrapolate. Secondly, interior pressures in super-Earths would be as much as 10 times the pressure at the center of Earth, well beyond the range of traditional measuring tactics.

Image caption: June Wicks

The team, led by June K. Wicks, an assistant professor in Johns Hopkins' Department of Earth and Planetary Sciences who did the work as an associate research scholar at Princeton, directed a short but intense laser beam onto two iron samples: one similar to the modeled composition of Earth's core and another more like silicon-rich planets. The laser compressed the samples for only a few billionths of a second, but long enough to probe the atomic structure using a pulse of bright X-rays.

They discovered significant information about the crystal structure—one of the most critical pieces of the puzzle about the foundation of a planet. The core of a planet effects everything from its magnetic field and thermal evolution to its mass-radius relationship.

At ultrahigh pressures, the lower-silicon alloy organized into a hexagonal close-packed crystal structure, while the higher-silicon alloy adopted body-centered cubic packing.

"This atomic difference has enormous implications," Wicks said. "Knowledge of the crystal structure is the most fundamental piece of information about the material making up the interior of a planet, as all other physical and chemical properties follow from the crystal structure."

Next, Wicks and her colleagues plan to investigate how other light elements, such as carbon or sulfur, affect the structure and density of iron at ultrahigh pressure conditions. They also hope to continue to build more informed models of exoplanets' interiors.

The authors also included other researchers from Johns Hopkins and Princeton and scientists from Lawrence Livermore National Laboratory, the California Institute of Technology, and the University of Rochester.