Probing the dark hydrogen of giant planets
Researchers observe an intermediate stage of hydrogen.
Hydrogen is the most-abundant element in the universe. It’s also the simplest—with only a single electron in each atom. But that simplicity is deceptive, because there is still so much we have to learn about hydrogen.
One of the biggest unknowns is its transformation under the extreme pressures and temperatures found in the interiors of stars and giant planets, where it is squeezed until it becomes liquid metal, capable of conducing electricity. New work published in Physical Review Letters by the University of Edinburgh’s Stewart McWilliams and Carnegie Mellon University's Alexander Goncharov measures the conditions under which hydrogen undergoes this transition in the lab and finds an intermediate state between gas and metal, which they’re calling dark hydrogen.
On the surface of giant planets like Jupiter, hydrogen is a gas. But between this gaseous surface and the liquid metal hydrogen in the planet’s core lies a layer of dark hydrogen, according to findings gleaned from the team’s lab mimicry.
Using a laser-heated diamond anvil cell to create the conditions likely to be found in gas giant planetary interiors, the team probed the physics of hydrogen under a range of pressures from 10,000 to 1.5 million times normal atmospheric pressure and up to 10,000 degrees Fahrenheit.
They discovered this unexpected intermediary phase, which does not reflect or transmit visible light, but does transmit infrared radiation.
“This observation would explain how heat can easily escape from gas giant planets like Saturn,” explained Goncharov.
They also found that this intermediary dark hydrogen is somewhat metallic, meaning it can conduct an electric current, albeit poorly. This means that it could play a role the process by which churning metallic hydrogen in gas giant planetary cores produces a magnetic field around these bodies, in the same way that the motion of liquid iron in Earth’s core created and sustained our own magnetic field.
“This dark hydrogen layer was unexpected and inconsistent with what modeling research had led us to believe about the change from hydrogen gas to metallic hydrogen inside of celestial objects,” Alexander Goncharov.
The results are detailed in a paper published in Physical Review Letters.
"In this paper, we measure the conditions where hydrogen becomes a metal inside planets, and observe an intermediate state – dark hydrogen – between the insulating gas and liquid metal. A dark hydrogen layer in giant planets separates the atmosphere and the metallic interior, and neither reflects nor transmits visible light, but does allow infrared radiation to pass. This indicates heat can easily escape from within giant planets. The dark hydrogen layer also weakly conducts electricity, allowing it to participate in the production of the planetary magnetic field." Stewart McWilliams, Centre for Science at Extreme Conditions, who took part in the study.
The team also included Carnegie’s Allen Dalton and Howard University’s Mohammad Mahmood.