Spacecraft Juno nears planet orbit, but Harvard team may already have predicted part of what it will find

June 30, 2016 by Leah Burrows, Harvard John A. Paulson School of Engineering and Applied Sciences
Harvard researchers observed evidence of the transition of hydrogen to metallic hydrogen by squeezing a sample of liquid hydrogen between two diamond tips. Credit: Mohamed Zaghoo/Harvard SEAS

In less than a week, the spacecraft Juno will arrive at Jupiter, the culmination of a five-year, billion-dollar journey. It's mission: to peer deep inside the gas giant and unravel its origin and evolution. One of the biggest mysteries surrounding Jupiter is how it generates its powerful magnetic field, the strongest in the solar system.

One theory is that about halfway to Jupiter's core, the pressures and temperatures become so intense that the hydrogen that makes up 90 percent of the planet—molecular gas on Earth—looses hold of its electrons and begins behaving like a liquid metal. Oceans of surrounding Jupiter's core would explain its powerful magnetic field.

But how and when does this transition from gas to liquid metal occur? How does it behave? Researchers hope that Juno will shed some light on this exotic state of hydrogen—but one doesn't need to travel all the way to Jupiter to study it.

Four hundred million miles away, in a small, windowless room in the basement of Lyman Laboratory on Oxford Street in Cambridge, Massachusetts, there was, for a fraction of a fraction of a second, a small piece of Jupiter.

Earlier this year, in an experiment about five-feet long, Harvard University researchers say they observed evidence of the abrupt transition of hydrogen from liquid insulator to . It is one of the first times such a transition has ever been observed in any experiment.

They published their research in Physical Review B.

"This is planetary science on the bench," said Mohamed Zaghoo, the NASA Earth & Space Science Fellow at the Harvard John A. Paulson School of Engineering and Applied Sciences (SEAS). "The question of how hydrogen transitions into a metallic state—whether that is an abrupt transition or not—has huge implications for planetary science. How hydrogen transitions inside Jupiter, for example, says a lot about the evolution, the temperature and the structure of these gas giants interiors."

In the experiment, Zaghoo, Ashkan Salamat, and senior author Isaac Silvera, the Thomas D. Cabot Professor of the Natural Sciences, recreated the extreme pressures and temperatures of Jupiter by squeezing a sample of hydrogen between two diamond tips, about 100 microns wide, and firing short bursts of lasers of increasing intensity to raise the temperature.

This experimental setup is significantly smaller and cheaper than other current techniques to generate , most of which rely on huge guns or lasers that generate shock waves to heat and pressurize hydrogen.

The transition of the liquid to metallic hydrogen happens too quickly for human eyes to observe and the sample lasts only a fraction of a second before it deteriorates. So, instead of watching the sample itself for evidence of the transition, the team watched lasers pointed at the sample. When the phase transition occurred, the lasers abruptly reflected.

"At some point, the hydrogen abruptly transitioned from an insulating, transparent state, like glass, to a shiny metallic state that reflected light, like copper, gold or any other metal," Zaghoo said. "Because this experiment, unlike shock wave experiments, isn't destructive, we could run the experiment continuously, doing measurements and monitoring for weeks and months to learn about the transition."

"This is the simplest and most fundamental atomic system, yet modern theory has large variances in predictions for the transition pressure," Silvera said. "Our observation serves as a crucial guide to modern theory."

The results represent a culmination of decades of research by the Silvera group. The data collected could begin to answer some of the fundamental questions about the origins of solar systems.

Metallic hydrogen also has important ramifications here on Earth, especially in energy and materials science.

"A lot of people are talking about the hydrogen economy because hydrogen is combustibly clean and it's very abundant," said Zaghoo. "If you can compress hydrogen into high density, it has a lot of energy compacted into it."

"As a rocket fuel, metallic hydrogen would revolutionize rocketry as propellant an order of magnitude more powerful than any known chemical," said Silvera. "This could cut down the time it takes to get to Mars from nine months to about two months, transforming prospects of human space endeavors."

Metallic hydrogen could be used to make room temperature or even higher than room temperature super-conductors.

The Juno mission goes hand-in-hand with laboratory experiments into metallic , Zaghoo said.

"The measurements of Jupiter's magnetic field that Juno will be collecting is directly related to our data," he said. "We're not in competition with NASA but, in some ways, we got to Jupiter first."

Explore further: Probing giant planets' dark hydrogen

More information: Mohamed Zaghoo et al. Evidence of a first-order phase transition to metallic hydrogen, Physical Review B (2016). DOI: 10.1103/PhysRevB.93.155128

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shavera
4.4 / 5 (14) Jun 30, 2016
metallic state that reflected light, like copper, gold or any other metal,


Completely inadvertent, I'm sure, but it's interesting that the metals used in this analogy actually have different spectra of reflectance in the visible spectrum than most metals; ie, they're not shiny grey, reflecting all visible light roughly equally, they're shiny gold or copper, absorbing some of the blue light incident on their surface.
Mike_Massen
3.4 / 5 (10) Jul 01, 2016
Very interesting line of experimental research

shavera offered
.. metals used in this analogy actually have different spectra of reflectance in the visible spectrum than most metals
Indeed which raises few questions

1. Spectra of emission/absorbance correlated with pressure (fluctuations) re any nucleonic decay or probabilistic H-H/H-D fusion, paper link has 4 graphs but, nil spectra, early days I expect
2. Potential re 1. to search for signature of fusion Eg from even probabilistically low tunneling as is modeled in Sol's core - ie Less per m^3 (~270W) than a human body's output via chemistry despite Sol's much higher H2 density at core
3. And re 1. extrapolation if any Eutectic's arising which might moderate/augment probabilistic fusion equilibria even to ignite interest ;-)

IOW. We know fusion easy to generate at low level but, not efficient re power yet.

Then might study of Jupiter's core & spectra offer clues re potential to accelerate fusion here ?
FredJose
1.4 / 5 (10) Jul 04, 2016
None of the gas- giants should exist - according to the powder-puff accretion theory of planetary formation.
By all accounts they should still be in the "process of formation" since by that little muffinary theory that's how long it'll take to get these planets to form all by themselves since the evolutionary beginning of the solar system.

But since these planets are all there and looking decidedly aged already, one can justly jump to the conclusion that the theory itself is very nebular in substance.
Further condemnation of the nebulous theory of accretion is the great number of "Hot" Jupiters that has been discovered already - making a great mockery of the famously nebulous accretion theory of planetary formation.
CockyChocachubra
Jul 04, 2016
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