Skip to main content

Inside giant ice planets, it could be raining diamonds

The universe is stranger than you can imagine, and out in the depths of space, there are wild and weird exoplanets to be found — planets with glowing rivers of lava, or planets under gravitational forces so strong they are shaped like a football. We can add to this list another class of strange planet, ones on which it rains diamonds.

The diamond rain effect is thought to occur deep within ice giants like Uranus and Neptune, and it was re-created in a lab here on Earth in 2017. Now, researchers have found that this effect isn’t just a rare fluke but could be more common than previously thought.

Diamond rain could occur on ice giant planets in the presence of oxygen.
Diamond rain can occur deep within ice giant planets and is more common in the presence of oxygen. Greg Stewart/SLAC National Accelerator Laboratory

The international group of researchers working with the SLAC National Accelerator Laboratory previously created the diamond rain effect by placing hydrogen and carbon under extremely high pressures. But in this new research, they wanted to make the conditions more realistic to what the interior of an ice giant planet would be like by also including other elements that would be present, such as oxygen.

To simulate this mix of chemicals, the researchers used a familiar material — PET plastic, like that used in good packaging, which turns out to be chemically similar to the conditions they wanted to create. “PET has a good balance between carbon, hydrogen, and oxygen to simulate the activity in ice planets,” explained one of the researchers, Dominik Kraus of the University of Rostock.

The researchers used a high-powered laser to create shock waves in the plastic, then observed how X-rays bounced off it. This let them see how small diamonds were forming. The diamonds produced in the experiment were very small, called nanodiamonds, but at around 5,000 miles beneath the surface of an ice giant much larger diamonds could form, where they would fall toward the planet’s icy core. The diamonds could even sink into the core and form a thick diamond layer.

In the new experiments, the team found that when they included oxygen then the nanodiamonds grew at lower temperatures and pressures, which means that having oxygen present makes the formation of diamond rain more likely. “The effect of the oxygen was to accelerate the splitting of the carbon and hydrogen and thus encourage the formation of nanodiamonds,” Kraus said. “It meant the carbon atoms could combine more easily and form diamonds.”

With this discovery, the researchers now want to try the experiments again and include chemicals like ethanol, water, and ammonia to even more closely model the environments of ice giants.

“The fact that we can recreate these extreme conditions to see how these processes play out on very fast, very small scales is exciting,” said SLAC scientist and collaborator Nicholas Hartley. “Adding oxygen brings us closer than ever to seeing the full picture of these planetary processes, but there’s still more work to be done. It’s a step on the road towards getting the most realistic mixture and seeing how these materials truly behave on other planets.”

The research is published in the journal Science Advances.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
James Webb observes extremely hot exoplanet with 5,000 mph winds
This artist’s concept shows what the hot gas-giant exoplanet WASP-43 b could look like. WASP-43 b is a Jupiter-sized planet circling a star roughly 280 light-years away, in the constellation Sextans. The planet orbits at a distance of about 1.3 million miles (0.014 astronomical units, or AU), completing one circuit in about 19.5 hours. Because it is so close to its star, WASP-43 b is probably tidally locked: its rotation rate and orbital period are the same, such that one side faces the star at all times.

Astronomers using the James Webb Space Telescope have modeled the weather on a distant exoplanet, revealing winds whipping around the planet at speeds of 5,000 miles per hour.

Researchers looked at exoplanet WASP-43 b, located 280 light-years away. It is a type of exoplanet called a hot Jupiter that is a similar size and mass to Jupiter, but orbits much closer to its star at just 1.3 million miles away, far closer than Mercury is to the sun. It is so close to its star that gravity holds it in place, with one side always facing the star and the other always facing out into space, so that one side (called the dayside) is burning hot and the other side (called the nightside) is much cooler. This temperature difference creates epic winds that whip around the planet's equator.

Read more
First indications of a rare, rainbow ‘glory effect’ on hellish exoplanet
For the first time, potential signs of the rainbow-like ‘glory effect’ have been detected on a planet outside our Solar System. Glory are colourful concentric rings of light that occur only under peculiar conditions. Data from ESA’s sensitive Characterising ExOplanet Satellite, Cheops, along with several other ESA and NASA missions, suggest this delicate phenomenon is beaming straight at Earth from the hellish atmosphere of ultra-hot gas giant WASP-76b, 637 light-years away.

Just from looking at our own solar system, we can see that planets come in a wide variety of colors -- from the dusty red of Mars to the bright blues of Uranus and Neptune. Planets like Jupiter have beautiful bands of color caused by variations in the atmosphere, while it's hard to even see the surface of Venus because its atmosphere is so thick. But there are other variations in color which planets can display, like a stunning rainbow-hued set of circular rings called a glory.

Glories are observed on Earth, and have been seen just once on another planet, Venus. But now, researchers believe they may have identified a glory on a planet outside our solar system for the first time. The extreme exoplanet WASP-76b could be host to the first known extrasolar glory, observed by the European Space Agency (ESA)'s Characterising ExOplanet Satellite (Cheops).

Read more
Is dark energy changing over time? A new survey suggests it could be
An artistic celebration of the Dark Energy Spectroscopic Instrument (DESI) year-one data, showing a slice of the larger 3D map that DESI is constructing during its five-year survey. By mapping objects across multiple periods of cosmic history with extremely high precision, DESI is allowing astronomers to make unprecedented measurements of dark energy and its effect on the accelerating expansion of the Universe.

New results from a survey into dark energy show a look back  11 billion years into the past, revealing the locations of tens of thousands of galaxies in the largest ever 3D map of the universe. The results from the Dark Energy Spectroscopic Instrument Survey, or DESI, were released this week and show how the universe has expanded over billions of years.

The results so far are shown in a 3D map covering 600,000 galaxies, though incredibly this data is just 0.1% of the total volume of the full survey. The results have been plotted to show how galaxies appear to be moving away from us as the universe expands, with light that has traveled the furthest represented in red, referring to the most distant galaxies, and nearer galaxies represented in blue.

Read more