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.

Recommended Videos

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…
Astronomers spot the shiniest exoplanet ever discovered
An artist impression of exoplanet LTT9779b orbiting its host star.

When you look up at the night sky you see mostly stars, not planets -- and that's simply because planets are so much smaller and dimmer than stars. But you can see planets in our solar system, like Venus, which is one of the brightest objects in the night sky. Due to its thick, dense atmosphere, Venus reflects 75% of the sun's light, making it shine brightly. Recently, though, astronomers discovered a planet that reflects even more of its star's light, making it the shiniest exoplanet ever found.

Exoplanet LTT9779 b reflects 80% of the light from its star, which it orbits very close to. That makes it extremely hot, and researchers believe that the planet is covered in clouds of silicate and liquid metal, which is what makes it so reflective.

Read more
Astronomers spot an exoplanet creating spiral arms around its star
The Large Binocular Telescope in Arizona. The LBTI instrument combines infrared light from both 8.4-meter mirrors to image planets and disks around young and nearby stars.

When you imagine a galaxy like our Milky Way, you're probably picturing a swirl shape with arms reaching out from a central point. These spiral arms are a classic feature of many galaxies. Similar structures can be found around young stars which are surrounded by disks of matter from which planets form, called protoplanetary disks. Now, astronomers have discovered evidence that these structures could be created by recently formed exoplanets.

Astronomers used Large Binocular Telescope in Arizona to investigate a giant exoplanet named MWC 758c which seems to be forming the spiral arms around its host star. Located 500 light-years away, the star is just a few million years old, making it a baby in cosmic terms. "Our study puts forward a solid piece of evidence that these spiral arms are caused by giant planets," said lead researcher Kevin Wagner of the University of Arizona in a statement. "And with the new James Webb Space Telescope, we will be able to further test and support this idea by searching for more planets like MWC 758c."

Read more
This exoplanet is over 2,000-degrees Celsiu, has vaporized metal in its atmosphere
This artist impression illustrates how astronomers using the Gemini North telescope, one half of the International Gemini Observatory operated by NSF’s NOIRLab, have made multiple detections of rock-forming elements in the atmosphere of a Jupiter-sized exoplanet, WASP-76b. The so-called “hot Jupiter” is perilously close to its host star, which is heating the planet’s atmosphere to astounding temperatures and vaporized rock-forming elements such as magnesium, calcium and iron, providing insight into how our own Solar System formed.

Astronomers have studied a strange, puffy, scorching-hot planet located 600 light-years away, and have seen elements that would normally form rocks, but are so hot that they have vaporized into the atmosphere.

The planet, named WASP-76b, is around the mass of Jupiter, but orbits its star 12 times closer than Mercury is to the sun. Being so close, its atmosphere its heated to a scorching 2,000- degrees Celsius, which makes it puff up to a large size that's six times the volume of Jupiter. These high temperatures also give astronomers the opportunity to observe elements that would normally be hard to identify in the atmosphere of a gas giant.

Read more