The Solar System — 03

There Are Diamonds Raining on Neptune

Seven thousand kilometres below the cloud tops, pressure crushes carbon into crystal. The diamonds fall like hailstones through a sea of hydrogen — for thousands of years — until they vanish into the core.

12 min read · Interactive article
01 — The Rain No One Can See

Inside an Ice Giant

Neptune is the most distant major planet in the solar system — 4.5 billion kilometres from Earth, so far that sunlight takes over four hours to reach it. From the outside, it looks serene: a jewel of deep azure floating in darkness, brushed with faint bands of white cloud.

But that calm exterior conceals one of the most extreme environments in the solar system. Beneath the upper atmosphere of hydrogen and helium lies a thick envelope of water, ammonia, and methane, compressed to densities that blur the line between liquid and solid. There is no surface to stand on. The “ice” in “ice giant” is not frozen in any familiar sense — it is a hot, dense fluid crushed under millions of atmospheres of pressure.

And somewhere inside that crushing darkness, carbon atoms are being squeezed into diamonds.

“The conditions inside Neptune are so extreme that methane — the simplest organic molecule with carbon — is literally ripped apart, and the freed carbon atoms are compressed into diamond.”

Dominik Kraus, Helmholtz-Zentrum Dresden-Rossendorf

Not tiny industrial fragments. Not microscopic inclusions in rock. Scientists estimate that diamonds the size of icebergs may be falling through Neptune’s mantle at this moment — a slow, continuous rain of gemstone that has lasted for billions of years.

Neptune’s Interior Tap layers to explore
LayerUpper Atmosphere
Depth0 km
Pressure1 bar
Temperature72 K

Neptune has no well-defined surface. The atmosphere thins gradually into a hot, dense mantle of compressed ices. The planet’s interior is layered by density and pressure: hydrogen and helium give way to a thick slurry of water, ammonia, and methane. Deeper still, temperatures reach 7,000 K and pressures exceed 6 million atmospheres.

It is in this region — the boundary between the ice mantle and the rocky core — that diamond rain is thought to form.

02 — Squeezing Carbon Into Crystal

How We Know

For decades, diamond rain inside ice giants was an elegant hypothesis with no experimental confirmation. The physics seemed plausible — methane decomposes under extreme pressure and temperature, freeing carbon atoms that crystallise into diamond — but no one had reproduced the conditions in a laboratory.

That changed in 2017.

1977
Voyager 2 launch
The only spacecraft to visit Neptune. Arrives in 1989, revealing a dynamic atmosphere with the fastest winds in the solar system (2,100 km/h) and a mysterious internal heat source — Neptune radiates 2.6 times more energy than it receives from the Sun.
1999
Early compression experiments
Researchers at Lawrence Livermore National Laboratory use shock compression on liquid methane, detecting hints of diamond formation. The results are suggestive but indirect.
2017
Kraus et al. — Nature Physics
At SLAC National Accelerator Laboratory, a team led by Dominik Kraus fires the world’s most powerful X-ray laser at polystyrene (a hydrocarbon stand-in for methane). For the first time, they watch diamond nanocrystals form in real time under conditions matching Neptune’s interior: 150 GPa, 5,000 K.
2022
Confirmation — PET plastic experiments
A follow-up study at SLAC uses PET plastic, which includes oxygen — a closer match to planetary ices. Diamonds form even more readily. The oxygen acts as a catalyst, accelerating carbon crystallisation. Diamond rain inside ice giants is no longer a hypothesis — it is a near-certainty.

The experiments revealed something else: the diamonds, once formed, would be denser than the surrounding material. They would sink. Slowly, relentlessly, through thousands of kilometres of compressed fluid — a rain that has likely been falling for 4.5 billion years.

“We produced diamond rain in the laboratory. The high-pressure conditions we created correspond to a depth of about 10,000 kilometres inside Neptune.”

Dominik Kraus, Nature Physics, 2017
Descent into Neptune Drag the slider to descend
Upper Atmosphere
0 km depth
Cloud tops Core

Thin hydrogen and helium atmosphere. Temperatures near −220°C. Winds exceed 2,000 km/h — the fastest in the solar system.

Pressure1 bar
Temperature−220 °C
Density0.001 g/cm³
03 — A Universe of Diamond Worlds

The Most Common Planet We’ve Never Visited

Here is the fact that makes diamond rain more than a curiosity: ice giants are the most common type of large planet in the galaxy.

Our solar system has two — Uranus and Neptune. But exoplanet surveys suggest that ice-giant-sized worlds outnumber gas giants like Jupiter and Saturn by a factor of ten. The Kepler space telescope found them orbiting stars of every spectral type, at distances from scorching-close to freezing-far.

~10×
More ice giants than gas giants in the Milky Way
Kepler survey estimates suggest ice giants are the most common class of large planet — and we have visited exactly one of them, once, for twelve hours.

If diamond rain occurs inside our two ice giants — and the lab experiments strongly suggest it does — then it is happening right now inside billions of planets across the galaxy. It is not an exotic curiosity. It may be one of the most common geological processes in the universe.

And it may explain a long-standing puzzle. Neptune radiates 2.6 times more thermal energy than it receives from the Sun. Where does the extra heat come from? One answer: the gravitational energy released by sinking diamonds. As they fall through the mantle, they convert potential energy into heat — a slow furnace of crystallised carbon warming the planet from within.

Diamond Rain Diamonds fall through the mantle

Each diamond may take thousands of years to sink from the formation zone to the core — a slow, glittering descent through crushing darkness.

Diamonds in view0
Avg. size
Fall velocity

We do not yet know what happens to the diamonds when they reach the core. Some models suggest they accumulate over billions of years into a thick diamond shell surrounding the rocky centre. Others propose they dissolve back into carbon in the extreme heat near the core boundary. Either way, the process is ongoing — a slow, vast, alien form of weather that has no parallel on Earth.

“The universe makes diamonds the way Earth makes rain. We just happen to live on a world too small and too cool for the process.”

No spacecraft has ever orbited an ice giant. No probe has descended into one. What we know about diamond rain comes from fleeting flybys, laboratory lasers, and mathematical models. There is a proposed NASA mission — a Neptune orbiter and atmospheric probe — in the 2030s Planetary Science Decadal Survey. If it flies, it would be our first real look inside an ice giant.

Until then, the diamonds keep falling. They have been falling for longer than life has existed on Earth. And somewhere, around a star we have not yet named, they are falling right now — inside a world we will never visit — in a rain that no one will ever see.

Frequently Asked Questions

Almost certainly, yes. Laboratory experiments at SLAC National Accelerator Laboratory in 2017 and 2022 produced diamond crystals under conditions matching Neptune’s interior (150 GPa pressure, 5,000 K). While no probe has directly observed diamond rain inside an ice giant, the physics is well-established and the experimental confirmation is strong.

Laboratory experiments produce nanoscale diamond crystals, but models suggest that inside a real planet — where the process has been continuous for 4.5 billion years — the diamonds could grow much larger. Some estimates suggest diamonds could reach masses of millions of carats, though the exact size remains uncertain.

Methane (CH₄) is a simple molecule: one carbon atom bonded to four hydrogen atoms. Under extreme pressure (above ~100 GPa), the molecular bonds break. The freed carbon atoms are squeezed into the dense, tetrahedral crystal structure of diamond. The hydrogen floats upward as a separate fluid. The 2022 experiments showed that oxygen, present in planetary ices, accelerates this process.

Yes. Uranus has a similar bulk composition to Neptune — both are classified as ice giants with thick mantles of water, ammonia, and methane. The conditions for diamond formation exist inside Uranus as well, though Uranus radiates less internal heat than Neptune, which may indicate differences in the interior dynamics.

Not with any foreseeable technology. The diamonds form at depths of 7,000–10,000 km below the cloud tops, under pressures exceeding 1 million atmospheres and temperatures above 3,500°C. There is no solid surface to land on. Any material sent into those depths would be crushed and dissolved. The diamonds of Neptune will remain permanently inaccessible.

Neptune emits 2.6 times more thermal energy than it absorbs from the Sun. Diamond rain may be a significant contributor: as diamonds sink through the mantle, they release gravitational potential energy as heat. Other proposed mechanisms include ongoing gravitational contraction and compositional differentiation, but diamond rain provides an elegant explanation for the excess heat.