

The ice giants Uranus and Neptune do not get almost sufficient press; all the eye goes to their bigger siblings, mighty Jupiter and sumptuous Saturn.
At first look, Uranus and Neptune are simply bland, boring balls of uninteresting molecules. However hiding beneath the outer layers of these worlds, there could also be one thing spectacular: a continuing rain of diamonds.
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“ice giants” might conjure the picture of a Tolkien-esque creature, but it surely’s the identify astronomers use to categorize the outermost planets of the photo voltaic system, Uranus and Neptune.
Confusingly, although, the identify has nothing to do with ice within the sense you’ll usually acknowledge it — as in, say, ice cubes in your drink. The excellence comes from what these planets are manufactured from. The gasoline giants of the system, Jupiter and Saturn, are made nearly fully of gasoline: hydrogen and helium. It is by the speedy accretion of these parts that these enormous planets managed to swell to their present measurement.
In distinction, Uranus and Neptune are made largely of water, ammonia and methane. Astronomers generally name these molecules “ices,” however there actually is not cause for it, besides that when the planets first fashioned, these parts have been doubtless in strong type.
Into the (not so) icy depths
Deep beneath the inexperienced or blue cloud tops of Uranus and Neptune, there’s a variety of water, ammonia and methane. However these ice giants doubtless have rocky cores surrounded by parts which might be in all probability compressed into unique quantum states. In some unspecified time in the future, that quantum weirdness transitions right into a super-pressurized “soup” that typically thins out the nearer you get to the floor.
However fact be instructed, we do not know so much in regards to the interiors of the ice giants. The final time we received close-up knowledge of these two worlds was three many years in the past, when Voyager 2 whizzed by in its historic mission.
Since then, Jupiter and Saturn have performed host to a number of orbiting probes, but our views of Uranus and Neptune have been restricted to telescope observations.
To attempt to perceive what’s inside these planets, astronomers and planetary scientists must take that meager knowledge and mix it with laboratory experiments that attempt to replicate the situations of these planets’ interiors. Plus, they use some good old school math — a variety of it. Mathematical modeling helps astronomers perceive what’s occurring in a given state of affairs primarily based on restricted knowledge.
And it is by that mixture of mathematical modeling and laboratory experiments that we realized Uranus and Neptune might need so-called diamond rain.
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It is raining diamonds
The concept of diamond rain was first proposed earlier than the Voyager 2 mission which launched in 1977. The reasoning was fairly easy: We all know what Uranus and Neptune are manufactured from, and we all know that stuff will get hotter and denser the deeper right into a planet you go. The mathematical modeling helps fill within the particulars, like that the innermost areas of the mantles of those planets doubtless have temperatures someplace round 7,000 kelvins (12,140 levels Fahrenheit, or 6,727 levels Celsius) and pressures 6 million occasions that of Earth’s environment.
Those self same fashions inform us that the outermost layers of the mantles are considerably cooler — 2,000 Ok (3,140 F or 1,727 C — and considerably much less intensely pressurized (200,000 occasions Earth’s atmospheric stress). And so, it is pure to ask: What occurs to water, ammonia and methane at these sorts of temperatures and pressures?
With methane, particularly, the extraordinary pressures can break the molecule aside, releasing the carbon. The carbon then finds its brethren, forming lengthy chains. The lengthy chains then squeeze collectively to type crystalline patterns like diamonds.
The dense diamond formations then drop by the layers of the mantle till it will get too sizzling, the place they vaporize and float again up and repeat the cycle — therefore the time period “diamond rain.”
Lab-grown diamonds
The easiest way to validate this concept could be to ship a spacecraft toUranus or Neptune. That will not be an choice anytime quickly, so we now have to go together with the second-best method: laboratory experiments.
On Earth, we will shoot highly effective lasers at targets to very briefly replicate the temperatures and pressures discovered contained in the ice giants. One experiment with polystyrene (aka Styrofoam) was capable of make nano-sized diamonds. No, Uranus and Neptune do not comprise huge portions of polystyrene, however the plastic was a lot simpler than methane to deal with within the laboratory and, presumably, behaves very equally.
Additionally, Uranus and Neptune can sustain these pressures for lots longer than a laboratory laser, so the diamonds may presumably develop to be so much bigger than nano-sized.
The tip consequence? Based mostly on every part we all know in regards to the composition of the ice giants, their inside buildings, outcomes from laboratory experiments and our mathematical modeling, diamond rain is a really actual factor.
Paul M. Sutter is an astrophysicist at SUNY Stony Brook and the Flatiron Institute, host of “Ask a Spaceman” and “Area Radio,” and writer of “Find out how to Die in Area.”
Study extra by listening to the “Ask A Spaceman” podcast, accessible on iTunes and askaspaceman.com. Ask your personal query on Twitter utilizing #AskASpaceman or by following Paul @PaulMattSutter and fb.com/PaulMattSutter.
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