Nine years ago, NASA's Phoenix Mars Lander saw something magical.

It was the middle of the night, and it was snowing on mars.

At the time, mission scientists believed that this snow acted a lot like it does here on

Earth, with individual ice particles drifting down over the course of hours.

But thanks to new research published this week in the journal Nature Geoscience, we

now know that might not be the only way snow falls on Mars.

Instead, just like some storms on Earth, lots of snow might fall

pretty much all at the same time, in what's called a microburst.

The researchers figured this out using a series of computer simulations that divided chunks

of the Martian atmosphere into layers of just a couple hundred meters thick.

It might come as a shock to think that a planet as famously dry as Mars

even has clouds of water at all.

And the Martian atmosphere is definitely pretty dry, but it's also really cold and very

thin, which provides the right conditions for what little water Mars does have to form

into clouds during the day.

Once night falls, though, the temperature drops and some of the ice particles from those

clouds start to sink down.

This vertical motion creates turbulence both inside and below the cloud, resulting in a

process called convection, where cooler air falls toward the planet's surface, taking

nearby ice particles with it.

Rushing air helps dramatically accelerate the snowfall: instead of a single flake taking

hours to fall, convection pushes it down in just minutes.

In most cases, the snow probably vaporizes before it gets to ground level.

But, sometimes, if the clouds are just a kilometer or two above the ground, the end result might

be a blanket of fresh snow on the Martian surface.

Maybe not a blanket of snow.

But, still, It's snow.

On Mars!

The model makes another, more ominous prediction.

On Earth, microbursts are some of the most common causes for plane crashes, especially

during take-off and landing.

So if we ever decide to use drones to study Mars, they could suffer a similar fate.

But, hey, at least some of the craters they would make would be covered in snow!

Snowstorms on Mars weren't the only breakthrough in planetary science announced this week.

We also recreated diamond rain.

With lasers.

That's the key result of a new paper out this week in the journal Nature Astronomy,

where researchers looked into a weird prediction made about the insides of ice giants like

Uranus and Neptune.

The interiors of the giant planets have always been extra-mysterious because they exist at

temperatures and pressures we've only started to be able to create in the lab.

For a long time, we've had to rely on theoretical predictions to tell us what the insides of

these planets might be like, and some of those predictions can be downright weird.

Like, for example, a rain of diamonds falling from the sky.

Uranus and Neptune both contain a bunch of the compound methane,

which is made of a carbon atom and four hydrogens.

Inside these planets, individual methane atoms start linking together

to form chains of carbon-based molecules.

Put those chains under enough pressure and, in theory,

that carbon might become solid diamond.

But that's been hard to test, because we're talking about a lot of pressure —

about 150 Gigapascals.

That's roughly the equivalent of stacking 5000 metric tons on top of a penny,

except with tiny molecules.

That's pretty hard to do, which is where the lasers come in.

To simulate these carbon-based molecular chains, the researchers decided to experiment on a

plastic called polystyrene, which also has a bunch of carbons linked together.

When you shoot a material like polystyrene with a carefully-timed burst of light, you

can create a shockwave of pressure that ripples through it.

To recreate the environment deep inside Neptune, they used a powerful laser to create not one,

but two of those shockwaves.

On their own, neither would have been strong enough.

But when the two waves collided, for just an instant, the material reached the pressure

at which diamonds can form.

The researchers also wanted to see this process in action, which involved timing a burst of

powerful x-rays to coincide with the shockwave collision.

That way they could see what was happening using a technique called x-ray diffraction,

which identifies microscopic materials based on how light reflects off their structure.

And they saw exactly what they had predicted: the pressure formed nanometer-sized diamonds.

In a planet like Neptune, those diamonds could grow thousands of times larger

than the biggest we've ever found on Earth.

Like, millions of carats.

As they fell through the planet's layers of gas, the giant diamonds would collect in

a region surrounding Neptune's core, basically coating it with diamond.

Meanwhile, the hydrogen left over from the original methane

would float up towards the surface.

By separating the heavier carbon from the lighter hydrogen, over time the distribution

of mass and even the size of the planet could change.

Which is important for us to know, because a lot of exoplanets seem to be similar to

Neptune, and their size is one of the things we can measure.

But, let's keep our eyes on the real prize here: Laser diamonds.

It's been a pretty good week for astronomy!

Thanks for watching this episode of SciShow Space News, and if all this talk about snow

made you want to take a ski trip to Olympus Mons,

you can plan your trip while gazing longingly at this SciShow Space ski poster.

Get yours at DFTBA.com/SciShow.

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