The solar system, it turns out, is full of volcanoes, but not all of them spew or ooze

liquid rock, like you might tend to picture.

Where it's cold enough, we also see evidence of cryovolcanoes that spit out slushy ices.

So far, we've found them on several gas giant moons and on Pluto.

And we've even found one in the asteroid belt, on the dwarf planet Ceres.

Now, scientists reported this week in Nature Astronomy that they may have discovered up

to 31 more cryovolcano remnants on Ceres.

It's a volcano wonderland.

In 2015, NASA's Dawn spacecraft arrived at Ceres, and it's been mapping and studying

the object's surface ever since.

During its first year, Dawn found one cryovolcano that formed the mountain Ahuna Mons.

It's probably less than 240 million years old, which isn't that ancient when you're

talking about space volcanoes.

To really understand Ceres's history, researchers need to study older volcanoes.

But it's been harder to find any, because the material they're made out of sags and

flattens over time.

At least, that's what astronomers hypothesized.

To confirm that, the team analyzed images of Ceres's surface, looking for large structures

that might be flattened-out former cryovolcanoes, or, as they call them, viscously relaxed domes.

And they found a ton! Including Ahuna Mons, the team spotted a whopping 32 candidates.

Next, they used Dawn's camera to estimate the domes's heights.

For 10 of the 32 structures, they couldn't get clear enough data,

so they were excluded from the analysis.

But the rest were all over 1 kilometer tall.

Based on a set of assumptions, like how large the domes would have been when they started

out, and how much ice they contain, the team estimated the ages of these domes.

This time, they were able to date all but one.

They found that most of the structures were between 2 and 700 million years old,

but a couple were over 2 billion years old.

This all suggests that, over the last billion years,

Ceres got a new cryovolcano every 50 million years or so on average.

Besides teaching us more about Ceres's history, this study also supported the fact that cryovolcanoes

are really different from the hot, lava-spewing mountains on Earth.

For one, the icy magma on Ceres may originate in the dwarf planet's crust,

not in any sort of mantle like we see on terrestrial planets.

Ceres is also a lot less active.

This new study found that the total amount of matter put out by its cryovolcanoes is

between 1000 and 100,000 times less than that of the inner planets and the Moon.

Even if you account for surface area, terrestrial volcanic activity is still an order of magnitude higher.

This could mean that all cryovolcanic bodies, including places like Pluto and Europa,

have similarly low activity, but we'll need more data to know for sure.

Still, any day where you find a bunch of new volcanoes in the asteroid belt is a pretty good day.

Without a telescope or a good pair of binoculars, you probably won't be able to see Ceres from Earth.

But if you look up on a clear night, you might see a light

zooming across the sky for just a few seconds.

It's not a meteor, and it's probably not a UFO.

Instead, it's what's called a satellite flare: a satellite unintentionally catching

the light of the Sun and bouncing it down to you.

The brightest of these are called Iridium flares, but you'll only be able to see them

easily for a little while longer.

So consider this your heads-up.

These flares started around 1997, and they come from a group of

Low-Earth orbit communications satellites.

They're controlled by Iridium Communications Inc., hence the name.

They're not actually made of iridium or anything.

The flares come from sunlight bouncing off the three silver-coated antennae on each satellite.

If the angle is just right, they're bright enough to outshine Venus,

and even to be visible during the day.

But Iridium's network of 66 satellites is being replaced right now,

with a fleet of 75 smaller ones.

These new ones aren't the same shape, so they won't produce any flares.

As of July 2018, there have been seven successful launches to install new, flare-less satellites,

and the eighth and final launch is scheduled for November.

With the new guard coming in, some of the old satellites have already begun de-orbiting,

and they will be spiraling down until they're burned up by the Earth's atmosphere.

But they won't fall out of the sky all at once.

The different satellites all have their own paths to destruction, and for some of them,

that process could take up to 20 years.

So while the number of Iridium flares will drop drastically in the next year or so, you

might manage to catch one every once in a while.

It will just be much harder.

I remember when I was a teen, my dad took me out into the nighttime to be like,

there's the new iridium satellites,

and he timed it so that we could watch it together cuz he's a big nerd.

Today, since the satellites' orbits are actively controlled, it's really easy to

calculate when and where you need to be to see a flare, but that will change soon.

The good news for sky-watchers is that, even once the first Iridium satellites are gone,

other satellite flares will still be out there.

They're just not as spectacular.

And while you and I might be a little sad about that,

at least one group of people will be happy: astronomers.

Since Iridium flares are so bright, they tend to turn up as annoying streaks in study images.

So at least somebody's happy about these satellites

getting destroyed by the friction of the atmosphere.

If you're interested in checking out the last predictable Iridium flares,

the company has some resources to help you out, and we'll leave a link to them in the description.

They even have a bit of a social media campaign about it.

It's called #Flarewell, because they just, I guess they had to do that.

Thanks for watching this episode of SciShow Space News!

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