Name: 木星の近くに星間小惑星が隠れている (There's an Interstellar Asteroid Hiding Near Jupiter)
Uploaded: 2021-01-14T10:29:04.000Z
Duration: 6 min 11 s
Description: VoiceTubeの動画で発音を聞きながら英語表現を覚えよう！学べる英語：

It was the interstellar asteroid astronomers spotted last fall, and it got everyone all

psyched because it's an interstellar asteroid.

If we want to study a different part of the galaxy we can't do that because we can't

get there but sometimes there comes here!

But, that object was just passing through, though, so scientists didn't have a ton

But this week, according to a paper published Monday in MNRAS: Letters, there's some good

news: We seem to have found another interstellar asteroid.

Except, instead of just visiting our solar system, this one permanently moved in.

The object is named 2015 BZ509, or “Bee-Zed” for short, and it orbits the Sun in a pretty

For one, it moves backwards, or retrograde.

It circles the Sun clockwise, instead of the counter-clockwise motion we see in all of

Its orbit is also pretty elliptical, and it's inclined 163° below the ecliptic, which means

Astronomers first spotted this asteroid in 2015 -- like the name suggests -- but they

originally thought it was just part of a class of objects called Centaurs.

These are objects, both asteroids and other icy bodies, that hang out between Jupiter and Neptune.

For the most part, scientists believe these objeccts originally came from the Kuiper Belt

or the Oort Cloud -- two regions past Neptune -- but got pushed in among the planets by

gravitational encounters with other objects.

Because of all that, their orbits are pretty chaotic!

Like, that's actually the technical term: They are in chaotic orbits, with all kinds

Still, Bee-Zed was always especially weird among the Centaurs.

And this new paper has a hypothesis about why: It's not from around these parts.

The team ran statistical simulations on lots of objects like this asteroid, tracking their

possible orbits over the entire life of the solar system.

And they found that Bee-Zed specifically has an unusual, but really stable orbit.

In fact, it appears that it didn't get nudged toward the Sun like other Centaurs: It's

been hanging around there since the time when the planets formed around 4.5 billion years ago.

But if it's been around for that long, its orbit should be a lot more normal.

It should've formed from the same spinning disk of matter as everything else.

And that would mean it would have a similar orbit to everything else.

The researchers suggest that Bee-Zed could only have such a strange path if it came from

outside the solar system, and was later captured by the Sun's gravity.

Basically, billions of years ago, it immigrated to our neighborhood.

Based on those simulations, it probably wasn't the only one, either.

There may be a bunch of other extrasolar asteroids orbiting on even weirder paths.

The simulations showed lots of potential objects congregating on an orbit perpendicular to

the solar system, which the researchers dubbed the polar corridor.

If it's real — in more than just the math — it would start a long way away from the Sun.

So if these other objects exist, they'd be orbiting really far out there, even into

the Oort cloud around 150 million kilometers away.

And that would help explain why we haven't detected them yet: They'd be really hard to see!

Now, even though this paper made a good case, there's still a chance that Bee-Zed came

There's still a lot we don't know about the regions beyond Neptune, and this simulation

also didn't show the asteroid being directly captured by the Sun or anything.

But it is a good start and hopefully we'll figure out that it definitely is and then

we'll go visit it and it will be like visiting another part of the galaxy without having

Meanwhile, in this week's more local news, scientists may have figured out why Saturn

The planet has at least 62 of them, and lots of the smaller, inner ones have just some

Like, there's Pan, which is shaped kinda like a little empanada, and Atlas, which looks

And then there's Prometheus, which looks vaguely like a burrito.

We've wondered for a while why these tiny moons are shaped the ways they are, and thanks

to a paper published Monday in Nature Astronomy, we think we know!

Based on a combination of modeling processes, the authors suggest those moons got their

shapes from specific kinds of impacts between smaller objects called moonlets.

To get their results, they simulated a bunch of these moonlets using a mix of N-body simulations

and smooth particle hydrodynamic, or SPH, modeling.

N-body simulations describe the gravitational interactions of massive objects hanging out

together, and SPH modeling is great for impacts.

According to these processes, a few things could happen when the moonlets crashed into each other.

Depending on the angle they collided, they could either merge, stick together for a bit

and then separate, or glance off each other in, like, “hit-and-runs”.

In those cases, they didn't merge, and they also probably didn't exchange insurance information.

Most of Saturn's inner moons seem to have formed when the moonlets stuck together.

And their weird shapes were specifically determined by the angle at which they collided.

In the simulation, oblique collision angles gave more oblong, burrito-like shapes, creating

And more direct collision angles made an equatorial ridge, like on Pan and Atlas.

These models also apply to at least one of Saturn's larger, more distant moons, too:

Iapetus, which also has an equatorial ridge.

Of course, we'd figured for a while that collisions were involved somewhere in these

funny shapes, but that's also kind of just the astronomer's fall-back.

Now, we at least have some serious math to back up that hypothesis!

Well, at least for these moons, not for all the other weird stuff in space.

Thanks for watching this episode of SciShow Space News!

If you'd like to keep up to date with the latest news from the solar system and beyond,

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