Huge Magnetic Bubbles May Churn at Solar System's Edge

Old and new views of the heliosheath. Red and blue spirals are the gracefully curving magnetic field lines of orthodox models. New data from Voyager add a magnetic froth (inset) to the mix.
Old and new views of the heliosheath. Red and blue spirals are the gracefully curving magnetic field lines of orthodox models. New data from Voyager add a magnetic froth (inset) to the mix. (Image credit: NASA)

The edge of the solar system is a turbulent place, filled with a roiling sea of huge magnetic bubbles, new research suggests.

The find, made with the help of observations from NASA's venerable Voyager probes, shakes up prevailing views of the solar system's outer reaches. And it shows that this region, once thought to be a relatively firm shield against interstellar particles such as galactic cosmic rays, is actually more of a porous membrane.

"We will have to change our view of how the sun interacts with particles, fields and gases from other stars," Arik Posner, a Voyager program scientist at NASA Headquarters in Washington, D.C., told reporters today (June 9).

Not smooth, but bubbly

Our sun's sphere of influence, composed of solar plasma and solar magnetic fields, is called the heliosphere. This gigantic structure is about three times wider than the orbit of Pluto. At the edge of the heliosphere lies the heliosheath, a boundary region between the solar system and interstellar space.

For decades, scientists had thought that, in the heliosheath, the sun's magnetic field curves around in a smooth, consistent arc, forming a relatively uniform structure. [Solar System Explained From the Inside Out]

But that appears not to be the case.

An artist's concept of the Voyager 1 and Voyager 2 probes near interstellar space. (Image credit: NASA/JPL [Full Story])

The twin unmanned probes Voyager 1 and Voyager 2, both launched in 1977, are currently plying different parts of the heliosheath, more than 9 billion miles (14.5 billion kilometers) from Earth. And their observations are spurring a rethink of the region. [5 Facts About NASA's Voyager Spacecraft]

Specifically, the probes measured abrupt changes in the flow of particles, such as electrons, from one patch of space to another.

"What really struck us were the sudden differences between what Voyager 1 was seeing and what Voyager 2 was seeing," said study co-author James Drake of the University of Maryland. "We had to explain, well, why is that?"

The best explanation, according to subsequent computer models, is that the probes are flying through a frothy field of magnetic bubbles. These bubbles act as particle traps. So particle readings increase while the spacecraft are inside one, then drop when they exit.

These bubbles form as a result of the interaction between the sun's rotation and its magnetic field. As the sun spins, its magnetic field churns and twists out in the heliosheath. The folded field bunches up on itself, causing lines of magnetic force to crisscross and reconnect, forming the sea of bubbles.

Huge, sausage-shaped bubbles

The sausage-shaped bubbles are gigantic, measuring about 100 million miles (161 million km) across. And there are a lot of them. [Amazing New Sun Photos from Space]

"This entire thing is bubbly, just like the most bubbly parts of your Jacuzzi," Drake said. He added that an observer flying aboard one of the Voyagers would not be able to see the bubbles, because the gas in the area is too diffuse.

Researchers are confident that this interpretation best fits the Voyager data, though they'd love some more information from newer, more advanced spacecraft as well. So the team is pushing for new missions to further explore this enigmatic region.

"We are pretty confident of this scenario," said study lead author Merav Opher of Boston University. But, she added, "we need more sensitive instruments with a better suite to really uncover what's happening. We are just scraping the surface."

The researchers report their findings in the June 9 issue of the Astrophysical Journal.

A porous shield

Astronomers had imagined that a smooth, laminar heliosheath acted as a pretty stout shield around the solar system, keeping out many fast-moving particles known as galactic cosmic rays.

Cosmic rays are a threat to astronauts, as they can slam into spaceflyers' cells and damage their DNA. Earth's atmosphere attenuates cosmic rays, shielding folks on the ground from their worst effects.

However, the sea of bubbles likely acts more like a membrane than a shield, researchers said, potentially letting some of these particles zip through into the inner solar system. But scientists don't fully understand how the membrane works and just what is able to pass through it.

The bubbles may trap cosmic rays for a while, forcing them to bounce around like pinballs before they finally escape. Figuring out which one of these scenarios is accurate could have a huge bearing on our understanding of the interstellar space environment. If the bubbles are leaky like a sieve, for example, it implies that there may not be as many galactic cosmic rays out there as researchers had thought.

This is just one question of many that astronomers will be tackling now, thanks to the new results.

"We are still trying to wrap our minds around the implications of these findings," Drake said.

Voyager 1 is now about 11 billion miles (17.7 billion kilometers) from Earth, while Voyager 2 is about 9 billion miles (14.5 billion km) away. Voyager 1 is the most far-flung human-made object in the universe.

You can follow senior writer Mike Wall on Twitter: @michaeldwall. Follow for the latest in space science and exploration news on Twitter @Spacedotcom and on Facebook.

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Mike Wall
Senior Space Writer

Michael Wall is a Senior Space Writer with and joined the team in 2010. He primarily covers exoplanets, spaceflight and military space, but has been known to dabble in the space art beat. His book about the search for alien life, "Out There," was published on Nov. 13, 2018. Before becoming a science writer, Michael worked as a herpetologist and wildlife biologist. He has a Ph.D. in evolutionary biology from the University of Sydney, Australia, a bachelor's degree from the University of Arizona, and a graduate certificate in science writing from the University of California, Santa Cruz. To find out what his latest project is, you can follow Michael on Twitter.