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There's a Violent Battle Between Solar Wind and Cosmic Rays, and Voyager 2 Just Passed Through it

This illustration shows our solar system suspended in the "bubble" of protective solar wind known as the heliosphere. Where the sphere ends, harsh cosmic rays butt up against our solar system.
Enclosed in a "bubble" of solar wind called the heliosphere, our solar system is relatively safe from the ravages of cosmic rays flying through interstellar space.
(Image: © NASA Goddard Space Flight Center/ Ryan Fitzgibbons, Walt Feimer, Chris Meaney, Swarupa Nune, and Merav Opher))

Solar wind is not exactly our friend. 

The flood of hot, electric particles constantly gushing out of the sun bathes the entire solar system in radiation, frying the occasional satellite and making life impossible on any planet not shielded by an atmosphere. In both a literal and figurative sense, the solar wind blows — but, as new observations from the edge of our solar system suggest, it also protects everything it touches from the even more damaging forces of interstellar space.

As the solar wind flows outward for billions of miles in every direction, it creates a bubble of energy that surrounds our entire solar system. At the edge of this bubble, where the solar wind finally collides with powerful cosmic rays beaming through interstellar space, there is a hot, thick wall of plasma called the heliopause. This cosmic border sits about 120 times farther from the sun than Earth does, where it helps deflect and dilute the powerful radiation released by distant stars and celestial explosions. 

Related: Spaced Out! 101 Astronomy Images That Will Blow Your Mind

Now, in a series of studies published Nov. 4 in the journal Nature Astronomy, astronomers directly analyzed this cosmic frontier for the first time using data collected by NASA's Voyager 2 spacecraft, which passed through the heliopause and into interstellar space a year ago. 

While Voyager 2 was able to cruise seamlessly through the heliopause in about a day, researchers found that the plasma barrier was significantly hotter and thicker than previous studies estimated, effectively forming a physical shield between our solar system and interstellar space. According to study co-author Edward Stone, an astronomer at the California Institute of Technology who has worked on the Voyager program since it launched in 1977, this shield stops about 70% of cosmic radiation from breaking into our solar system.

"The heliopause is the contact surface where two winds [collide] — the wind from the sun and the wind from space, which comes from supernova that exploded millions of years ago," Stone said in a news conference about the new Voyager studies. "Only about 30% of what's outside of the bubble can get in."

This illustration shows Voyager 1 and 2 passing through the heliopause and leaving our solar system — the first man-made interstellar space travelers ever. (Image credit: NASA/JPL-Caltech)

Interstellar robots phone home

In November 2018, NASA's Voyager 2 (V2) satellite passed through the heliopause, becoming only the second man-made object in history to leave our solar system. (The satellite's twin, Voyager 1, became the first in August 2012 — however, Voyager 1 was unable to analyze the border properly due to a sensor malfunction.)

According to radiation data collected by V2 on its interstellar journey, temperatures in the heliopause reached up to 89,000 degrees Fahrenheit (31,000 degrees Celsius) — roughly double the temperature that previous astronomical models predicted, suggesting a far more violent clash between the solar wind and cosmic rays than scientists ever predicted.

While the heliopause's hot, thick wall of plasma protects our solar system from most of the harmful rays darting through space, the researchers also found that the boundaries of the heliopause are not quite as uniform as anticipated. The edge of heliopause is not a perfect "bubble" after all, but contains porous holes that allow interstellar radiation to leak in at certain points. 

Voyager 2 data detected two such holes on our side of the heliopause, where radiation levels spiked much higher than normal background levels before dropping back down again. Eventually, when the levels of cosmic radiation skyrocketed and stayed that way, it was clear the Voyager 2 had entered a new region of space, beyond our sun's domain.

The sheath of hot, charged wind protecting our solar system might not be perfect (and it still might not be our friend) but, as Voyager 2 confirmed, it is part of what separates our cozy cosmic home from the ferocious wilderness of space. For that, perhaps, we should be thankful.

Originally published on Live Science.

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  • kristi276
    There is a region of bow shock wave of super hot plasma that is in the front of our solar system as it plows its way around the Milky Way. Our solar system is traveling at 515,000 miles per hour, although the solar winds are traveling at 400 kilometers per hour. The speed of the cosmic winds are 20 million miles per hour. There is a lot of energy that is coming from all sorts of places, the speed of the solar system, and the speed of the solar wind times the speed of the cosmic winds (20 million miles per hour). All these forces come colliding at one central point; the bow of the solar system. What is the physics involved in all of this mess? Will we ever send a probe into this cosmic soup, as we traverse 515, 000 miles per hour.
  • rod
    How can science show the Sun is moving at 515,000 miles per hour or some 230 km/s? There was a long battle over the geocentric teachers where the Earth was immovable. The heliocentric solar system works but in my studies, does not require the Sun to be moving :)