New IBEX data show heliosphere's long-theorized bow shock does not exist
The latest refinements in relative speed and local interstellar magnetic field strength prevent the “bubble” that surrounds our solar system from developing a bow shock.
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Southwest Research Institute, San Antonio, Texas —
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May 14, 2012 The heliosphere is the region of space dominated by the Sun that cocoons Earth and the other planets. Inflated by the million-mile-per-hour solar wind, the bubble-shaped heliosphere pushes its way through the galaxy. For a quarter-century, researchers believed a bow "shock" formed ahead of the heliosphere as it moved through interstellar space — similar to the sonic boom made by a jet breaking the sound barrier. New data from NASA's Interstellar Boundary Explorer (IBEX) shows that the heliosphere moves through space too slowly to form a bow shock. Courtesy Southwest Research Institute
The latest refinements in relative speed and local interstellar magnetic field strength prevent the heliosphere, the magnetic "bubble" that cocoons Earth and the other planets, from developing a bow shock. The bow shock would consist of ionized gas or plasma that abruptly and discontinuously changes in density in the region of space that lies straight ahead of the heliosphere.
"The sonic boom made by a jet breaking the sound barrier is an earthly example of a bow shock," said David McComas from the Southwest Research Institute (SwRI) in San Antonio, Texas. "As the jet reaches supersonic speeds, the air ahead of it can't get out of the way fast enough. Once the aircraft hits the speed of sound, the interaction changes instantaneously, resulting in a shock wave."
For about a quarter-century, researchers believed that the heliosphere moved through the interstellar medium at a speed fast enough to form a bow shock. IBEX data have shown that the heliosphere actually moves through the local interstellar cloud at about 52,000 mph (84,000 km/h), roughly 7,000 mph (11,000 km/h) slower than previously thought — slow enough to create more of a bow "wave" than a shock.
"While bow shocks certainly exist ahead of many other stars, we're finding that our Sun's interaction doesn't reach the critical threshold to form a shock, so a wave is a more accurate depiction of what's happening ahead of our heliosphere — much like the wave made by the bow of a boat as it glides through the water," said McComas.
Another influence is the magnetic pressure in the interstellar medium. IBEX data, as well as earlier Voyager observations, show that the magnetic field is stronger in the interstellar medium, requiring even faster speeds to produce a bow shock. Combined, both factors now point to the conclusion that a bow shock is highly unlikely.
The IBEX team combined its data with analytical calculations and modeling and simulations to determine the conditions necessary for creating a bow shock. Two independent global models — one from a group in Huntsville, Alabama, and another from Moscow — correlated with the analytical findings.
"It's too early to say exactly what this new data means for our heliosphere. Decades of research have explored scenarios that included a bow shock. That research now has to be redone using the latest data," said McComas. "Already, we know there are likely implications for how galactic cosmic rays propagate around and enter the solar system, which is relevant for human space travel."
IBEX's primary mission has been to image and map the invisible interactions occurring at the outer reaches of the solar system. Since its launch in October 2008, the spacecraft also has shed new light on the complex structure and dynamics occurring around Earth and discovered neutral atoms coming off the Moon.
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