Beyond the Sun's bubble, the universe is far stranger than expected

What Will The Voyager Find In Deep Interstellar Space? · 18:43 · Video: Insane Curiosity · Watch at the source

In short: For decades, we viewed interstellar space as a silent void. But as Voyager 1 and 2 pushed past the heliosphere, they encountered a complex landscape of plasma walls, magnetic structures, and cosmic ray storms. We are finally seeing the true face of the space between the stars.

The heliosphere is a protective bubble of charged particles blown outward by the Sun. Its outer boundary, the heliopause, marks the transition into the interstellar medium—a region filled with gas, dust, and particles from other stars. As the solar wind travels outward, it eventually hits the pressure of this interstellar medium. This interaction causes the solar wind to slow abruptly from supersonic speeds to less than the speed of sound at a boundary called the termination shock.

The Voyager probes have provided our first direct look at this frontier. Voyager 1 crossed the heliopause in 2012, while Voyager 2 followed in 2018. Interestingly, both probes crossed at nearly the same distance from the Sun—between 119 and 121.6 astronomical units (AU). This consistency is surprising to scientists because the crossings occurred during different phases of the Sun's 11-year activity cycle: one during a solar minimum and the other during a solar maximum.

The data reveals that the heliosphere is not a static structure; it is 'breathing.' It expands and contracts over time and experiences shorter-term perturbations caused by coronal mass ejections—massive explosions of solar plasma. Beyond the heliopause, the Voyagers are detecting mysterious magnetic fields, dense plasma walls, and signals that scientists are still struggling to fully explain. These measurements are helping us piece together the first real picture of the edge of our solar system's influence.

While the Voyagers were originally designed to study the giant planets like Jupiter and Saturn, they have become our primary tools for understanding the interstellar medium. They are currently measuring the magnetic fields and plasma waves of the deep cosmos, pushing the limits of what human-made technology can endure in the cold, tenuous environment of deep space.

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