As Voyager crossed the heliopause, its detectors recorded a sharp drop in incoming cosmic rays from outside, showing the firewall’s effectiveness as a natural filter.

High-energy cosmic rays constantly travel through the galaxy. Without barriers, they would freely penetrate the Solar System and reach Earth in far greater numbers.

Voyager 1 and 2 confirmed the existence of a firewall at the edge of the Solar System, a region where the solar wind collides with interstellar plasma, forming a turbulent shield.

This firewall slows down and scatters charged particles. Much like a sieve, it prevents the most energetic cosmic rays from directly streaming into the inner Solar System.

As Voyager crossed the heliopause, its detectors recorded a sharp drop in incoming cosmic rays from outside, showing the firewall’s effectiveness as a natural filter.

Even with the firewall in place, some cosmic radiation enters the Solar System. On Earth, the magnetosphere and atmosphere provide a second layer of protection.

The firewall is not static. Its strength changes with the solar wind cycle, expanding when solar activity is high and contracting during quieter periods.

By blocking a large portion of cosmic radiation, the firewall contributes to maintaining a stable radiation environment in the inner Solar System, essential for both planetary habitability and safe human space exploration.