The firewall acts as a filter, deflecting many high-energy cosmic rays. This shield helps reduce radiation exposure within the solar system, playing a role in Earth’s long-term habitability.

At the outer edge of the solar system, solar wind collides with material from interstellar space. This clash creates a “firewall” of charged particles surrounding our system.

Voyager 1 crossed this frontier in 2012, with Voyager 2 following in 2018. Both spacecraft recorded a sudden change in particle density, confirming they had passed through this charged barrier.

Inside the firewall, charged particles from the Sun dominate. Beyond it, particles from the interstellar medium prevail. Voyager’s detectors revealed this sharp transition, showing where the solar system ends.

The firewall acts as a filter, deflecting many high-energy cosmic rays. This shield helps reduce radiation exposure within the solar system, playing a role in Earth’s long-term habitability.

Voyager measured plasma temperatures up to tens of thousands of degrees. However, the particles are so sparse that the spacecraft remains unaffected, offering a reminder that “heat” in space behaves differently.

By recording changes in particle type, density, and energy, Voyager provided the first direct evidence of this frontier, confirming theories that had only existed in models.

The firewall of charged particles is more than a boundary. It defines the edge of the Sun’s influence and helps astronomers understand how other stars protect their planetary systems.