A University of Iowa-led research team has reported in a new study the most detailed observations to date of the bow shock at Jupiter, our solar system’s gas giant. The findings from NASA’s Juno mission reveal key differences between Jupiter’s bow shock and Earth’s. They also may lead to a better understanding of the physics of how shocks function in even more powerful energy releases, such as those from dying stars. The research is published in Nature Communications.

The bow shock is an invisible boundary between the sun and a planet’s magnetic field. It is the first line of defense against the supersonic burst of energetic particles from the sun known as the solar wind.

On Earth, the bow shock is important because it marks the point where the solar wind is slowed, heated and then deflected around Earth. If that didn’t happen, our planet would be bombarded by the solar wind, and those harmful particles could reach our atmosphere and make Earth less safe for life.