Space

Boom! Juno within Jupiter’s magnetosphere

On July 4, 2016 – at 8:18 p.m. PDT (July 5 at 0318 UTC) – NASA’s solar-powered Juno spacecraft will begin moving into orbit around Jupiter. One of the mission goals is to understand Jupiter’s enormous magnetosphere, the magnetic environment surrounding the planet.

Click here for links that’ll help you follow the Juno mission

Juno crossed the boundary into Jupiter’s immense magnetic field on June 24, 2016. The craft’s Waves instrument recorded the encounter with the bow shock over the course of about two hours. Bow shock – analogous to a sonic boom on Earth – is where the supersonic solar wind is heated and slowed by Jupiter’s magnetosphere.

The next day, June 25, 2016, the Waves instrument witnessed the crossing of the magnetopause. In the video above, trapped continuum radiation refers to waves trapped in a low-density cavity in Jupiter’s magnetosphere.

Planets’ magnetic environments don’t exist in isolation. They’re the result of a collision between a planet’s intrinsic magnetic field and the supersonic solar wind. NASA said :

Jupiter’s magnetosphere – the volume carved out in the solar wind where the planet’s magnetic field dominates – extends up to nearly 2 million miles (3 million km). If it were visible in the night sky, Jupiter’s magnetosphere would appear to be about the same size as Earth’s full moon.

As Juno orbits Jupiter in the coming months and years, we’ll learn more!

Read about Juno and Jupiter’s magnetosphere from NASA

Scientists will use the twin magnetometers aboard NASA's Juno spacecraft to gain a better understanding about how Jupiter's magnetic field is generated. Image via NASA Goddard Space Flight Center
Scientists will use twin magnetometers aboard the Juno spacecraft to learn how Jupiter’s magnetic field is generated. Image via NASA Goddard Space Flight Center

Bottom line: NASA video discusses how the Juno mission, arriving at Jupiter on July 4, 2016, will explore the planet’s massive magnetosphere.

Posted 
July 3, 2016
 in 
Space

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