5 Quick Facts About NASA's Juno Mission to Jupiter

What is so risky about Juno’s special maneuver? How close will the spacecraft get to the gas giant, and what does it hope to learn? Here are five quick facts summarizing the excitement around the recent Juno mission to Jupiter.

Sabrina Stierwalt, PhD
5-minute read
Episode #199


Late on the night of July 4th, NASA team members spent a suspenseful 35 minutes watching as the spacecraft Juno attempted to enter the region around the gas giant planet Jupiter, using a risky maneuver known as an orbital insertion. The main goal of this mission is to learn more about the origin and evolution of Jupiter, which will ultimately improve our understanding of how our entire solar system came to be.

What is so risky about Juno’s orbital insertion maneuver? How close will the spacecraft get to the gas giant, and what does it hope to learn? Here are five quick facts summarizing the excitement around the Juno mission.

1. Juno will get closer to Jupiter than any previous spacecraft ever has

Jupiter is surrounded by an intense band of highly energetic charged particles known as a "radiation belt." A planet’s magnetic field offers protection against such particles, but will also cause them to be trapped along the magnetic field lines in toroid, or donut-shaped, belts.

Mercury, Jupiter, Saturn, Uranus, and even Earth are known to have radiation belts. Venus and Mars, however, do not have significant magnetic fields, and so do not have the ability to trap particles. Jupiter has the strongest magnetic field in the solar system, at nearly 20,000 times stronger than that of the Earth.

To protect them from the planet’s intense radiation field, the instruments on board the Juno spacecraft are housed inside a 400-pound titanium vault. The probe will circle the planet 37 times over 20 months, traveling between Jupiter and its radiation belt. That’s about 16 days per orbit, compared to the 90 minutes it takes to traverse a low Earth orbit.

NASA’s Galileo spacecraft orbited the gas giant at a distance larger than 200,000 miles and, despite being heavily shielded, was still damaged by the radiation field. Cassini, NASA’s Saturn-focused mission, only made it to almost 6 million miles away. Juno, however, will come as close as 2,600 miles from the tops of Jupiter’s clouds.

2. NASA only has one shot to get Juno into orbit

Upon its approach to Jupiter, Juno will be the fastest human-made object ever recorded, traveling at 40 miles per second (that's 144,000 miles per hour.) The probe will thus have to slow down significantly to enter into orbit around Jupiter. To do so, Juno will burn its engines for a suspenseful 35 minutes. If the maneuver is not done precisely right – the right timing, the right amount of deceleration, the right positioning – the $1.1 billion spacecraft will miss its entry point and pass by Jupiter, drifting off into space.

3. Data collected by Juno can help settle a debate about how planets, including Earth, are formed

Despite our ability to send probes to view our own planetary backyard close up, and now our ability to detect planets around other stars, there are still major unanswered questions about how such solar systems form.

Formation theories always begin with a collapsing cloud of gas and dust. Most of that material goes into forming a star, like our Sun, and the remainder can be used as building blocks for planets. However, it’s not clear exactly how this is done: do planetary cores form first, and then accumulate their outer layers of gas just through gravitational attraction? Or do particularly large instabilities in that collapsing gas cloud collapse separately to form planets?

Learning more about the make up of Jupiter’s core can help differentiate between these two scenarios, and is thus one of the main goals of the Juno mission. Juno will measure both the gravitational and magnetic fields surrounding the gas giant planet to reveal both the interior structure and mass of the central core.


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About the Author

Sabrina Stierwalt, PhD

Dr Sabrina Stierwalt earned a Ph.D. in Astronomy & Astrophysics from Cornell University and is now a Professor of Physics at Occidental College.