Juno: Surprises in First Science Results

From its dynamic atmosphere to its hidden depths, Juno reveals Jupiter as never before.

Juno at Jupiter

An artist's conception of Juno in orbit around Jupiter.
NASA

Forget what you thought you knew about Jupiter. The first science results are in from NASA's Juno spacecraft, currently in orbit around Jove. The findings were published in this week's Science and Geophysical Research Letters today, along with a salvo of press releases.

For starters, there was this eye-popping, never-before-seen sequence of Jupiter's aurorae, captured by Juno's Ultraviolet Spectrograph. The long-tailed "comet" on the left is the footprint of an electromagnetic connection to the moon Io:

 

Juno's orbit takes it around Jupiter once every 53 days, from a perijove 2,500 miles (4,000 km) above the Jovian cloud tops, to a five million mile (8 million km) apojove out past the orbit of Callisto. Original plans called for Juno to enter a tighter, 14-day-long orbit around Jupiter, but NASA decided to keep Juno in its present initial capture orbit after a helium valve engine anomaly turned up during a course correction burn last October. Juno will complete eight more planned orbits and was granted a brief reprieve as its final disposal via atmospheric entry won't occur now until July 2018.

Comparing Gas Giants

It has been a thrilling ride, as Juno scans Jupiter in detail from pole-to-pole once every pass in a whirlwind six hour science phase. Juno completed its sixth perijove pass earlier this week. Unlike what Cassini is seeing on its Grand Finale orbits around Saturn, however, the poles of Jupiter are chaotic and complex.

Juno's view

Juno's swift and changing view as it passed from one pole of Jupiter to another through perijove on May 19th.
NASA / MSSS / SwRI / Gerald Eichstädt / Seán Doran

"We knew, going in, that Jupiter that Jupiter would throw us some curves," says Scott Bolton (Southwest Research Institute) in a NASA press release. "But now that we are here we are finding that Jupiter can throw the heat, as well as knuckleballs and sliders. There is so much going on here that we didn't expect, that we have to take a step back and begin to rethink of this as a whole new Jupiter."

Jupiter white spot

A swirling white spot captured by Juno on February 2nd.
NASA / MSSS / JPL / SwRI / Bjorn Jonsson

Thus far, Juno has delivered unparalleled views of Jupiter's poles, revealing complex cloud festoons and enigmatic white ovals and cyclones the size of the Earth. Pioneer 11 in 1974 and the Ulysses flyby of Jupiter in 1992 provided the only other polar views of Jupiter, and these were from much greater distances.

Here's a highlight rundown of the first science findings of Juno at Jupiter:

Infrared Jupiter

A full disk rotation video of Jupiter in the infrared captured by Juno's JIRAM instrument.
NASA/J.E.P. Connerney et al/Science

Atmosphere: Sounding by Juno's Microwave Radiometer instrument points towards a robust cycling of the ammonia clouds shrouding the planet and an ammonia-based weather cycle extending deep below the cloud tops. This ammonia stream is evident racing around Jupiter's equatorial belt — Jupiter rotates once every 10 hours, the fastest spin of any planet in the solar system — but Juno sees this ammonia belt extending deeper than expected, to a depth of at least 300 km. In fact, the main ammonia-rich plume near the Northern Equatorial Belt resembles a larger version of the Hadley Cell circulation seen in the equatorial regions of the Earth.

Just what powers the swirling storms near Jupiter's poles, and why does the northern pole of the planet differ dramatically from the south? "We're questioning whether this is a dynamic system," Says Bolton in a recent press release. "Are we seeing just one stage, and over the next year, we're going to watch it disappear, or is this a stable configuration and these storms are circulating around one another?"

Jupiter core

A possible textbook "slice of Jupiter" due for revision? The upper meteorological layer, versus a possible deep rocky core.
NASA / JPL / SwRI

Gravitational field: The orbit of Juno makes it an ideal platform to plumb the extent of Jupiter's gravitational field, giving scientists a chance to understand the interior structure of the planet. By carefully tracking Juno's motion, engineers back on Earth can detect minute changes in the planet's attractive force on the spacecraft.

Previous models featured sharp demarcations between transition layers, with perhaps a metallic liquid hydrogen core enveloping a bizarre high pressure zone of helium precipitation. Juno's preliminary findings, however, challenge this assertion and suggest instead a large but indistinct “fuzzy” core diluted with layers that are intermixing. Understanding whether or not Jupiter has a solid core is a key mystery in planetary formation.

Jupiter magnetic field

Jupiter's lumpy magnetic field from north to south. The black line represents the track on Jupiter directly below the spacecraft during one of its perijove passes.
NASA / MSSS / SwRI / Caltech

Finally, Juno delivered another surprise. Jupiter's magnetic field is not only almost twice as strong as expected in spots, but it's not uniform. These results come from Juno's magnetometer and microwave radiometer. Specifically, the field strength peaks near 8 to 9 gauss, nearly twice the expected 5 gauss. Earth's magnetic field is a paltry 0.3 to 0.7 gauss: for comparison, a typical refrigerator magnet has a field of about 50 gauss, powerful over short distances. Juno also recorded variances in the magnetic field map surrounding Jupiter up to 2 gauss. This strongly suggests that the dynamo generating the field is relatively shallow, rather than the deep-seated engine driving the magnetic field emanating from Earth's core.

Jupiter

A close up along Jupiter's terminator from March 27th, showing the "STB Spectre" feature (the blue streak, right half of the image).
NASA / MSSS / Caltech / SwRI / Roman Tkachenko

Radiation: The mission has provided another unique plus, with spectacular closeups of aurora over both poles of Jupiter. Jovian aurora have been seen by the Hubble Space Telescope orbiting the Earth, and Juno has now chronicled these up close, along with the footprint of the powerful Io flux tube extending from the innermost Galilean moon. JunoCam and Jovian Infrared Auroral Mapper (JIRAM) are the prime instruments monitoring Jovian aurora.

Thus far, Juno has navigated through the intense radiation field surrounding Jupiter relatively unscathed. The main spacecraft bus is shielded within a sturdy titanium housing.

Juno is the first outer solar system mission powered by three solar panels instead on a plutonium-fueled generator. And those panels are huge, each 29½ feet (9 meters) long. Engineers noticed "flecks of light" traveling across Juno's navigational star camera field of view, which were traced back to micrometeoroid impacts along its three huge solar panels. Like with LISA Pathfinder, researchers soon realized that Juno can also serve as a micrometeoroid detector, the largest ever flown.

But that's not all that the star trackers saw. Gaze upon the Jovian ring system seen, for the first time, from the planet's perspective:

rings of Jupiter

The first ever view of Jupiter's tenuous rings, looking from the inside out. Captured by Juno's Stellar Reference Unit SRU-1, watchers will note the Belt of Orion asterism (lower right) and the bright star Betelgeuse (just above the ring).
NASA / MSSS / Caltech / SwRI

More science is sure to come, as researchers analyze Juno data. We've got just over a year remaining to this exciting mission to unravel the secrets of the largest planet in the solar system.

6 thoughts on “Juno: Surprises in First Science Results

  1. kdconodkdconod

    There’s some funny math here…last perijove was May 19. End of mission is in July 2018. Not sure of exact date but just for a back-of-the-envelope calculation, the time between May 19 and the end of July 2018 is only enough for 8 orbits. There’s no way Juno will reach 33 orbits as mentioned above.

  2. Roger

    Fascinating stuff!

    With regard to the aurora images of Jupiter’s South Pole, I note that the South Pole is currently tilted toward Earth by 2.74 degrees. (Jupiter’s obliquity is only 3.12 degrees) Thus, the aurora images are in daylight. Were they narrow waveband images? Ultraviolet? Or, is the aurora so bright that it can be imaged in integrated light?

    Despite the small obliquity, each pole spends about 6 Earth-years in darkness during the Jovian year. It is reasonable to suspect that the atmospheric circulations at the poles would be somewhat different according to the season of the Jovian year. Is Juno able to make IR images of the North Pole now, while it is not illuminated by the Sun, or are the researchers’ comments based only on what they see at the South Pole?

  3. philip-gardner

    Not being a physicist or space junkie, I wonder if the core of Jupiter is not one of those weirdo asteroid shapes we keep seeing and the rotating magnetic field would be unbalanced, wacking ammonia and other gasses on the way, spitting it out then sucking it back in as it passes every 10 hours? Its a wild ride out there. Great results. Congratulations to all on the Juno project.

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