Twenty-five years ago, NASA sent history's first probe into the atmosphere of the solar system's largest planet. But the information returned by the Galileo probe during its descent into Jupiter caused head-scratching: The atmosphere it was plunging into was much denser and hotter than scientists expected.

New data from NASA's Juno spacecraft suggests that these "hot spots" are much wider and deeper than anticipated. The findings on Jupiter's hot spots, along with an update on Jupiter's polar cyclones, were revealed on Dec. 11, during a virtual media briefing at the American Geophysical Union's fall conference.

"Giant planets have deep atmospheres without a solid or liquid base like Earth," said Scott Bolton, principal investigator of Juno at the Southwest Research Institute in San Antonio.

"To better understand what is happening deep into one of these worlds, you need to look below the cloud layer. Juno, which recently completed its 29th close-up science pass of Jupiter, does just that. The spacecraft's observations are shedding light on old mysteries and posing new questions - not only about Jupiter, but about all gas giant worlds."

The latest longstanding mystery Juno has tackled stems from 57 minutes, 36 seconds of data Galileo beamed back on Dec. 7, 1995. When the probe radioed back that its surroundings were dry and windy, surprised scientists attributed the finding to the fact that the 75-pound (34-kilogram) probe had descended into the atmosphere within one of Jupiter's relatively rare hot spots - localized atmospheric "deserts" that traverse the gas giant's northern equatorial region.

But results from Juno's microwave instrument indicate that the entire northern equatorial belt - a broad, brown, cyclonic band that wraps around the planet just above of the gas giant's equator - is generally a very dry region.

The implication is that the hot spots may not be isolated "deserts," but rather, windows into a vast region in Jupiter's atmosphere that may be hotter and drier than other areas.

Juno's high-resolution data show that these Jovian hot spots are associated with breaks in the planet's cloud deck, providing a glimpse into Jupiter's deep atmosphere.

They also show the hot spots, flanked by clouds and active storms, are fueling high-altitude electrical discharges recently discovered by Juno and known as "shallow lightning." These discharges, which occur in the cold upper reaches of Jupiter's atmosphere when ammonia mixes with water, are a piece of this puzzle.

"High up in the atmosphere, where shallow lightning is seen, water and ammonia are combined and become invisible to Juno's microwave instrument. This is where a special kind of hailstone that we call 'mushballs' are forming," said Tristan Guillot, a Juno co-investigator at the Universite Cote d'Azur in Nice, France.

"These mushballs get heavy and fall deep into the atmosphere, creating a large region that is depleted of both ammonia and water. Once the mushballs melt and evaporate, the ammonia and water change back to a gaseous state and are visible to Juno again."

Jupiter Weather Report
Last year the Juno team reported on the cyclones of the south pole. At that time, Juno's Jovian Infrared Auroral Mapper instrument captured images of a new cyclone appearing to attempt to join the five established cyclones revolving around the massive central cyclone at the south pole.

"That sixth cyclone, the baby of the group, appeared to be changing the geometric configuration at the pole - from a pentagon to a hexagon," said Bolton. "But, alas, the attempt failed; the baby cyclone got kicked out, moved away, and eventually disappeared."

At present, the team doesn't have an agreed-upon theory regarding how these giant polar vortices form - or why some appear stable while others are born, grow, and then die relatively quickly.

Work continues on atmospheric models, but at present no one model appears to explain everything. How new storms appear, evolve, and are either accepted or rejected is key to understanding the circumpolar cyclones, which might help explain how the atmospheres of such giant planets work in general.

Related Links
Juno at NASA
Juno at SWRI
The million outer planets of a star called Sol

Tweet

Thanks for being here; We need your help. The Space Media Network continues to grow but revenues have never been harder to maintain. With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords. Our news coverage takes time and effort to publish 365 days a year. If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.
SpaceMediaNetwork Contributor $5 Billed Once credit card or paypal		SpaceMediaNetwork Monthly Supporter $5 Billed Monthly paypal only

Swedish space instrument participates in the search for life around Jupiter
Stockholm, Sweden (SPX) Nov 19, 2020
The Swedish-led satellite instrument Particle Environment Package (PEP) will help researchers at the Swedish Institute of Space Physics (IRF) to understand how three of Jupiter's icy moons are affected by the particles around Jupiter and search for the pre-conditions for life. After 14 years of work, the instrument is ready to take its place on ESA's Jupiter spacecraft JUICE. Prof. Stas Barbash is the Principal Investigator for the instrument Particle Environment Package (PEP) on board the Europea ... read more