“Jupiter’s Strange Hotspots” –Windows into a Vast Region Below the Gas Giant’s Clouds



Jupiter's Hotspots


“Giant planets have deep atmospheres without a solid or liquid base like Earth,” said Scott Bolton, the visionary and principal investigator for NASA’s Juno spacecraft, currently orbiting Jupiter after traveling nearly two billion miles, about the discovery by the Galileo probe 25 years ago that the atmosphere it was plunging into was much denser and hotter than scientists expected. But it may have sampled a particularly dry spot and missed more abundant water elsewhere.

“To better understand what is happening deep into one of these worlds,’ said Bolton, “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.”

“Jupiter guards secrets about the early solar system,” says Bolton. “It grabbed most of the leftovers after the Sun formed. When we want to go back and try to understand how the planets were made—where the stuff that made us came from—Jupiter represents that first step.”

Jupiter’s Water Mystery –“Juno Probe Finds Amount Increasing”

New data released from NASA’s Juno spacecraft, reports the JPL, suggests that these “hot spots” are much wider and deeper than anticipated according to 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, when the 75-pound (34-kilogram) probe 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.

New data 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, implying 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.

NASA Juno Probe’s Strange New Discoveries on Jupiter –“The Electric Giant”

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 Université Côte 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 South Pole


Last year the Juno team reported on the cyclones of the south pole shown above. 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.

The Daily Galaxy, Sam Cabot, via NASA/JPL and The Smithsonian


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