Weizmann Institute scientists reveal how gigantic cyclones remain stable at both of Jupiter’s poles.

Jupiter, the fifth planet from the Sun and the largest in the solar system, was named after the Roman god Jupiter – the king of the gods – because it is so huge.

Lacking a well-defined solid surface, it is composed mostly of hydrogen gas, but another gas, helium, makes up a quarter of its mass and a tenth of its volume – making it a gas giant with a mass more than two and a half times that of all the other planets in the solar system combined, but slightly less than one-thousandth the mass of the Sun. 

It probably also has a rocky core of heavier elements. Being so large, it is the third-brightest natural object in the Earth’s night sky after Earth’s Moon and Venus


Cyclones at Jupiter’s north pole look like swirls of bold colors. The huge, persistent cyclone found at Jupiter’s north pole is encircled by smaller cyclones that range in size from 4,000 to 4,600 kilometers. Together, this pattern of storms covers an area that would dwarf the Earth.

The US National Aeronautics and Space Administration (NASA) launched its Juno space probe in August 2011, and it reached Jupiter and began to orbit the planet’s in 2016 to measure Jupiter’s composition, gravitational fieldmagnetic field and polar magnetosphere. It was meant also to search for clues about how the planet formed, including whether it has a rocky core, the amount of water present within the deep atmosphere, mass distribution and its deep winds, which can reach speeds up to 620 kilometers per hours. After completing its mission, Juno will be intentionally deorbited into Jupiter’s atmosphere.  

Juno discovered cyclonic vortices thousands of kilometers wide at the gas giant’s poles. What made those cyclones unique compared with others in planetary atmospheres was their configurations — they formed stable, polygonal patterns. The north pole has nine vortices, shown in the photo, and the south pole has six. Except for one temporary interloper at the north pole, the arrangements have remained stable since Juno’s arrival. That stability is surprising because planetary rotation pushes cyclones toward the poles, so storms would be expected to accumulate there and grow in number, or merge, as they do on Saturn. But Jupiter’s cyclone configurations remain stable.

The discovery of the massive Jovian tempest over its south pole occurred in November during its 22nd flyby. When Juno first arrived, its infrared and visible-light cameras discovered giant cyclones encircling both the planet’s poles – nine in the north and six in the south. Were they, like their Earthly siblings, a transient phenomenon, taking only weeks to develop and then ebb? Or could these cyclones, each nearly as wide as the continental US, be more permanent fixtures?

With each flyby, the data reinforced the idea that five windstorms were swirling in a pentagonal pattern around a central storm at the south pole and that the system seemed stable. None of the six storms showed signs of yielding to allow other cyclones to join in.

Before Juno entered its orbit, no one knew that powerful cyclones, approximately the size of Australia, rage across its polar regions. Jupiter’s storms, as opposed to their earthly variety, do not disperse, hardly change, and are clearly not associated with flying rooftops and damp weather reporters. In an article just published in the prestigious journal Nature Geoscience, researchers from the Weizmann Institute of Science in Rehovot revealed the mysteries of Jupiter’s cyclones – which forces are at work fixing these gargantuan storms to their polar locations and why their numbers and locations remain more or less constant over time.

“We can think of Jupiter as an ideal climate laboratory,” noted Prof. Yohai Kaspi of Weizmann’s earth and planetary sciences department. Earth is an intricate and multivariable system; it has oceans and an atmosphere, continents, biology and, of course, human activity. As Jupiter is composed of gas, it is a far easier system to study – one that we can create predictions for and test hypotheses on, he continued. Kaspi, a NASA co-investigator on the Juno mission, witnessed one of its more exciting findings – the cyclone storms swirling around the planet’s poles. 


“If we look at older images of Jupiter taken before 2016,” continued Kaspi, “we see that the poles were commonly represented as large grey areas because no one knew then what they actually look like.” The reason for that is the fact that the solar system is organized on the same plane, which is very close to the plane of Jupiter’s equator. Therefore, past observations of the planet that were carried out from Earth or from earlier space missions could, for the most part, capture only Jupiter’s lower latitudes. 


So one of the Juno mission’s important innovations is its polar orbit, which allowed researchers to observe in detail Jupiter’s tumultuous poles for the first time. This is exactly how the cyclones were exposed, surprisingly organized and resembling a round tray of cinnamon rolls, along latitude 84° N and S. The discovery that the number of cyclones remains fixed – eight are active around the north pole and five around the south, was very surprising at the time,” recalled Kaspi, “because we expected the poles to be more or less symmetric.” In a previous study, Kaspi used the lack of symmetry in Jupiter’s gravitational field to determine the depth of the strong east-west wind belts that are characteristic of the planet’s atmosphere. 


On Earth, tropical cyclonic storms form in areas where the water temperature exceeds 26° Celsius – usually in the center of the Atlantic and Pacific Oceans – and they drift in a circular motion toward the poles, owing to a pull resulting from the planet’s spin. 


On Jupiter, strong jet streams prevent these storms from forming below latitude 60° – only above it are the currents weak enough to allow cyclones to rage on. What causes these particular storms on Jupiter to settle at latitude 84°? According to the new Weizmann study, Jupiter’s cyclones are indeed attracted to the poles, but the polar storm located in the center of the ring of cyclones pushes them away, preventing them from reaching the pole itself. 


“As long at the cyclones remain at a distance from the pole – they are attracted to it. But the nearer they venture – the more strongly they are repelled,” added doctoral student Nimrod Gavriel from Kaspi’s research group, whose thesis focuses on elucidating this phenomenon. “The question is whether the repulsion effect is strong enough to resist the pole’s attraction. Latitude 84° is where these forces even up.” Gavriel and Kaspi proposed a mathematical model that considers the diameter of the polar cyclone (which is larger at the south pole than in the north), the possible minimal distance between each cyclone, the surface area around latitude 84° and the size of the cyclones and their spin, and that accurately predicts the presence of eight cyclones across the north pole. 


As for the south pole, based on their calculations, the number of cyclones should be 5.62. This number is consistent with the data collected by Juno: in reality this number cannot exist, but the five southern storms often separate into six storms, as observed during the probe’s eighteenth and thirty-fourth orbits around Jupiter. The proposed model also explains why this phenomenon is absent on Jupiter’s closest neighboring planet – Saturn. 


“We are trying to understand atmospheric dynamics at a large scale, and providing a successful explanation for the phenomenon of Jupiter’s polar cyclones gives us the confidence that we truly know what’s going on there,” concluded Kaspi. “This confidence may be paramount for us here on Earth, since a deeper understanding of cyclones could aid meteorologists to predict, for example, how the heating up of our planet will affect the movement of storms across it – a challenge that humanity will most likely face in the near future.”


But Kaspi’s fascination with the exploration of Jupiter is more straightforward: “There are no new islands to discover in the Pacific, and most planetary bodies in the solar system have already been mapped. The poles of Jupiter and the other gaseous planets are, perhaps, the last spots in the solar system that are still left to explore. We are expecting more valuable data to come in from Juno during the next couple of years, following the recent extension of the Juno mission to 2025. Owing to gradual changes in the spacecraft’s polar orbit, it is now getting closer and closer to Jupiter’s north pole, allowing us to gain information about this polar region from several specialized instruments.” 



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