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Our solar system is home to some weird and wonderful weather, with storms more terrifying in scale than anything in Earth's recorded history. From centuries-old hurricanes on Jupiter to immense winds on Neptune, if you leave Earth you'll be shocked by what you find.

Thanks to recent missions into space, we have learned more about these fascinating weather systems than ever before. Scientists are also performing long-term studies of weather systems, such as storms erupting from the Sun that can have direct effects on Earth. As we continue to reach into the unknown, who knows what else there is to discover in the solar system?

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This iconic storm has been raging on Jupiter for centuries, but it may not be around forever. The giant spinning storm is comparable to a hurricane on Earth, although it is considerably larger. It measures about 10,000 miles (16,000 kilometers across), which is roughly 1.3 times the width of our planet. Scientists think its roots go up to 100 times deeper into Jupiter than Earth's oceans. Recent evidence, however, suggests the storm may be shrinking, although it can devour other storms to gain a boost.

That's not the only extreme weather on Jupiter: Its north and south poles have strange arrays of cyclones arranged in a circle, while the intense radiation from the planet bathes some of its moons, such as Io and Europa.

NASA's Juno spacecraft, which entered orbit around Jupiter in 2016, has been collecting incredible data about this gas giant using an array of instruments. This includes a microwave radiometer to measure the deep atmosphere of Jupiter, ultraviolet and infrared cameras to take images of the planet's atmosphere and its aurorae, and JunoCam, which has also been busy snapping visible light images.

By observing radio emissions from the planet, Cassini was also able to 'hear' the storms discharging in the atmosphere. Saturn occasionally develops massive storms that extend more than 190,000 miles (300,000 kilometers), encircling almost the entire planet, while the gas giant's north pole plays host to a weird, permanent hexagon of clouds that extends deep into the planet.

The sun can wreak havoc on our planet. Its solar storms consist of bursts of radiation and charged particles, which can seriously damage satellites that keep a close eye on the sun's activity and prepare for the worst, but occasionally, when a large storm heads our way, satellites and power grids need to be turned off so they can ride it out.

Solar activity has even been suggested to be a possible cause for the sinking of the Titanic. As new research suggests a solar storm behind the impressive northern light show at the time of the sinking could have disrupted the ship's navigation and communication systems and severely hindered rescue operations.

Venus is also the hottest planet in the solar system, but remarkably not the closest to the sun. Its hellishly dense atmosphere blankets the planet and traps heat in a runaway greenhouse effect. As a result, Venusian temperatures can reach 870 degrees Fahrenheit (465 degrees Celsius).

Neptune, the furthest planet from the Sun, has the fastest winds in the solar system. At the planet's highest altitudes, where methane gives Neptune its blue color, winds can reach speeds of more than 1,300 miles (2,100 kilometers) per hour or 1.6 times the speed of sound. These immense winds also give rise to some large storms, such as the famous "Great Dark Spot" seen by the Voyager 2 probe in 1989.

Since then Hubble has kept a watchful eye on Neptune's turbulent storms which rotate clockwise due to the planet's rotation (unlike hurricanes on Earth which are low-pressure systems and rotate counterclockwise). Over the years Hubble has noted the arrival and demise of many Neptunian storms, one of which has recently perplexed scientists.

This particular vortex had been observed sweeping southward toward Neptune's equator, following the path of various storms before it. Though unlike its predecessors this vortex made a sharp U-turn and began to drift back northwards, much to the surprise of researchers.

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It is unlikely that even these dust storms could strand an astronaut on Mars, however. Even the wind in the largest dust storms likely could not tip or rip apart major mechanical equipment. The winds in the strongest Martian storms top out at about 60 miles per hour, less than half the speed of some hurricane-force winds on Earth.

Large global dust storms put enough dust in the air to completely cover the planet and block out the sun, but doing so ultimately dooms the storm itself. The radiative heat of sunlight reaching the surface of the planet is what drives these dust storms.

As sunlight hits the ground, it warms the air closest to the surface, leaving the upper air cooler. As in thunderstorms on Earth, the warm and cool air together become unstable, with warm air rising up and taking dust with it.

Rising plumes of warm air create everything from small dust devils, similar to those that form in deserts on Earth, to larger continent-sized storms. These larger storms sometimes combine into the global storms, which cover the entire planet in atmospheric dust.

Imagine a massive dust storm blanketing the entire North American continent for weeks on end. It sounds like the end of the world, but on Mars, storms of apocalyptic proportions happen several times a year. Every three Martian years or so (every five or six Earth years), one of these regional storms swells up and circles the whole planet with swirling red dust, leaving only the 15 mile-high peak of Olympus Mons peeking above the storm.

Warm air rising from the Martian surface carries the fine-grained dust aloft, where it absorbs more sunlight and radiates its warmth back to the surrounding air. That warm air interacts with cooler air to produce winds that lift more dust. As blowing dust particles brush against each other, they produce a tremendous amount of static electricity, so lightning crackles and sparks throughout the growing storm.

The Great Red Spot is a persistent high-pressure region in the atmosphere of Jupiter, producing an anticyclonic storm that is the largest in the Solar System. It is the most recognizable feature on Jupiter, owing to its red-orange color whose origin is still unknown. Located 22 degrees south of Jupiter's equator, it produces wind-speeds up to 432 km/h (268 mph). Observations from 1665 to 1713 are believed to be of the same storm; if this is correct, it has existed for at least 358 years.[1] It was next observed in September 1831, with 60 recorded observations between then and 1878, when continuous observations began.[2][3]

The Great Red Spot may have existed before 1665, but it could be that the present spot was first seen only in 1830, and was well studied only after a prominent appearance in 1879. The storm that was seen in the 17th century may have been different from the storm that exists today.[4] A long gap separates its period of current study after 1830 from its 17th century discovery. Whether the original spot dissipated and reformed, whether it faded, or if the observational record was simply poor is unknown.[5]

The first sighting of the Great Red Spot is often credited to Robert Hooke, who described a spot on the planet in May 1664. However, it is likely that Hooke's spot was not only in another belt altogether (the North Equatorial Belt, as opposed to the current Great Red Spot's location in the South Equatorial Belt), but also that it was in the shadow of a transiting moon, most likely Callisto.[6] Far more convincing is Giovanni Cassini's description of a "permanent spot" the following year.[7] With fluctuations in visibility, Cassini's spot was observed from 1665 to 1713, but the 118-year observational gap makes the identity of the two spots inconclusive. The older spot's shorter observational history and slower motion than the modern spot makes it difficult to conclude that they are the same.[8]

In the 21st century, the major diameter of the Great Red Spot has been observed to be shrinking in size. At the start of 2004, its length was about half that of a century earlier, when it reached a size of 40,000 km (25,000 mi), about three times the diameter of Earth. At the present rate of reduction, it will become circular by 2040. It is not known how long the spot will last, or whether the change is a result of normal fluctuations.[12] In 2019, the Great Red Spot began "flaking" at its edge, with fragments of the storm breaking off and dissipating.[13] The shrinking and "flaking" fueled speculation from some astronomers that the Great Red Spot could dissipate within 20 years.[14] However, other astronomers believe that the apparent size of the Great Red Spot reflects its cloud coverage and not the size of the actual, underlying vortex, and they also believe that the flaking events can be explained by interactions with other cyclones or anticyclones, including incomplete absorptions of smaller systems; if this is the case, this would mean that the Great Red Spot is not in danger of dissipating.[15]

A smaller spot, designated Oval BA, formed in March 2000 from the merging of three white ovals,[16] has turned reddish in color. Astronomers have named it the Little Red Spot or Red Jr. As of 5 June 2006, the Great Red Spot and Oval BA appeared to be approaching convergence.[17] The storms pass each other about every two years, but the passing of 2002 and 2004 were of little significance. Amy Simon-Miller, of the Goddard Space Flight Center, predicted the storms would have their closest passing on 4 July 2006. She worked with Imke de Pater and Phil Marcus of UC Berkeley as well as a team of professional astronomers beginning in April 2006 to study the storms using the Hubble Space Telescope; on 20 July 2006, the two storms were photographed passing each other by the Gemini Observatory without converging.[18] In May 2008, a third storm turned red.[19] ff782bc1db