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Extraterrestrial vortex

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An extraterrestrial vortex is a spinning atmospheric pattern found on planets or natural satellites other than Earth. These vortices can only exist on worlds that possess a sufficient atmosphere to support them. Most observed extraterrestrial vortices take the form of large cyclones or anticyclones. A cyclone is a typical storm, while an anticyclone is a vortex that rotates in the opposite direction of the planet's rotation.

PIA21641-Jupiter-SouthernStorms-JunoCam-20170525
PIA21641-Jupiter-SouthernStorms-JunoCam-20170525

These phenomena are critical for scientists to study because they reveal how different atmospheres move and function. They range from massive, long-lasting storms on gas giants to small, seasonal shifts on distant moons.

The mechanisms that drive these vortices vary significantly depending on the planet's composition. On Venus, polar vortices are caused by the Hadley Cell, which is a type of atmospheric circulation in the lower atmosphere. On Saturn's moon Titan, the weather is driven by liquid and gaseous methane and ethane rather than water.

Vortex on saturn's moon titan
Vortex on saturn's moon titan

On Mars, dust storms can trigger the formation of vortices by disrupting particles in the air. Even Mercury, which has a very thin atmosphere, exhibits a unique type of vortex. NASA's MESSENGER mission observed magnetic "tornadoes" in 2008, which are twisted bundles of magnetic fields connecting the planet to space.

Different planets display distinct types and stages of vortex activity. The gas giants, Jupiter and Saturn, and the ice giants, Uranus and Neptune, host the largest vortices in the solar system. Jupiter is unique because 90% of its vortices are anticyclones, unlike the terrestrial atmosphere.

Great Red Spot From Voyager 1
Great Red Spot From Voyager 1

On Saturn, massive "Great White Spots" appear every Saturn year, which lasts about 28 Earth years. These storms are short-lived but can impact the planet's temperature for up to 3 Earth years. Mars also experiences seasonal polar vortices that form over the north pole every winter.

Spacecraft missions have provided the history of these discoveries through direct observation. In 1979, NASA's Pioneer Venus observed a double vortex cyclone at the north pole of Venus. The Hubble Space Telescope detected a rare Martian cyclone in the northern polar region on April 27, 1999. This specific storm consisted of three cloud bands wrapped around a massive eye. On Neptune, the Voyager 2 mission observed the Earth-sized Great Dark Spot in 1989.

Neptune's Great Dark Spot colorcorrected
Neptune's Great Dark Spot colorcorrected

Later, the Hubble Space Telescope saw that this specific spot had vanished by 1994.

The scale of these storms is often much larger than anything found on Earth. Jupiter's Great Red Spot is the largest known extraterrestrial anticyclone. While it was over two Earths wide more than 100 years ago, it is currently about 1.3 Earths wide.

Great Red Spot From Voyager 1
Great Red Spot From Voyager 1

On Neptune, the Great Dark Spot featured wind speeds of approximately 682 kilometers per hour. This vortex rotated around the planet once every 18.3 hours. On Saturn, the hexagonal cyclone at the north pole is nearly 36,000 kilometers in diameter and reaches a depth of about 300 kilometers.

There are many surprising facts regarding the behavior and location of these storms. On Venus, lightning is associated with sulfuric acid clouds instead of water clouds. Most Venusian storms form about 25 miles above the surface, and precipitation evaporates about 20 miles up. On Saturn, a region called "storm alley" exists 35 degrees south of the equator. Scientists still do not know why such a high abundance of storm activity occurs in this specific zone.

Saturn Storm
Saturn Storm

Additionally, the Dragon Storm on Saturn produces radio emissions similar to lightning on Earth.

Studying these vortices helps scientists connect atmospheric science to broader planetary systems. On Titan, the presence of a south polar vortex was imaged in 2012, showing it sits high in the atmosphere. This allows it to be illuminated by the Sun despite the moon's hazy atmosphere.

Vortex on saturn's moon titan
Vortex on saturn's moon titan

On Uranus, researchers hypothesize that large polar caps and dark spots are formed by seasonal changes in atmospheric flow. By observing how these vortices merge, dissipate, or persist, we gain a deeper understanding of the complex fluid dynamics that govern the entire solar system.

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🖼️ Images & Media (10)
File:Mars Before and During Global Dust Storm.jpg
Mars Before and During Global Dust Storm.jpg
File:Mars cyclone.jpg
Mars cyclone.jpg
File:Great Red Spot From Voyager 1.jpg
Great Red Spot From Voyager 1.jpg
File:PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg
PIA21641-Jupiter-SouthernStorms-JunoCam-20...
File:Saturn Storm.jpg
Saturn Storm.jpg
File:Dragon Storm.jpg
Dragon Storm.jpg
File:Vortex on saturn's moon titan.png
Vortex on saturn's moon titan.png
File:Uranus Dark spot.jpg
Uranus Dark spot.jpg
File:Neptune's Great Dark Spot colorcorrected.jpg
Neptune's Great Dark Spot colorcorrected.jpg
File:Small Dark Spot Colored.png
Small Dark Spot Colored.png
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