Cloud vortices off Heard Island, south Indian Ocean. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA’s Aqua satellite captured this true-color image of sea ice off Heard Island on Nov 2, 2015 at 5:02 AM EST (09:20 UTC). Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team

Cloud vortices off Heard Island, south Indian Ocean. The Moderate Resolution Imaging Spectroradiometer (MODIS) aboard NASA’s Aqua satellite captured this true-color image of sea ice off Heard Island on Nov 2, 2015 at 5:02 AM EST (09:20 UTC). Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagrid.me/nasagoddard/?vm=grid" rel="nofollow">Instagram</a></b>

NASA image acquired August 14, 2010 at 14:55 UTC Cloud vortices off Madeira and Canary Islands Satellite: Aqua Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team Click here to see more images from <b><a href="http://rapidfire.sci.gsfc.nasa.gov/gallery/?latest" rel="nofollow">MODIS</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Join us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a><b></b></b>

STS040-75-003 (5-14 June 1991) --- This image shows several of the Canary Islands, located in the North Atlantic Ocean just west of Africa. Low level stratus clouds often form here (and along the west coast of continents at these latitudes) are trapped in vertical movement due to an overlying atmospheric temperature inversion. The islands are generating disturbances in the low-level wind flow which is generally from the north-northeast or from top to bottom in the image. These disturbances travel downstream from the islands and manifest themselves as cloud swirls which are called von Karman vortices. The northern extent of a large dust storm moving off the coast of Africa is apparent at the lower right of the image. The dust, extended across the Atlantic Ocean as far west as the Dominican Republic later in the mission.

Stable, south flowing air over the western Pacific Ocean (26.0N, 131.0E) is disturbed by islands south of Korea, resulting in sinuous clouds known as von Karman vortices. The smoke plume from Japan's Mount Unzen Volcano on Kyushu, is visible just west of the large cloud mass and extending southward. A very large, purple tinged dust pall, originating in Mongolia, can be seen on the Earth's Limb, covering eastern China and extending into the East China Sea.

Two bright vortices roll across the cloud-lined face of Saturn, where winds howl at high speeds never experienced on Earth

Bright, high altitude clouds, like those imaged here, often appear more filamentary or streak-like than clouds imaged at slightly deeper levels in Saturn atmosphere. This view also shows one of the many cat eye vortices.

S65-63150 (16 Dec. 1965) --- Eddies in stratocumulus clouds over the Canary Islands as seen from the Gemini-6 spacecraft during its 14th revolution of Earth. Photo credit: NASA or National Aeronautics and Space Administration

ISS015-E-09199 (23 May 2007) --- Von Karman cloud vortices near the Aleutian Islands are featured in this image photographed by an Expedition 15 crewmember on the International Space Station. The vortices are created by the wind encountering a barrier such as an island, changing direction and velocity and forming eddies in the wind and cloud pattern on the lee side of the island. The nadir point of the space station when the image was taken was 51.1 degrees north latitude and 178.8 degrees west longitude.

STS083-749-079 (4-8 April 1997) --- Cloud wake covers the Leeward Islands. Like a ship making a wake in the water, Guadeloupe Island is making a wake in the clouds. Seeing certain weather features tells us information as to what the conditions were at the time the photo was taken. For instance, a solid cloud area is formed behind the island in this photo so the winds are under or at 5 meters per second (mps). If the winds were greater Von Karman Vortices would develop. Formation of Von Karman Vortices requires wind speeds of 5 and 13 mps and a strong low level temperature inversion below the highest peak of the island.

ISS002-E-7710 (21 June 2001) --- Commonly visible cloud vortices hover in the area of the Canary Islands off the coast of Morocco in this Expedition Two digital still camera's view from the International Space Station (ISS).

S125-E-007900 (16 May 2009) --- A nadir view of cloud vortices in the area of the Canary Islands in the North Atlantic Ocean was recorded by one of the STS-125 crewmembers on a busy flight day six.

SL4-140-4111 (14 Jan. 1974) --- The Aleutian Islands area of Alaska, as photographed from the Skylab space station in Earth orbit by one of the Skylab 4 crewmen. The camera used was a hand-held Hasselblad, with SO-368 medium-speed Ektachrome. Here is another macro scale phenomenon which is difficult to observe except from a space platform. The Aleutian Islands and clouds with very elaborate van Karman vortices was photographed on Jan. 14, 1974. In addition to the vortices the waves in the clouds due to the mountains on the islands are very evident. In fact, the easiest way to find the mountains is to start with their atmospheric disturbance and work back to the mountain. Photo credit: NASA

P-21742 BW Range: 6 million kilometers (3.72 million miles) This Voyager 2 image shows the region of Jupiter extending from the equator to the southern polar latitudes in the neighborhood of the Great Red Spot. A white oval, different from the one observed in a similiar position at the time of the Voyager 1 encounter, is situated south of the Great Red Spot. The region of white clouds now extends from east of the red spot and around its northern boundary, preventing small cloud vortices from circling the feature. The disturbed region west of the red spot has also changed since the equivalent Voyager 1 image. It shows more small scale structure and cloud vortices being formed out of the wave structures.

P-21742 C Range: 6 million kilometers (3.72 million miles) This Voyager 2 image shows the region of Jupiter extending from the equator to the southern polar latitudes in the neighborhood of the Great Red Spot. A white oval, different from the one observed in a similiar position at the time of the Voyager 1 encounter, is situated south of the Great Red Spot. The region of white clouds now extends from east of the red spot and around its northern boundary, preventing small cloud vortices from circling the feature. The disturbed region west of the red spot has also changed since the equivalent Voyager 1 image. It shows more small scale structure and cloud vortices being formed out of the wave structures.

ISS040-E-016570 (21 June 2014) --- From an altitude of 223 nautical miles, one of the Expedition 40 crew members on the International Space Station photographed this nearly vertical image of Guadalupe Island and the Von Karman cloud vortices that are its storied neighbors just off southern California's Pacific Coast.

ISS040-E-016569 (21 June 2014) --- From an altitude of 223 nautical miles, one of the Expedition 40 crew members on the International Space Station photographed this nearly vertical image of Guadalupe Island and the Von Karman cloud vortices that are its storied neighbors just off southern California's Pacific Coast.

ISS036-E-035663 (24 Aug. 2013) --- One of the Expedition 36 crew members aboard the International Space Station recorded this still image of unusual cloud patterns surrounding Guadalupe Island in the Pacific Ocean (left center). These are the result of a ubiquitous occurrence in the motion of fluids—a vortex street, which is a linear chain of spiral eddies called von Karman vortices. Von Karman vortices are named after Theodore von Karman, a co-founder of NASA's Jet Propulsion Laboratory. who first described the phenomenon in the atmosphere. Guadalupe Island or Isla Guadalupe is a volcanic island located 241 kilometers (150 statute miles) off the west coast of Mexico's Baja California peninsula.

ISS030-E-254259 (22 April 2012) --- Cloud vortices off the Pacific coast of Mexico's Baja California were captured by one of the six expedition 30 crew members aboard the International Space Station as three of their number ready for their return trip to Earth in a few days. The Gulf of California or Sea of Cortez is completely clear of clouds as are the inland parts of Mexico and California pictured. The Salton Sea is visible at the lower right edge.

STS080-752-011 (19 Nov.-7 Dec. 1996) --- This view, photographed by one the crewmembers aboard the Earth-orbiting space shuttle Columbia, shows an area covered with clouds near the terminator thus the long shadows from the towering clouds. A portion of the vertical stabilizer of the space shuttle Columbia is seen on the right. Vortices indicate that it is a Southern Hemisphere photograph.

This image captures swirling cloud belts and tumultuous vortices within Jupiter's northern hemisphere. NASA's Juno spacecraft took this color-enhanced image at 10:23 p.m. PDT on May 23, 2018 (1:23 a.m. EDT on May 24), as the spacecraft performed its 13th close flyby of Jupiter. At the time, Juno was about 9,600 miles (15,500 kilometers) from the planet's cloud tops, above a northern latitude of 56 degrees. The region seen here is somewhat chaotic and turbulent, given the various swirling cloud formations. In general, the darker cloud material is deeper in Jupiter's atmosphere, while bright cloud material is high. The bright clouds are most likely ammonia or ammonia and water, mixed with a sprinkling of unknown chemical ingredients. A bright oval at bottom center stands out in the scene. This feature appears uniformly white in ground-based telescope observations. However, with JunoCam we can observe the fine-scale structure within this weather system, including additional structures within it. There is not significant motion apparent in the interior of this feature; like the Great Red Spot, its winds probably slows down greatly toward the center. Citizen scientists Gerald Eichstädt and Seán Doran created this image using data from the spacecraft's JunoCam imager. The view is a composite of several separate JunoCam images that were re-projected, blended, and healed. https://photojournal.jpl.nasa.gov/catalog/PIA22424

NASA image acquired September 15, 1999 This Landsat 7 image of clouds off the Chilean coast near the Juan Fernandez Islands (also known as the Robinson Crusoe Islands) on September 15, 1999, shows a unique pattern called a “von Karman vortex street.” This pattern has long been studied in the laboratory, where the vortices are created by oil flowing past a cylindrical obstacle, making a string of vortices only several tens of centimeters long. Study of this classic “flow past a circular cylinder” has been very important in the understanding of laminar and turbulent fluid flow that controls a wide variety of phenomena, from the lift under an aircraft wing to Earth’s weather. Here, the cylinder is replaced by Alejandro Selkirk Island (named after the true “Robinson Crusoe,” who was stranded here for many months in the early 1700s). The island is about 1.5 km in diameter, and rises 1.6 km into a layer of marine stratocumulus clouds. This type of cloud is important for its strong cooling of the Earth’s surface, partially counteracting the Greenhouse warming. An extended, steady equatorward wind creates vortices with clockwise flow off the eastern edge and counterclockwise flow off the western edge of the island. The vortices grow as they advect hundreds of kilometers downwind, making a street 10,000 times longer than those made in the laboratory. Observing the same phenomenon extended over such a wide range of sizes dramatizes the “fractal” nature of atmospheric convection and clouds. Fractals are characteristic of fluid flow and other dynamic systems that exhibit “chaotic” motions. Both clockwise and counter-clockwise vortices are generated by flow around the island. As the flow separates from the island’s leeward (away from the source of the wind) side, the vortices “swallow” some of the clear air over the island. (Much of the island air is cloudless due to a local “land breeze” circulation set up by the larger heat capacity of the waters surrounding the island.) The “swallowed” gulps of clear island air get carried along within the vortices, but these are soon mixed into the surrounding clouds. Landsat is unique in its ability to image both the small-scale eddies that mix clear and cloudy air, down to the 30 meter pixel size of Landsat, but also having a wide enough field-of-view, 180 km, to reveal the connection of the turbulence to large-scale flows such as the subtropical oceanic gyres. Landsat 7, with its new onboard digital recorder, has extended this capability away from the few Landsat ground stations to remote areas such as Alejandro Island, and thus is gradually providing a global dynamic picture of evolving human-scale phenomena. For more details on von Karman vortices, refer to <a href="http://climate.gsfc.nasa.gov/~cahalan" rel="nofollow">climate.gsfc.nasa.gov/~cahalan</a>. Image and caption courtesy Bob Cahalan, NASA GSFC Instrument: Landsat 7 - ETM+ Credit: NASA/GSFC/Landsat <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Join us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b>

STS100-710-182 (19 April-1 May 2001) --- Easily recognizable in this STS-100 70mm frame are phenomena known as the von Karman vortices, which were forming in the stratocumulus field downwind from the volcanic island of Rishiri-to in the northern Sea of Japan off the northwest coast of Hokkaido, Japan. According to NASA scientists studying the STS-100 photo collection, these features form when a stable atmosphere with low clouds flows past a relatively small obstacle with a height greater than the depth of the cloud layer. Because the atmosphere is stable, a series of eddies form in the moving cloud field.

ISS024-E-014559 (14 Sept. 2010) --- Hurricane Igor is featured in this Sept. 14 image photographed by an Expedition 24 crew member on the International Space Station. At the time this image was taken, Hurricane Igor was about 648 miles east of Barbuda Island in the Lesser Antilles. It was travelling to the northeast (290 degrees) at 6.2 mph (6 kts). The winds were already 132.5 mph (115 kts) gusting to 161.3 mph (140 kts) and forecast to intensify. Igor?s well-defined eye was a dynamic area of swift rising winds in the outer wall and sinking winds in the center. His strong eye wall surrounded a low level cloud deck of clouds containing additional vortices.

ISS040-E-016422 (20 June 2014) --- One of the Expedition 40 crew members aboard the International Space Station used a 28mm focal length to record this long stretch of California's Pacific Coast on June 20, 2014. Guadalupe Island and the surrounding von Karman cloud vortices over the Pacific can be seen just above frame center. San Diego is visible in upper left and the Los Angeles Basin is just to the left of center frame. Much of the Mojave Desert is visible in bottom frame.

STS099-703-007 (11-22 February 2000) ---A distinct cumulus cloud pattern marks the island wake within a weak northerly wind field in the vicinity of Isla Socorro, south of the Baja Peninsula of Mexico. The photo was taken by one of the astronauts aboard the Space Shuttle Endeavour as it orbited Earth in February 2000. A smaller companion island, San Benedicto, is visible to the north-northeast. Socorro rises to just over 3,400 feet and disrupts the winds which apparently are not strong or persistent enough to form closed vortices.

As the air blows over the tops of the mountain peaks, seen here in the clear region, the direction of the air flow is disturbed. These disturbances in the flow pattern are generally small circular eddies with one circulating in a clockwise direction and the next in the reverse direction. The wind here has caused the shallow cloud cover to change accordingly. These eddies are commonly called von Karmen Vortices.

As NASA's Juno mission completed its 43rd close flyby of Jupiter on July 5, 2022, its JunoCam instrument captured this striking view of vortices – hurricane-like spiral wind patterns – near the planet's north pole. These powerful storms can be over 30 miles (50 kilometers) in height and hundreds of miles across. Figuring out how they form is key to understanding Jupiter's atmosphere, as well as the fluid dynamics and cloud chemistry that create the planet's other atmospheric features. Scientists are particularly interested in the vortices' varying shapes, sizes, and colors. For example, cyclones, which spin counter-clockwise in the northern hemisphere and clockwise in the southern, and anti-cyclones, which rotate clockwise in the northern hemisphere and counter-clockwise in the southern hemisphere, exhibit very different colors and shapes. A NASA citizen science project, Jovian Vortex Hunter, seeks help from volunteer members of the public to spot and help categorize vortices and other atmospheric phenomena visible in JunoCam photos of Jupiter. This process does not require specialized training or software, and can be done by anyone, anywhere, with a cellphone or laptop. As of July 2022, 2,404 volunteers had made 376,725 classifications using the Jovian Vortex Hunter project web site at https://www.zooniverse.org/projects/ramanakumars/jovian-vortex-hunter. Another citizen scientist, Brian Swift, created this enhanced color and contrast view of vortices using raw JunoCam image data. At the time the raw image was taken, the Juno spacecraft was about 15,600 miles (25,100 kilometers) above Jupiter's cloud tops, at a latitude of about 84 degrees. https://photojournal.jpl.nasa.gov/catalog/PIA25017

Two frame "movie" of a pair of vortices in Jupiter's southern hemisphere. The two frames are separated by ten hours. The right oval is rotating counterclockwise, like other anticyclonic bright vortices in Jupiter's atmosphere. The left vortex is a cyclonic (clockwise) vortex. The differences between them (their brightness, their symmetry, and their behavior) are clues to how Jupiter's atmosphere works. The frames span about fifteen degrees in latitude and longitude and are centered at 141 degrees west longitude and 36 degrees south planetocentric latitude. Both vortices are about 3500 kilometers in diameter in the north-south direction. The images were taken in near infrared light at 756 nanometers and show clouds that are at a pressure level of about 1 bar in Jupiter's atmosphere. North is at the top. The smallest resolved features are tens of kilometers in size. These images were taken on May 7, 1997, at a range of 1.5 million kilometers by the Solid State Imaging system on NASA's Galileo spacecraft. An animation is available at http://photojournal.jpl.nasa.gov/catalog/PIA01230

ISS041-E-016962 (18 Sept. 2014) --- Although land and waters of Mexico's Pacific area pictured here are influenced by masses of clouds, for Baja California and other parts of Mexico in this photograph made from the International Space Station, things are quite calmer than a few days ago when Hurricane Odile unleashed its power on the peninsula, especially Baja's south end (right side of frame) and Cabo San Lucas (just out of frame right). The Sea of Cortez (Gulf of California) experiences rather calm weather in this view. California's Salton Sea is visible at left center; and Guadalupe Island is visible at lower left, surrounded by von Karman vortices.

NASA's Juno spacecraft observed the complex colors and structure of Jupiter's clouds as it completed its 43rd close flyby of the giant planet on July 5, 2022. Citizen scientist Björn Jónsson created these two images using raw data from the JunoCam instrument aboard the spacecraft. At the time the raw image was taken, Juno was about 3,300 miles (5,300 kilometers) above Jupiter's cloud tops, at a latitude of about 50 degrees. North is up. At that moment, the spacecraft was traveling at about 130,000 mph (209,000 kilometers per hour) relative to the planet. The image was digitally processed to increase both the color saturation and contrast to sharpen small-scale features and to reduce compression artifacts and noise that typically appear in raw images. This clearly reveals some of the most intriguing aspects of Jupiter's atmosphere, including color variation that results from differing chemical composition, the three-dimensional nature of Jupiter's swirling vortices, and the small, bright "pop-up" clouds that form in the higher parts of the atmosphere. https://photojournal.jpl.nasa.gov/catalog/PIA25018

Theodore von Kármán, a Hungarian-American physicist, was the first to describe the physical processes that create long chains of spiral eddies like the one shown above. Known as von Kármán vortices the patterns can form nearly anywhere that fluid flow is disturbed by an object. Since the atmosphere behaves like a fluid, the wing of an airplane, a bridge, even an island can trigger the distinctive phenomenon. On May 22, 2013, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Terra satellite captured this natural-color image of cloud vortices behind Isla Socorro, a volcanic island located in the Pacific Ocean. The island, which is located a few hundred kilometers off the west coast of Mexico and the southern tip of Baja California, is part of the Revillagigedo Archipelago. Satellite sensors have spotted von Kármán vortices around the globe, including off of Guadalupe Island, near the coast of Chile, in the Greenland Sea, in the Arctic, and even next to a tropical storm. NASA image courtesy Jeff Schmaltz, LANCE/EOSDIS MODIS Rapid Response Team at NASA GSFC. Caption by Adam Voiland. Instrument: Terra - MODIS More info: <a href="http://1.usa.gov/14VSDQa" rel="nofollow">1.usa.gov/14VSDQa</a> Credit: <b><a href="http://www.earthobservatory.nasa.gov/" rel="nofollow"> NASA Earth Observatory</a></b> <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASA_GoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>

A swirling storm somersaults through Jupiter's South Equatorial Belt in this view taken by NASA's Juno spacecraft. This feature -- not to be confused with the planet's iconic Great Red Spot -- is escorted by several smaller, reddish vortices above and to the left. This natural color view offers an approximation of what Jupiter would look like to human eyes from Juno's vantage point near the time of closest approach in its orbit. Jupiter's stunning appearance is due to its atmosphere of colorful cloud bands and spots. The vivid red and orange hues are created by chemicals of uncertain composition called "chromophores." The image was taken at 10:28 p.m. PDT on July 15, 2018 (1:28 a.m. EDT on July 16), as the spacecraft performed its 14th close flyby of Jupiter. At the time, Juno was about 4,900 miles (8,000 kilometers) from the planet's cloud tops, above a southern latitude of 36 degrees. Citizen scientist Björn Jónsson created this image using data from the spacecraft's JunoCam imager. https://photojournal.jpl.nasa.gov/catalog/PIA22427. - Enhanced image by Björn Jónsson (CC-NC-SA) based on images provided courtesy of NASA/JPL-Caltech/SwRI/MSSS

NASA's Juno spacecraft captured this detailed look at Jupiter's most recognizable feature, the Great Red Spot. Data from Juno's instruments indicate this giant, long-lived vortex extends far deeper into Jupiter's atmosphere than scientists previously expected, to about 300 miles (500 kilometers) below the cloud tops. The surprising discovery demonstrates that the Great Red Spot and other vortices descend below the depth where sunlight warms the atmosphere, providing new clues about the inner workings of the planet's beautiful but violent atmosphere. Researchers published the findings in the journal Science in Oct. 2021: https://www.nasa.gov/press-release/nasa-s-juno-science-results-offer-first-3d-view-of-jupiter-atmosphere Citizen scientist Andrea Luck processed this image from raw JunoCam data. The original image was taken on July 10, 2017, at 07:10 p.m. PDT (10:10 p.m. EDT), as the Juno spacecraft performed its seventh close flyby of Jupiter. At the time, the spacecraft was about 8,600 miles (13,840 kilometers) from the cloud tops, above latitude 33 degrees south. https://photojournal.jpl.nasa.gov/catalog/PIA25011

Saturn's clouds are full of raw beauty, but they also represent a playground for a branch of physics called fluid dynamics, which seeks to understand the motion of gases and liquids. Saturn's lack of a solid planetary surface (as on Earth, Mars or Venus) means that its atmosphere is free to flow around the planet essentially without obstruction. This is one factor that generates Saturn's pattern of alternating belts and zones -- one of the main features of its dynamic atmosphere. Winds in the belts blow at speeds different from those in the adjacent zones, leading to the formation of vortices along the boundaries between the two. And vigorous convection occasionally leads to storms and waves. Saturn's innermost rings are just visible at the bottom and in the upper left corner. This view is centered on clouds at 25 degrees north latitude on Saturn. The image was taken with the Cassini spacecraft wide-angle camera on July 20, 2016 using a spectral filter which preferentially admits wavelengths of near-infrared light centered at 728 nanometers. The view was obtained at a distance of approximately 752,000 miles (1.21 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 6 degrees. Image scale is 45 miles (72 kilometers) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA20503

Oval cloud systems of this type are often associated with chaotic cyclonic systems such as the balloon-shaped vortex seen here between the well-formed ovals. This system is centered near 30 degrees south latitude relative to the center of the planet and 100 degrees west longitude, and rotates in a clockwise direction about its center. The oval shaped vortices in the upper half of the mosaic are two of the three long-lived white ovals that formed to the south of the Great Red Spot in the 1930's and, like the Great Red Spot, rotate in a counterclockwise sense. The east-to-west dimension of the left-most white oval is 9,000 kilometers (5,592 miles) across. For comparison, the diameter of Earth is 12,756 kilometers, or 7,928 miles. The white ovals drift in longitude relative to one another and are presently restricting the cyclonic structure. To the south, the smaller oval and its accompanying cyclonic system are moving eastward at about 0.4 degrees per day relative to the larger ovals. The interaction between these two cyclonic storm systems is producing high, thick cumulus-like clouds in the southern part of the more northerly trapped system. The top mosaic combines the violet (410 nanometers) and near infrared continuum (756 nanometers) filter images to create a mosaic similar to how Jupiter would appear to human eyes. Differences in coloration are due to the composition and abundance of trace chemicals in Jupiter's atmosphere. The lower mosaic uses the Galileo imaging camera's three near-infrared wavelengths (756 nanometers, 727 nanometers, and 889 nanometers displayed in red, green, and blue) to show variations in cloud height and thickness. Light blue clouds are high and thin, reddish clouds are deep, and white clouds are high and thick. The clouds and haze over the white ovals are high, extending into Jupiter's stratosphere. There is a lack of high haze over the cyclonic feature. Dark purple most likely represents a high haze overlying a clear deep atmosphere. Galileo is the first spacecraft to distinguish cloud layers on Jupiter. North is at the top of these mosaics. The smallest resolved features are tens of kilometers in size. These images were taken on February 19, 1997, at a range of 1.1 million kilometers (683,507 miles) by the solid state imaging (CCD) system aboard NASA's Galileo spacecraft. http://photojournal.jpl.nasa.gov/catalog/PIA00700

This image captures the intensity of the jets and vortices in Jupiter's North North Temperate Belt. NASA's Juno spacecraft took this color-enhanced image at 10:31 p.m. PDT on May 23, 2018 (1:31 a.m. EDT on May 24), as Juno performed its 13th close flyby of Jupiter. At the time, the spacecraft was about 4,900 miles (7,900 kilometers) from the tops of the clouds of the gas giant planet at a northern latitude of about 41 degrees. The view is oriented with south on Jupiter toward upper left and north toward lower right. The North North Temperate Belt is the prominent reddish-orange band left of center. It rotates in the same direction as the planet and is predominantly cyclonic, which in the northern hemisphere means its features spin in a counter-clockwise direction. Within the belt are two gray-colored anticyclones. To the left of the belt is a brighter band (the North North Temperate Zone) with high clouds whose vertical relief is accentuated by the low angle of sunlight near the terminator. These clouds are likely made of ammonia-ice crystals, or possibly a combination of ammonia ice and water. Although the region as a whole appears chaotic, there is an alternating pattern of rotating, lighter-colored features on the zone's north and south sides. Scientists think the large-scale dark regions are places where the clouds are deeper, based on infrared observations made at the same time by Juno's JIRAM experiment and Earth-based supporting observations. Those observations show warmer, and thus deeper, thermal emission from these regions. To the right of the bright zone, and farther north on the planet, Jupiter's striking banded structure becomes less evident and a region of individual cyclones can be seen, interspersed with smaller, darker anticyclones. https://photojournal.jpl.nasa.gov/catalog/PIA22423 . - Enhanced image by Kevin M. Gill (CC-BY) based on images provided courtesy of NASA/JPL-Caltech/SwRI/MSSS

The easternmost edge of Jupiter's Great Red Spot and surrounding south tropical disturbance are captured in this image from NASA's Juno spacecraft. At left, wispy tendrils from the Red Spot give the atmosphere a layered appearance as they partially obscure cloud features below. Jupiter's appearance is a tapestry of vivid colors and swirling atmospheric vortices. Many aspects of the planet's atmosphere are still a mystery. For example, the origin of individual storms or churning cloud features is unknown. By studying Jupiter's weather up close for the first time, Juno is helping researchers better understand how atmospheres work in general -- including our own. What we learn about Jupiter's atmosphere will also help scientists understand how gas-giant planets work in general, including those now being discovered beyond our solar system. This color-enhanced image was taken at 3:01 a.m. PDT on April 1, 2018 (6:01 a.m. EDT), as the spacecraft performed its 12th close flyby of Jupiter. At the time, Juno was about 7,900 miles (12,750 kilometers) from the planet's cloud tops, above a southern latitude of approximately 26 degrees. Citizen scientist Kevin M. Gill created this image using data from the spacecraft's JunoCam imager. https://photojournal.jpl.nasa.gov/catalog/PIA22429 . - Enhanced image by Kevin M. Gill (CC-BY) based on images provided courtesy of NASA/JPL-Caltech/SwRI/MSSS

On Nov. 29, 2021, NASA's Juno mission completed its 38th close flyby of Jupiter. As the spacecraft sped low over the giant planet's cloud tops, its JunoCam instrument captured this look at two of Jupiter's largest moons. In the foreground, hurricane-like spiral wind patterns called vortices can be seen spinning in the planet's north polar region. These powerful storms can be over 30 miles (50 kilometers) in height and hundreds of miles across. Below Jupiter's curving horizon, two Jovian moons make an appearance: Callisto (below) and Io (above). Juno will make close flybys of Io in December 2023 and February 2024, the first such close encounters with this intriguing moon in over two decades. Io is the most volcanic body in our solar system, and its eruptions leave a trail of material behind that both fills Jupiter's magnetosphere and creates a torus of gas and dust around Jupiter. During the flybys, Juno will study Io's volcanoes and geology, search for signs of a magma ocean, and investigate how Io interacts with Jupiter's giant magnetosphere. Citizen scientist Gerald Eichstädt used raw JunoCam data to make the original version of this image, and then another citizen scientist, Thomas Thomopoulos, further processed it, zooming in and making color enhancements. In this view, north is down. At the time the image was taken, Juno was about 8,700 miles (14,000 kilometers) above Jupiter's cloud tops, at a latitude of about 69 degrees, traveling at a speed of about 123,000 mph (198,000 kilometers per hour) relative to the planet. https://photojournal.jpl.nasa.gov/catalog/PIA25019

The Boeing KC-135 Stratotanker, besides being used extensively in its primary role as an inflight aircraft refueler, has assisted in several projects at the NASA Dryden Flight Research Center, Edwards, California. In 1957 and 1958, Dryden was asked by what was then the Civil Aeronautics Administration (later absorbed into the Federal Aviation Administration (FAA) in 1958) to help establish new approach procedure guidelines on cloud-ceiling and visibility minimums for Boeing's first jet airliner, the B-707. Dryden used a KC-135 (the military variant of the 707), seen here on the runway at Edwards Air Force Base, to aid the CAA in these tests. In 1979 and 1980, Dryden was again involved with general aviation research with the KC-135. This time, a special wingtip "winglet", developed by Richard Whitcomb of Langley Research Center, was tested on the jet aircraft. Winglets are small, nearly vertical fins installed on an airplane's wing tips to help produce a forward thrust in the vortices that typically swirl off the end of the wing, thereby reducing drag. This winglet idea was tested at the Dryden Flight Research Center on a KC-135A tanker loaned to NASA by the Air Force. The research showed that the winglets could increase an aircraft's range by as much as 7 percent at cruise speeds. The first application of NASA's winglet technology in industry was in general aviation business jets, but winglets are now being incorporated into most new commercial and military transport jets, including the Gulfstream III and IV business jets, the Boeing 747-400 and MD-11 airliners, and the C-17 military transport. In the 1980's, a KC-135 was used in support of the Space Shuttle program. Since the Shuttle was to be launched from Florida, researchers wanted to test the effect of rain on the sensitive thermal tiles. Tiles were mounted on special fixtures on an F-104 aircraft and a P-3 Orion. The F-104 was flown in actual rain conditions, and also behind the KC-135 spray tanker as it rel

Hubble Catches Jupiter's Largest Moon Going to the 'Dark Side' HST/WFPC2 Image of Jupiter and Ganymede Taken April 9, 2007 NASA's Hubble Space Telescope has caught Jupiter's moon Ganymede playing a game of &quot;peek-a-boo.&quot; In this crisp Hubble image, Ganymede is shown just before it ducks behind the giant planet. Ganymede completes an orbit around Jupiter every seven days. Because Ganymede's orbit is tilted nearly edge-on to Earth, it routinely can be seen passing in front of and disappearing behind its giant host, only to reemerge later. Composed of rock and ice, Ganymede is the largest moon in our solar system. It is even larger than the planet Mercury. But Ganymede looks like a dirty snowball next to Jupiter, the largest planet in our solar system. Jupiter is so big that only part of its Southern Hemisphere can be seen in this image. Hubble's view is so sharp that astronomers can see features on Ganymede's surface, most notably the white impact crater, Tros, and its system of rays, bright streaks of material blasted from the crater. Tros and its ray system are roughly the width of Arizona. The image also shows Jupiter's Great Red Spot, the large eye-shaped feature at upper left. A storm the size of two Earths, the Great Red Spot has been raging for more than 300 years. Hubble's sharp view of the gas giant planet also reveals the texture of the clouds in the Jovian atmosphere as well as various other storms and vortices. Astronomers use these images to study Jupiter's upper atmosphere. As Ganymede passes behind the giant planet, it reflects sunlight, which then passes through Jupiter's atmosphere. Imprinted on that light is information about the gas giant's atmosphere, which yields clues about the properties of Jupiter's high-altitude haze above the cloud tops. This color image was made from three images taken on April 9, 2007, with the Wide Field Planetary Camera 2 in red, green, and blue filters. The image shows Jupiter and Ganymede in close to natural colors. For additional information go to: <a href="http://hubblesite.org/newscenter/archive/releases/2008/42/" rel="nofollow">hubblesite.org/newscenter/archive/releases/2008/42/</a> Credit: NASA, ESA, and E. Karkoschka (University of Arizona) <b><a href="http://www.nasa.gov/audience/formedia/features/MP_Photo_Guidelines.html" rel="nofollow">NASA image use policy.</a></b> <b><a href="http://www.nasa.gov/centers/goddard/home/index.html" rel="nofollow">NASA Goddard Space Flight Center</a></b> enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. <b>Follow us on <a href="http://twitter.com/NASAGoddardPix" rel="nofollow">Twitter</a></b> <b>Like us on <a href="http://www.facebook.com/pages/Greenbelt-MD/NASA-Goddard/395013845897?ref=tsd" rel="nofollow">Facebook</a></b> <b>Find us on <a href="http://instagram.com/nasagoddard?vm=grid" rel="nofollow">Instagram</a></b>