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License = https://en.wikipedia.org/wiki/File:PIA22946-Jupiter-RedSpot-JunoSpacecraft-20190212.jpg
Title = This striking view of Jupiters Great Red Spot and turbulent southern hemisphere was captured by NASAs Juno spacecraft as it performed a close pass of the gas giant planet.
URL = https://upload.wikimedia.org/wikipedia/commons/7/71/PIA22946-Jupiter-RedSpot-JunoSpacecraft-20190212.jpg
02_CompareEarth/License = https://en.wikipedia.org/wiki/File:Jupiter,_Earth_size_comparison.jpg
02_CompareEarth/Title = Rough visual comparison of Jupiter, Earth, and the Great Red Spot.
02_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/c/c2/Jupiter,_Earth_size_comparison.jpg
03_Clouds/License = https://en.wikipedia.org/wiki/File:PIA21972_Jupiter_Blues.jpg
03_Clouds/Title = Jovian clouds in striking shades of blue in this new view taken by NASA's Juno spacecraft. The Juno spacecraft captured this image when the spacecraft was only 11,747 miles (18,906 kilometers) from the tops of Jupiter's clouds. The higher-altitude clouds can be seen casting shadows on their surroundings. The behavior is most easily observable in the whitest regions in the image, but also in a few isolated spots in both the bottom and right areas of the image.
03_Clouds/URL = https://upload.wikimedia.org/wikipedia/commons/5/5c/PIA21972_Jupiter_Blues.jpg
04_SouthernStorms/License = https://en.wikipedia.org/wiki/File:PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg
04_SouthernStorms/Title = This image shows Jupiter's south pole, as seen by NASA's Juno spacecraft from an altitude of 32,000 miles (52,000 kilometers). The oval features are cyclones, up to 600 miles (1,000 kilometers) in diameter.
04_SouthernStorms/URL = https://upload.wikimedia.org/wikipedia/commons/b/b0/PIA21641-Jupiter-SouthernStorms-JunoCam-20170525.jpg
05_TimelapseVoyager1/License = https://en.wikipedia.org/wiki/File:790106-0203_Voyager_58M_to_31M_reduced.gif
05_TimelapseVoyager1/Title = Jupiter seen by Voyager 1 probe with blue filter. One image was taken every Jupiter day (approximately 10 hours). These pictures were taken from 01/06 to 02/03, 1979 0x003B and Voyager 1 flew from 58 million to 31 million kilometers from Jupiter during that time. The small, round, dark spots appearing in some frames are the shadows cast by the moons passing between Jupiter and the Sun, while the small, white flashes around the planet, are the moons themselves.
05_TimelapseVoyager1/URL = https://upload.wikimedia.org/wikipedia/commons/a/a3/790106-0203_Voyager_58M_to_31M_reduced.gif
79_Moons_Orbiting/License = https://en.wikipedia.org/wiki/File:Jupiter_and_the_Galilean_moons_animation.gif
79_Moons_Orbiting/Title = Animation of a sequence of photographs taken by JunoCam aboard the Juno spacecraft, in June 2016, of Jupiter and the motion of the four Galilean moons, as the spacecraft approached the planet.
79_Moons_Orbiting/URL = https://upload.wikimedia.org/wikipedia/commons/6/66/Jupiter_and_the_Galilean_moons_animation.gif
80_Moons_Europa_1/License = https://en.wikipedia.org/wiki/File:Europa-moon-with-margins.jpg
80_Moons_Europa_1/Title = Europa is the smallest of the four Galilean moons orbiting Jupiter, and the sixth-closest to the planet of all the 79 known moons of Jupiter. It is also the sixth-largest moon in the Solar System. Europa was discovered in 1610 by Galileo Galilei and was named after Europa, the Phoenician mother of King Minos of Crete and lover of Zeus (the Greek equivalent of the Roman god Jupiter). Slightly smaller than Earth's Moon, Europa is primarily made of silicate rock and has a water-ice crust and probably an iron0x2013nickel core. It has a very thin atmosphere, composed primarily of oxygen. Its surface is striated by cracks and streaks, but craters are relatively few. 
80_Moons_Europa_1/URL = https://upload.wikimedia.org/wikipedia/commons/e/e4/Europa-moon-with-margins.jpg
80_Moons_Europa_2_CloseUp/License = https://en.wikipedia.org/wiki/File:Europa_PIA2387x_-_Chaos_Transition,_Crisscrossing_Bands_&_Chaos_Near_Agenor_Linea.jpg
80_Moons_Europa_2_CloseUp/Title = The surface of Jupiter's moon Europa features a widely varied landscape, including ridges, bands, small rounded domes and disrupted spaces that geologists called "chaos terrain."
80_Moons_Europa_2_CloseUp/URL = https://upload.wikimedia.org/wikipedia/commons/b/b3/Europa_PIA2387x_-_Chaos_Transition,_Crisscrossing_Bands_&_Chaos_Near_Agenor_Linea.jpg
80_Moons_Ganymede/License = https://en.wikipedia.org/wiki/File:Ganymede_g1_true-edit1.jpg
80_Moons_Ganymede/Title = Ganymede is the largest and most massive of the Solar System's moons. The ninth-largest object in the Solar System, it is the largest without a substantial atmosphere. It has a diameter of 5,268 km (3,273 mi), making it 26% larger than the planet Mercury by volume, although it is only 45% as massive.0x005B160x005D Possessing a metallic core, it has the lowest moment of inertia factor of any solid body in the Solar System and is the only moon known to have a magnetic field.
80_Moons_Ganymede/URL = https://upload.wikimedia.org/wikipedia/commons/f/f2/Ganymede_g1_true-edit1.jpg
80_Moons_Ganymede_2_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Ganymede,_Earth_&_Moon_size_comparison.jpg
80_Moons_Ganymede_2_CompareEarthMoon/Title = Diameter comparison of Ganymede, Moon, and Earth.
80_Moons_Ganymede_2_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/7/76/Ganymede,_Earth_&_Moon_size_comparison.jpg
80_Moons_Ganymede_3_CraterChain/License = https://en.wikipedia.org/wiki/File:Chain_of_impact_craters_on_Ganymede.jpg
80_Moons_Ganymede_3_CraterChain/Title = A chain of craters on Ganymede, probably caused by a similar impact event to Shoemaker-Levy crashing into Jupiter. The picture covers an area approximately 190 km (120 mi) across.
80_Moons_Ganymede_3_CraterChain/URL = https://upload.wikimedia.org/wikipedia/commons/d/dd/Chain_of_impact_craters_on_Ganymede.jpg
80_Moons_Io_1/License = https://en.wikipedia.org/wiki/File:Io_highest_resolution_true_color.jpg
80_Moons_Io_1/Title = Io is the innermost and third-largest of the four Galilean moons of the planet Jupiter. It is the fourth-largest moon in the Solar System, has the highest density of all of them, and has the lowest amount of water (by atomic ratio) of any known astronomical object in the Solar System. It was discovered in 1610 by Galileo Galilei and was named after the mythological character Io, a priestess of Hera who became one of Zeus's lovers. With over 400 active volcanoes, Io is the most geologically active object in the Solar System. This extreme geologic activity is the result of tidal heating from friction generated within Io's interior as it is pulled between Jupiter and the other Galilean moons0x2014Europa, Ganymede and Callisto.
80_Moons_Io_1/URL = https://upload.wikimedia.org/wikipedia/commons/7/7b/Io_highest_resolution_true_color.jpg
80_Moons_Io_2_CompareEarthMoon/License = https://en.wikipedia.org/wiki/File:Io,_Earth_&_Moon_size_comparison.jpg
80_Moons_Io_2_CompareEarthMoon/Title = Diameter comparison of Io, Moon, and Earth.
80_Moons_Io_2_CompareEarthMoon/URL = https://upload.wikimedia.org/wikipedia/commons/c/cc/Io,_Earth_&_Moon_size_comparison.jpg
80_Moons_Io_3_Vulcan/License = https://en.wikipedia.org/wiki/File:Tvastarpic2.jpg
80_Moons_Io_3_Vulcan/Title = The detection of very-high-temperature volcanism0x2014hotter than any terrestrial lavas currently erupting0x2014is one of the most spectacular discoveries by the Galileo mission at Io. The images are of an area called Tvashtar and show curtains of lava fountains erupting on the surface. They were taken by the Galileo spacecraft on November 26, 1999. The active region is approximately 25 km (15.5 miles) long and 1 km (0.6 mile) high. The radiant energy emitted from the lava curtain was so intense that it overpowered the camera's detector and it is registered only in white.
80_Moons_Io_3_Vulcan/URL = https://upload.wikimedia.org/wikipedia/commons/f/f0/Tvastarpic2.jpg
80_Moons_Io_4_VulcanAnimation/License = https://en.wikipedia.org/wiki/File:Tvashtarvideo.gif
80_Moons_Io_4_VulcanAnimation/Title = Five-image sequence of New Horizons images showing Io's volcano Tvashtar spewing material 330 km above its surface
80_Moons_Io_4_VulcanAnimation/URL = https://upload.wikimedia.org/wikipedia/commons/1/12/Tvashtarvideo.gif
90_Explore_40_Galileo/License = https://en.wikipedia.org/wiki/File:Galileo_Preparations_-_GPN-2000-000672.jpg
90_Explore_40_Galileo/Title = In the Vertical Processing Facility (VPF), Galileo is prepared for mating with the Inertial Upper Stage booster.
90_Explore_40_Galileo/URL = https://upload.wikimedia.org/wikipedia/commons/1/1d/Galileo_Preparations_-_GPN-2000-000672.jpg
90_Explore_50_Juno/License = https://en.wikipedia.org/wiki/File:Juno's_high-gain_antenna_just_before_installation.jpg
90_Explore_50_Juno/Title = Juno's high-gain antenna dish being installed
90_Explore_50_Juno/URL = https://upload.wikimedia.org/wikipedia/commons/c/c2/Juno's_high-gain_antenna_just_before_installation.jpg

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