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A Jovian Hotspot in True and False Colors Time set 3
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Jovian Lightning and Moonlit Clouds
Ver en NASA ↗Jovian Lightning and the Daytime Storm
Ver en NASA ↗Water Cloud Thunderstorm Northwest of Great Red Spot
Ver en NASA ↗This view from NASA Voyager 1 in 1979 is of the region just to the east of the Red Spot, seen in greatly exaggerated color.
Ver en NASA ↗PPR Great Red Spot Temperature Map
Ver en NASA ↗These mosaics 6 frames each show the appearance of the Great Red Spot in infrared light obtained on June 26, 1996 by the Solid State Imaging system on board NASA Galileo spacecraft.
Ver en NASA ↗A Jovian Hotspot in True and False Colors Time set 1
Ver en NASA ↗A high resolution image of the Jovian mid-latitudes taken by NASA Voyager 1 spacecraft on March 2, 1979, shows distinctly differing characteristics of the planet meteorology.
Ver en NASA ↗This model of Earth's interior includes a solid, mostly iron inner core beneath a convective liquid iron core that extends to half Earth's radius.
Ver en NASA ↗Photopolarimeter/Radiometer PPR Temperature Map of Great Red Spot
Ver en NASA ↗This color view of the region just to the East of the Great Red Spot was taken by NASA Voyager 1 on March 4, 1979 at a distance of 1,000,000 miles 1,800,000 km.
Ver en NASA ↗This image, bottom panel, from NASA Galileo orbiter indicates the forces powering Jovian winds, and differentiates between areas of strongest upwelling and downwelling winds in the upper part of the atmosphere where winds are strong.
Ver en NASA ↗GMT340_00_10_Terry Virts_venus sunset jupiter sunrise_131
Ver en NASA ↗Voyager 1 views of Jupiter's rings
Ver en NASA ↗GMT340_00_10_Terry Virts_venus sunset jupiter sunrise_131
Ver en NASA ↗GMT340_00_10_Terry Virts_venus sunset jupiter sunrise_131
Ver en NASA ↗The Culann Patera volcano on Jupiter moon Io was observed by the near-infrared mapping spectrometer instrument onboard NASA Galileo spacecraft during its Io flyby on Nov. 25, 1999.
Ver en NASA ↗This illustration shows three possible scenarios for the evolution of asteroid belts. At the top, a Jupiter-size planet migrates through the asteroid belt, scattering material and inhibiting the formation of life on planets.
Ver en NASA ↗Hot eruption sites scattered across Jupiter moon Io stand out dramatically in an infrared image taken Oct. 13, 2001, by NASA Galileo spacecraft as it sped past this most volcanically active of all known worlds.
Ver en NASA ↗This view of Jupiter moon Europa features several regional-resolution mosaics overlaid on a lower resolution global view for context. The regional views were obtained during several different flybys of the moon by NASA Galileo mission.
Ver en NASA ↗Changes in the volcanoes on Jupiter moon Io can be seen in these three views, taken by NASA Galileo spacecraft during its three flybys of Io in October 1999, November 1999 and February 2000.
Ver en NASA ↗This image of Jupiter moon Io and its surrounding sky is shown in false color. This image was taken on Nov. 9, 1996 through the green-yellow filter of the solid state imaging CCD system aboard NASA Galileo spacecraft.
Ver en NASA ↗This diagram illustrates how astronomers using NASA Spitzer Space Telescope can capture the elusive spectra of hot-Jupiter planets. Spectra are an object light spread apart into its basic components, or wavelengths.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.