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Atmospheric Motion in Jupiter's Northern Hemisphere

Jet Propulsion Laboratory https://www.jpl.nasa.gov/ Sept. 25, 2000
True-color (left) and false-color (right) mosaics of Jupiter's northern hemisphere between 10 and 50 degrees latitude. This image was taken by NASA's Galileo spacecraft on April 3, 1997 at a distance of 1.4 million kilometers.

True-color (left) and false-color (right) mosaics of Jupiter's northern hemisphere between 10 and 50 degrees latitude. Jupiter's atmospheric motions are controlled by alternating eastward and westward bands of air between Jupiter's equator and polar regions. The direction and speed of these bands influences the color and texture of the clouds seen in this mosaic. The high and thin clouds are represented by light blue, deep clouds are reddish, and high and thick clouds are white. A high haze overlying a clear, deep atmosphere is represented by dark purple. This image was taken by NASA's Galileo spacecraft on April 3, 1997 at a distance of 1.4 million kilometers (.86 million miles).

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Mission
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  • Jupiter
Spacecraft
  • Galileo Orbiter
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  • Solid-State Imaging
Credit
NASA/JPL/University of Arizona

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