CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Ultraviolet Movie of Jupiter's Polar Stratosphere

Unexpected dynamics in Jupiter's upper atmosphere, or stratosphere, including the birth and motion of a dark vortex wider than Earth, appear in a movie clip shown here spanning 11 weeks of ultraviolet imaging by the Cassini narrow-angle camera.

The development of the vortex resembles development of ozone holes in Earth's stratosphere in that both processes appear to occur only within confined masses of high-altitude polar air. That similarity may help scientists understand both processes better.

The movie is the first from any spacecraft to examine the planet's churning atmosphere in ultraviolet wavelengths. Hydrocarbons in Jupiter's stratosphere are transparent at the longer wavelengths of visible light and infrared light, but appear as haze in ultraviolet light.

Ultraviolet Movie of Jupiter's Polar Stratosphere
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  Cassini's narrow-angle camera took images from a near-equatorial perspective as the spacecraft approached Jupiter from Oct. 1, 2000, to Dec. 15, 2000. The images acquired over each 10 hour Jupiter rotation during this period were mosaicked together to form a cylindrical map (one of which is reproduced below) showing all 360 degrees of Jupiter's longitude. The top edge is at 60 degrees north latitude; the bottom at 60 degrees south latitude.

Haze in Jupiter's upper atmosphere, or stratosphere, scatters and reflects ultraviolet wavelengths, but is transparent in the visible-light portion of the spectrum. Hence, wave patterns at high latitudes, plus the famous Great Red Spot, dominate this ultraviolet map of Jupiter which is missing the low latitude horizontal stripes of dark and light bands of clouds that dominate the familiar visible-light views of Jupiter.

Ultraviolet Movie of Jupiter's Polar Stratosphere
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The maps were re-projected into a movie and displayed as if one were looking down at Jupiter's north pole and rotating with its magnetic field. Prograde (westerly) jets move in a counter-clockwise direction in this view. Contrast was enhanced to reveal faint features. The view extends south to the equator at the corners of the frame. The black area at the pole is where no presentable data were acquired due to Cassini's viewing angle. For reference, a circle of 60 degrees latitude is superimposed in white, and an oval where Jupiter has a persistent aurora is superimposed in blue. The aurora itself, comparable to Earth's Northern Lights, is not visible here.

Energetic auroras heat the stratosphere and stimulate the formation of complex hydrocarbons from the breakup of methane molecules. A dark patch appears and within two weeks becomes a well-defined oval about the same size and shape as Jupiter's southern hemisphere Great Red Spot. While this dark vortex is nestled inside the auroral oval, its outer edge begins to circulate in a clockwise direction as it simultaneously develops a small, brighter, inner core. It eventually moves out of the auroral region and deforms by flattening in latitude and growing in longitude. Near the end of the movie, a second, smaller, dark oval appears nearer to the pole and deforms in the wind shear.

A series of wave features rings the planet south of (outside of) the latitude-60 circle. These make visible some of the dynamics of how haze generated in the confined polar stratosphere mixes eventually into the winds farther south.

Comparison of this ultraviolet movie with a near-infrared movie that was produced the same way and released previously on July 16, 2001 reveals many differences. Instead of the waves and large vortex seen in the ultraviolet, the infrared imaging shows a multitude of small storms and parallel wind bands at a lower elevation in the atmosphere.

Cassini made its closest pass to Jupiter, about 10 million kilometers (6 million miles), on Dec. 30, 2000. It is now proceeding toward its ultimate destination, Saturn.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission, visit and the Cassini imaging team home page,

Credit: NASA/JPL/Cassini Imaging Team
Released: March 13, 2002
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