CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Strong Jet in False Colors
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A particularly strong jet stream churns through Saturn's northern hemisphere in this false-color view from NASA's Cassini spacecraft.

Clouds associated with the jet stream can be seen in the upper right about a third of the way down from the top of this image. The jet stream clouds appear like a thin, bright orange line here. Moving west and closer to the center of the image, the feature drops south. Farther to the west of this discontinuity, or drop, a blurrier form of the jet stream clouds continues to move along the latitude circle.

See PIA14917 for a closer view and to learn how eddies, or rotating storms, give the jet stream its shape and speed.

The winds of Saturn's jet streams are zonal, meaning they move eastward or westward at particular latitudes. This jet stream is located at about 42 degrees north latitude, and has been visible on Saturn since the days of the Voyager spacecraft (see PIA00027). In the Voyager days, this jet stream had an undulating appearance, leading scientists to dub it the "ribbon wave" (see PIA01378). The planet's atmosphere is always changing, and the jet stream now looks nothing like a ribbon.

Saturn's atmosphere and its rings are shown here in a false color composite made from three images taken in near infrared light through filters that are sensitive to varying degrees of methane absorption. Red and orange colors in this view indicate clouds that are deep in the atmosphere. Yellow and green colors, most noticeable near the top of the view, indicate intermediate clouds. White and blue indicate high clouds and haze.

The white clouds of the equatorial region appear oversaturated because the image was specially processed to bring out the wave.

The rings, in the upper left and lower left of the image, appear bright blue because they are outside of the atmosphere and not affected by methane absorption. This view looks toward the northern, unilluminated side of the rings from about 36 degrees above the ringplane.

The images were taken with the Cassini spacecraft wide-angle camera on Jan. 13, 2008 using a combination of spectral filters sensitive to wavelengths of near-infrared light. The image filtered at 890 nanometers is projected as blue. The image filtered at 728 nanometers is projected as green, and the image filtered at 752 nanometers is projected as red.

The view was acquired at a distance of approximately 810,000 miles (1.3 million kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 55 degrees. Image scale is 46 miles (74 kilometers) per pixel.

The Cassini Solstice Mission is a joint United States and European endeavor. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. 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 Solstice Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

Credit: NASA/JPL-Caltech/Space Science Institute
Released: June 25, 2012 (PIA 14916)
Image/Caption Information
  Strong Jet in False Colors
PIA 14916

Avg Rating: 9.09/10

Annotated Full Size 924x877:
JPEG 353 KB
PNG 1.1 MB
TIFF 1.5 MB

 

Strong Jet in False Colors
PIA 14916

Avg Rating: 7.89/10

Unannotated Full Size 924x877:
JPEG 353 KB
PNG 1.1 MB
TIFF 1.5 MB



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