CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Saturn's Active North Pole

Saturn's Active North Pole
PIA 09188

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  A bizarre six-sided feature encircling the north pole of Saturn near 78 degrees north latitude has been spied by the visual and infrared mapping spectrometer on NASA's Cassini spacecraft. This image is one of the first clear images ever taken of the north polar region as seen from a unique polar perspective.

Originally discovered and last observed by a spacecraft during NASA's Voyager flybys of the early 1980's, the new views of this polar hexagon taken in late 2006 prove that this is an unusually long-lived feature on Saturn.

This image is the first to capture the entire feature and north polar region in one shot, and is also the first polar view using Saturn's thermal glow at 5 microns (seven times the wavelength visible to the human eye) as the light source. This allows the pole to be revealed during the nighttime conditions presently underway during north polar winter. Previous images from Voyager and from ground-based telescopes suffered from poor viewing perspectives, which placed the feature and the north pole at the extreme northern limb (edge) of the planet.

To see the deep atmosphere at night, the infrared instrument images the thermal glow radiating from Saturn's depths. Clouds at depths about 75 kilometers (47 miles) lower than the clouds seen at visible wavelengths block this light, appearing dark in silhouette. To show clouds as features that are bright or white rather than dark, the original image has been contrast reversed to produce the image shown here. The nested set of alternating white and dark hexagons indicates that the hexagonal complex extends deep into the atmosphere, at least down to the 3-Earth-atmosphere pressure level, some 75 kilometers (47 miles) underneath the clouds seen by Voyager. Multiple images acquired over a 12-day period between Oct. 30 and Nov. 11, 2006, show that the feature is nearly stationary, and likely is an unusually strong pole-encircling planetary wave that extends deep into the atmosphere.

This image was acquired on Oct. 29, 2006, from an average distance of 902,000 kilometers (560,400 miles) above the cloud tops of Saturn.

For more information about the Cassini-Huygens mission visit The visual and infrared mapping spectrometer team homepage is at

Image Credit:
NASA/JPL/University of Arizona

Released: March 27, 2007 (PIA 09188)
Image/Caption Information

Alliance Member Comments
NeKto (Jun 19, 2008 at 5:10 PM):
as the seasons change on Saturn i would expect some changes in upper atmosphere flow paterns. on our tiny planet several factors can change the heat radiated to space, so i was wondering if there could be signifant weather changes on Saturn to measurably alter heat flow from lower to upper atmosphere. Are there any plans to do any comparison IR images as the northern hemisphere seasons change?