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South Polar Storms on Saturn

South Polar Storms on Saturn

14 November 2006

The instruments on board the Cassini spacecraft have observed an enormous storm raging in the atmosphere above Saturn's south pole. This type and scale of storm has never before been seen on another planet.

Images of the storm show it to be very similar in morphology to hurricanes on Earth, with a well-developed eye some 1500 km across, surrounded by a ~300 km wide ring of towering clouds. From the central ring, two spiral arms of clouds extend outwards and the entire storm measures ~8000 km across.

Instrument: ISS
Date: 11 October 2006
Distance: 340 000 km
Scale: ~17 km per pixel
Wavelength: 752 nm

Description: Wide-angle camera image of Saturn's south polar storm. The image has been contrast enhanced and re-projected to show the planet from a perspective directly over the south pole.

Credit: NASA/JPL/Space Science Institute

By analysing images of the storm taken with different Sun illumination angles, the height of the clouds relative to the central eye can be estimated. The clouds were found to tower 30-75 km above those in the centre, which is much higher than the ~15 km in similar storms on Earth.

The south polar area has been observed at different wavelengths in the visual and infrared by Cassini's Imaging Science Subsystem (ISS) and the Visual and Infrared Mapping Spectrometer (VIMS). In the below set of 6 images, the ISS images are in greyscale and the VIMS images in false-colour.

Instrument: ISS and VIMS
Date: 11 October 2006
Distance: 340 000 km
Scale: ISS: ~17 km per pixel, VIMS: ~174 km per pixel

Description: South polar storm imaged at 6 wavelengths (left to right, top to bottom): 460 nm, 752 nm, 728 nm, 890 nm, 2.8 μm, 5.0 μm.

Credit: NASA/JPL/Space Science Institute/University of Arizona

Over the eye, at the altitudes normally inhabited by bright ammonia clouds, there is a hole in the cloud layer and we can look deeper into Saturn's atmosphere. In the last two of the ISS images, this results in the eye to appear darker. At the concerned wavelengths (728 and 890 nm) methane gas absorbs light and only the highest clouds are visible, but these are absent over the eye of the storm

The absence of high clouds is also underlined by the brightness of the eye in the last image at 5.0 μm (with red colour scheme). At 5 μm, the lack of clouds at higher altitudes allows for the planet's thermal emission from below to escape, making the region appear brighter.

The dark spots in the two VIMS images are all smaller storms that are well developed and extend deep into the atmosphere, making them good absorbers of the thermal emission from the planet below. They therefore stand out in silhouette.

Polar Hot Spot

Observations by the Composite Infrared Spectrometer (CIRS) taken at the same time, but imaging higer altitudes, reveal a very small hot spot over the south pole coinciding with the eye of the storm.

Instrument: CIRS
Date: 11 October 2006
Distance: 340 000 km
Scale: ~17 km per pixel

Description: Temperature measurements, colour coded and plotted over an ISS wide-angle camera image of the south pole at 752 nm. The temperature ranges from 162 (black) to 165 Kelvin (red).
The hot spot is clearly visible.

Credit: NASA/JPL/Space Science Institute/GSFC

The measured temperature increase of ~2 Kelvin suggests that the atmosphere sinks over the south pole, with the increase in pressure causing the atmosphere to become compressed and heated up.

Seasonal Influences

The two VIMS images show the large number (hundreds) of smaller storms over the entire south polar region. This indicates the sheer extent of convective activity in the atmosphere there.

It is expected that the fact it is currently summer on Saturn's southern hemisphere plays a role. Follow-up observations over the next few years will help shed more light on the impact of the seasons on the convective activity at the south pole.

Last Update: 1 September 2019
23-Sep-2020 06:53 UT

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