Astronomers have gotten a first look at the aftermath of Saturn's 'Great Springtime Storm' thanks to the heat-seeking capabilities of the international Cassini spacecraft and two ground-based telescopes. Even though the cosmic event is hidden to the naked eye, a giant oval vortex continues to exist long after the visible effects of the storm have subsided. These spectacular observations were made possible thanks to the ground-based observations made by the Very Large Telescope of the European Southern Observatory in Chile, and NASA's Infrared Telescope Facility at the summit of Mauna Kea in Hawaii.
The vivid cloud structures made their first appearance in December 2010, and wreaked havoc across wide swathes of the mid-northern latitudes of Saturn's atmosphere well into much of 2011, capturing the the imaginations of amateur and professional astronomers alike. However, according to new reports focusing on the temperatures, winds and composition of Saturn's atmosphere, scientists are now discovering that the spectacular cloud displays were only part of the story. Much of the associated activity took place beyond the reach of visible-light cameras, and the after-effects are still continuing today.
'It's the first time we've seen anything like it on any planet in the Solar System,' says Leigh Fletcher from the University of Oxford, United Kingdom, lead author of the paper published in ICARUS. 'It's extremely unusual, as we can only see the vortex at infrared wavelengths — we can't tell that it is there simply by looking at the cloud cover.' A complementary paper by B. Hesman et al. has also been accepted for publication in the Astrophysical Journal.
As the visible storm erupted in the roiling cloud deck of Saturn's troposphere, waves of energy rippled hundreds of kilometres upwards, depositing their energy as two vast 'beacons' of hot air in the stratosphere. The beacons were expected to cool down and dissipate. However, by late April 2011, bright cloud material had encircled the entire planet and the hot spots had merged to create an enormous vortex that for a brief period exceeded even the size of Jupiter's famous Great Red Spot. Furthermore, the temperature of the vortex was far higher than expected, some 80 degrees Celsius warmer than the surrounding atmosphere. At the same time, huge spikes in the amount of gases like ethylene and acetylene were detected.
Saturn's vortex in some ways is similar to the Great Red Spot: it too cuts off the atmosphere in its core from the surrounding environment, constraining its unique chemistry and high temperatures within the walls of the powerful winds whipping around the edge.
'But Jupiter's vortex is embedded deep down in the turbulent "weather zone", whereas the vast vortex on Saturn is higher up in the atmosphere where, normally, you wouldn't expect anything like it to have formed,' says Dr Fletcher. 'Although there are parallels to be drawn between the two, the mechanisms by which they were formed and the length of time they are going to exist seem to be very different.'
Jupiter's famous vortex has raged for at least 300 years, but after traversing the planet once every 120 days since May 2011, Saturn's large beacon is cooling and shrinking. Scientists expect it to fade away completely by the end of 2013. The question now remains as to whether Saturn's storm-generating energy has been sapped or if there will be a repeat performance. The outburst already caught observers by surprise by arriving during the planet's northern hemisphere spring, years ahead of the predictably stormy summer season.
'The beauty is that Cassini will be operating until the Saturn system reaches its summer solstice in 2017, so if there is another global event like this, we'll be there to see it,' says ESA's Cassini project scientist Nicolas Altobelli.
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 mission for NASA’s Science Mission Directorate, Washington, DC.
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