The images were captured by Cassini's wide-angle camera between 2012 and 2016. Photos from 2012 show a bluish halo over Saturn's north pole, while those taken in 2016 show the same area with a more golden hue.
Saturn's north pole has a unique, six-sided jet stream known as "the hexagon," which is approximately 20,000 miles (32,000 kilometers) wide. Winds of this hexagonal vortex whip through the planet's atmosphere at approximately 200 mph (322 km/h).
Preliminary hypotheses suggest the color change observed in the atmosphere over Saturn's northern hemisphere could be associated with the jet stream. For instance, the hexagonal vortex may act as barrier and prevent surrounding particles from entering the area. In this case, the sky over Saturn's north pole would have been cleared of haze or aerosols during the seven-year-long Saturnian winter, according to a statement from NASA. Then, haze production would have ramped up again when the pole was exposed to sunlight.
"Scientists are investigating potential causes for the change in color of the region inside the north-polar hexagon on Saturn," NASA officials said in the statement. "The color change is thought to be an effect of Saturn's seasons. In particular, the change from a bluish color to a more golden hue may be due to the increased production of photochemical hazes in the atmosphere as the north pole approaches summer solstice in May 2017."
The observed color change in Saturn's north polar region between 2012 and 2016. |
Read more at Discovery News
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