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Saturns hexagon has remained visible to any probe thats visited planet, including Voyager, Hubble, and Cassini, though its structure is something of a mystery. In 2016, astronomers noticed that the hexagon had changed in hue, from blue to gold. New observations continue to show that theres a lot that scientists dont know about Saturn and its hexagon. Were seeing that it goes straight up into the stratosphere a long, long way. Thats unexpected, Glenn Orton, one of the studys authors and a physicist at NASAs Jet Propulsion Laboratory, told Gizmodo. Im s [url=https://www.cup-stanley.co.uk]stanley cup[/url] upposed to be wise about the dynamics, but Im at a loss as to how it could maintain itself that high. The scientists set out to study the North Polar Stratospheric Vortex NPSV . This is a swirling feature that forms during Saturns spring and summer in the stratosphere, the layer above the cloud tops, and disappears during the winter. The NPSV brings warmer temperatures and the increased presence of hydrocarbons, molecules made from hydrogen and carbon lik [url=https://www.cup-stanley.at]stanley thermobecher[/url] e methane. But Cassinis Composite Infrared Spectrometer demonstrated a significant surprise, according to the paper published this week in Nature Communications. The NPSV had a hexagon-shaped boundary that looked exactly like the well-known persisting hexagon in the lowest level of Saturns at [url=https://www.stanley-cup.cz]stanley cup[/url] mosphere. Somehow, during Saturns equivalent of spring and summer, the process that creates its hexagon appears to influence the molecules far above its cloud tops and causes the h