Not exact matches
Juno found
cyclones as big as 870 miles (1,400 km) in diameter swirling
over Jupiter's north and south
poles, shows the research published in this week's issue of the journal Science.
The researchers also cite previous research showing that
over the past 30 years, the location where tropical
cyclones reach their maximum intensity has shifted away from the equator and toward the
poles.
Previous surveys by Cassini have found that winds whip through the atmosphere
over Saturn's north
pole at more than 500 kilometers per hour — 30 percent faster than any gust ever recorded in a
cyclone on Earth.
In a paper published today in the journal Nature Geoscience, atmospheric scientists at MIT propose a possible mechanism for Saturn's polar
cyclones:
Over time, small, short - lived thunderstorms across the planet may build up angular momentum, or spin, within the atmosphere — ultimately stirring up a massive and long - lasting vortex at the
poles.
«This mechanism means that little thunderstorms — fast, abundant, but not very strong thunderstorms —
over a long period of time can actually accumulate so much angular momentum right on the
pole, that you get a permanent, wildly strong
cyclone.»
Like a compact series of cogs in an unimaginably large machine, vast
cyclones also swirl around the north and south
poles, clocking wind speeds of
over 220 miles per hour (350 kilometers per hour)-- wind speeds that are the equivalent of a terrestrial Category 5 hurricane.
Here's another finding, courtesy of Juno: Unlike Saturn's enigmatic hexagonal (six - sided polygon) cloud structure
over the ringed gas giant's north
pole, Jupiter's northern
cyclones form an octagonal (eight - sided) grouping.
«Now, with Juno flying
over the
poles at a close distance it permits the collection of infrared imagery on Jupiter's polar weather patterns and its massive
cyclones in unprecedented spatial resolution.»