Researchers Find Winds on Uranus and Neptune Confined to Thin Atmosphere Layer
Researchers Find Winds on Uranus and Neptune Confined to Thin Atmosphere Layer
(Phys.org) —A team of researchers from the U.S. and Israel has deduced that the winds that blow on Uranus and Neptune are confined to relatively thin atmospheric layers.
In their paper published in the journal Nature, the group describes how they used data from Voyager 2, ground based satellites and models to work out the thickness of the weather systems on the two ice giants.
With the downgrading of Pluto, Neptune and Uranus are now listed as the planet’s in our solar system the most distant from the sun.
Because of that, the least is known about them.
To date, just one spacecraft has flown close enough to either of them to offer useful information: Voyager 2 back in the 1980′s.
Scientists would like to know more of course—of particular interest are the bands of winds that blow at high speeds in the atmospheres of both planets.
URANUS, EARTH AND NEPTUNE COMPARISON
Are they fueled by mostly atmospheric conditions or by an unknown inner planetary dynamic? No one knows for sure, but work done in this latest effort suggests it’s more likely the former.
To learn more about the weather systems going on with both planets, the research team dug up gravity data from the Voyager 2 missions, used current telescopes and created models to help identify the factors that contribute to the wind bands.
They focused specifically on each planets’ gravitational field, noting that variations can occur due to a variety of factors.
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