Researchers using NASA’s Juno study have so far developed a comprehensive 3-D understanding of the planet’s atmosphere from beneath Jupiter’s clouds, and the research was recently published in a series of scientific and geophysical research journals: Planets.
Juno, which has been orbiting Jupiter since 2016, is the most popular for beautiful images of the planet captured by its Juno Game camera, according to technology digital trends.
But much of this recent research has been done with Juno’s other instrument: the microwave radiometer (MWR), which can scan clouds around the planet and look deeper into its atmosphere.
“Previously, Juno surprised us with signs that events in Jupiter’s atmosphere had gone deeper than expected,” said Scott Bolton, Juno’s lead researcher at the Southwest Research Institute in San Antonio and editor – in – chief of a new research paper.
“Now, we’re starting to put all of these unique pieces together and gain the first real understanding of how Jupiter’s beautiful, violent atmosphere works – in 3D.” Epic to a depth of 60 miles in the atmosphere.
Jupiter’s most famous storm – the impressive Great Red Spot – stretched over 200 miles, and researchers were able to detect changes in its speed using instruments that study the planet’s gravity.
“Completing the MWR discovery in depth will give us great confidence that future gravity tests on Jupiter will be able to perform future gravity tests on Jupiter,” said Marcia Paresi, a Juno scientist at NASA’s Jet Propulsion Laboratory. Author of an article on the gravitational pull of science in Southern California and the Great Red Spot. That would lead to equally interesting results. ”The other leaves cover the atmospheric belts, giving the planet its unique look, and strange geometric storms at its poles.
“These new observations of Juno open up a treasure trove of new information about the obscure features of Jupiter,” said Larry Glees, director of NASA’s planetary science division at the agency’s headquarters in Washington. Each paper highlights different aspects of the planet’s atmospheric processes. It’s a great example of how our diverse scientific teams can improve our understanding of our solar system. “
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