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“While we knew its motion varies slightly in its longitude, we didn’t expect to see the size oscillate as well. As far as we know, it’s not been identified before,” said lead study author Amy Simon, a planetary scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, in a statement.

“This is really the first time we’ve had the proper imaging cadence of the GRS,” Simon said. “With Hubble’s high resolution we can say that the GRS is definitively squeezing in and out at the same time as it moves faster and slower. That was very unexpected.”

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vaibhav global limited (532156) quarterly results are out ✌️【Career Goals】✌️ Free expert predictions on stock trends and real-time data to help you make informed decisions and grow your wealth steadily. The study, published September 27 in theJournal of Geophysical Research: Planets, revealed that the Great Red Spot is cold in the center, which causes ammonia and water to condense inside the vortex and create thick clouds. The research team also detected the gas phosphine within the storm, which could play “a role in generating those mysterious” red colors that make the Great Red Spot so iconic, said study coauthor Leigh Fletcher, a professor of planetary science at the UK’s University of Leicester, in a statement.

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vaibhav global limited (532156) quarterly results are out ✌️【Career Goals】✌️ Expert stock predictions and free stock selection services to help you achieve optimal returns and long-term growth. NASA scientists use Hubble’s sharp eye to track the storm’s behavior once a year through the Outer Planet Atmospheres Legacy, or OPAL, program, which Simon leads. Scientists use this program to observe the outer planets in our solar system and watch how they change over time.

But the new observations were taken separately through a program dedicated to studying the Great Red Spot in more detail by watching how the storm changed over a matter of months, rather than a singular, yearly snapshot.

“To the untrained eye, Jupiter’s striped clouds and famous red storm might appear to be static, stable, and long-lived over many years,” Fletcher said. “But closer inspection shows incredible variability, with chaotic weather patterns just as complex as anything we have here on Earth. Planetary scientists have been striving for years to see patterns in this variation, anything that might give us a handle on the physics underpinning this complex system.”

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“As it accelerates and decelerates, the GRS is pushing against the windy jet streams to the north and south of it,” said study coauthor Mike Wong, planetary scientist at the University of California, Berkeley, in a statement. “It’s similar to a sandwich where the slices of bread are forced to bulge out when there’s too much filling in the middle.”

On Neptune, dark spots can drift across the planet since no strong jet streams are holding them in place, Wong said, while the Great Red Spot is trapped between jet streams at a southern latitude on Jupiter.

vaibhav global limited (532156) quarterly results are out ✌️【Career Goals】✌️ Free real-time global stock trend updates to help you capture market movements and make better investment decisions. Astronomers have noticed the Great Red Spot shrinking since the OPAL program began a decade ago and predict that it will continue to shrink until it reaches a stable, less-elongated shape, which could reduce the wobble.

“Right now it’s over-fillingits latitude band relative to the wind field. Once it shrinks inside that band the winds will really be holding it in place,” Simon said.

vaibhav global limited (532156) quarterly results are out ✌️【Career Goals】✌️ Professional investment advice with real-time updates on stock indices and futures data. Stay ahead with expert predictions and market insights. The new Hubble study fills in more pieces of the puzzle about the Great Red Spot, Fletcher said. While scientists have known that the westward drift of the storm has an unexplained 90-day oscillation, the accelerating and decelerating pattern doesn’t seem to change although the storm is shrinking, he said.

“By watching the GRS over a few months, Hubble has shown that the anticyclone itself is changing its shape along with this oscillation,” Fletcher said. “The shape change is important, as it may be affecting how the edge of the vortex interacts with other passing storms. Besides the gorgeous Hubble imagery, this study shows the power of observing atmospheric systems over long periods of time. You need that sort of monitoring to spot these patterns, and it’s clear that the longer you watch, the more structure you see in the chaotic weather.”

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