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accel limited (517494) signs major deal ✌️【Risk Avoidance】✌️ Free global stock market data to help you plan the best investment strategies and seize market opportunities. When theVoyager 2 spacecraftbecame the first and only mission to fly by Uranus in 1986, it defined the way astronomers understand the ice giant. But the data collected by the probe also introduced new mysteries that have continued to puzzle scientists in the decades since the historic flyby.
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“The spacecraft saw Uranus in conditions that only occur about 4% of the time,” said lead study author Jamie Jasinski, space plasma physicist at NASA’s Jet Propulsion Laboratory in Pasadena, California, in a statement.
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Voyager 2’s flyby of the sideways-rotating Uranus revealed previously unknown rings and moons around the planet.
But the spacecraft’s observations of Uranus’ magnetosphere were wildly different from astronomers’ expectations, and scientists deemed the planet an outlier among the other large planets in our solar system, such as Jupiter, Saturn and Neptune.
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Understanding how magnetospheres function around other planets not only aids scientists in planning exploratory missions, it also provides insight about how Earth’s magnetosphere operates.
Voyager 2’s data showed that Uranus’ magnetosphere was home to unexpectedly powerful electron radiation belts. Their intensity was similar to the massive bands of radiation found around Jupiter.
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However, there was no apparent source for energetic particles to drive and boost the intensity of the belts seen around Uranus because there appeared to be a lack of plasma, or ionized gas, which was strange because plasma is a common element in magnetospheres around other planets.
Voyager 2’s observations of Uranus’ magnetosphere defied the way astronomers understand how magnetic fields trap energetic particles and their radiation.
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But a new analysis of the Voyager 2 data showed that Uranus experienced a rare cosmic occurrence just before the flyby.
Days before the flyby, an intense solar wind event was released from the sun, stirring up space weather throughout the solar system. Solar wind hit Uranus and dramatically compressed its magnetosphere, likely pushing plasma out of it. But the solar wind also made Uranus’ magnetosphere more dynamic by feeding it with electrons, which boosted the planet’s radiation belts, according to the new study.
“If Voyager 2 had arrived just a few days earlier, it would have observed a completely different magnetosphere at Uranus,” Jasinski said.
It’s likely that Uranus’ magnetosphere would have looked similar to the magnetic bubbles around the other giant planets in our solar system without any anomalies, the study authors said.
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“We highlight that our understanding of the Uranus system is highly limited, and our analysis shows that any conclusions made from the Voyager 2 flyby are similarly tentative,” the authors wrote in their study. “We suggest that discoveries made by the Voyager 2 flyby should not be assigned any typicality regarding Uranus’s magnetosphere.”
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“The magnetosphere Voyager 2 measured was only a snapshot in time,” Spilker said in astatement. “This new work explains some of the apparent contradictions, and it will change our view of Uranus once again.”
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If astronomers’ knowledge of Uranus is based on a flyby conducted under rare circumstances, it suggests that there may be good reason to revisit the ice giant. The James Webb Space Telescope has already helped reveal new information about Uranus, including highlighting its typically hiddenrings, moons, weather and atmosphere.
Fortunately, sending a dedicated mission to study Uranus in the future has become a priority for NASA, according to a report released in2022.
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