Something supercharged Uranus with radiation during Voyager flyby 40 years ago. Scientists now know what.
Scientists may have solved a long-standing mystery surrounding Uranus' extraordinarily strong radiation belt.
A new analysis of Voyager 2 data suggests that a temporary space weather event may have made the planet's electron radiation belt more intense than usual as Voyager 2 was passing by. The findings could help to explain why the radiation belt was so much stronger than scientists had predicted it would be.
Radiation belts are formed from interactions between the solar wind and a planet's magnetic field. The sun emits a continuous stream of protons and electrons from its outer atmosphere, called the corona. For planets that have a global magnetic field, including Earth and Uranus, some of those energetic, charged particles get trapped in the magnetosphere.
In January 1986, Voyager 2 flew by Uranus and measured the strength of its radiation belts. While the ion radiation belt was a little weaker than expected, the electron radiation belt was much more intense than scientists had predicted — close to the maximum intensity Uranus could sustain. Since then, scientists have tried to figure out how and why this was the case.
"Science has come a long way since the Voyager 2 flyby," Robert Allen, a space physicist at the Southwest Research Institute (SwRI) and coauthor of the new research, said in a statement. "We decided to take a comparative approach looking at the Voyager 2 data and compare it to Earth observations we've made in the decades since."
Earth versus Uranus
In the study, published in November 2025 in the journal Geophysical Research Letters, Allen and colleagues revisited data collected by Voyager 2 during its flyby of Uranus. They found several similarities between the Voyager data and the data collected from Earth orbit during a space weather event in 2019.
Uranus' unusually intense radiation belt may have been caused by a "co-rotating interaction region," the team found. A co-rotating interaction region occurs when high-speed solar winds overtake slower solar wind streams. The phenomenon could have accelerated electrons and added energy to the radiation belt, the researchers said.



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