Rob Chancia, a doctoral student at University of Idaho in the US, spotted key patterns in the rings while examining decades-old images of Uranus' icy rings taken by Voyager 2 which flew by the planet 30 years ago.
He noticed the amount of ring material on the edge of the alpha ring - one of the brightest of Uranus' multiple rings - varied periodically.
A similar, even more promising pattern occurred in the same part of the neighbouring beta ring.
Researchers analysed radio occultations - made when Voyager 2 sent radio waves through the rings to be detected back on Earth - and stellar occultations, made when the spacecraft measured the light of background stars shining through the rings, which helps show how much material they contain.
They found the pattern in Uranus' rings was similar to moon-related structures in Saturn's rings called moonlet wakes.
Uranian moons are especially hard to spot because their surfaces are covered in dark material.
"We haven't seen the moons yet, but the idea is the size of the moons needed to make these features is quite small, and they could have easily been missed," Hedman said.
"The Voyager images were not sensitive enough to easily see these moons," he said.
Hedman said their findings could help explain some characteristics of Uranus' rings, which are strangely narrow compared to Saturn's.
"The problem of keeping rings narrow has been around since the discovery of the Uranian ring system in 1977 and has been worked on by many dynamicists over the years," Chancia added.
The research was published in the Astronomical Journal.
Disclaimer: No Business Standard Journalist was involved in creation of this content
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