"Moons are always changing their orbits. That is inevitable. But that fact allows us to use computer simulations to tease out the history of Saturn's inner moons," said Matija Cuk from the Search for Extraterrestrial Intelligence (SETI) in the US.

Cuk, along with researchers from the Southwest Research Institute, used computer modelling to infer the past dynamic behaviour of Saturn's icy inner moons.

While our own moon has its orbit around Earth to itself, Saturn's many satellites have to share space with each other. All of their orbits slowly grow due to tidal effects, but at different rates, researchers said.

This results in pairs of moons occasionally entering so-called orbital resonances. These occur when one moon's orbital period is a simple fraction (for example, one-half or two-thirds) of another moon's period, they said.

In these special configurations, even small moons with weak gravity can strongly affect each other's orbits, making them more elongated and tilting them out of their original orbital plane, researchers said.

By comparing present orbital tilts and those predicted by computer simulations, researchers could learn how much the orbits of Saturn's moons grew. For some of the most important satellites - Tethys, Dione and Rhea - the orbits are less dramatically altered than previously thought, they said.

The relatively small orbital tilts indicate that they have not crossed many orbital resonances, meaning that they must have formed not far from where they are now.

To find out how long ago was their birth, researchers used results from NASA's Cassini mission to help answer this question. The Cassini spacecraft has observed ice geysers on Saturn's moon Enceladus.

According to the team's analysis, these would move the satellite by the small amount indicated by the simulations in only about 100 million years. The findings were published in the Astrophysical Journal.

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