Saturn-like worlds may abound throughout the universe, and NASA's planet-hunting Kepler spacecraft has the ability to find them, astronomers say.

Rings surround the gas giants in our solar system, but scientists have yet to find any on similar alien planets. The precise instruments on the Kepler spacecraft could change that.

"The ideal areas to try and look for rings are the regions Kepler is sensitive to," Hilke Schlichting, of the University of California, Los Angeles, explained.

Schlichting and Philip Chang of the Canadian Institute for Theoretical Astrophysics examined the types of rings that could form around large gas planets orbiting near their stars. [Photos: The Rings and Moons of Saturn]

Before Kepler scientists announced the spacecraft's discovery of over 1,200 potential alien worlds in February, gas giants with small orbits dominated Kepler's planetary findings.

Rocky rings

Such planets would likely be surrounded by rings made of rock rather than ice, the researchers said.

As with Saturn, the particles in these rings would range from micron size to tens of meters wide. Schlichting told they would resemble the bands around our own solar system's most notably ringed planet.

Of course, they might not appear exactly the same. Rings form around the equator of a planet, so if the planet is tilted in respect to Earth, the rings may be tipped on edge, or appear to surround the planet like a circular frame.

Some rings even may have a kink to them. That is, a portion of the ring near the planet would move out smoothly from the halo, then sharply bend. Such a warped ring might occur if the tilt of the planet changed over time, which could reveal details about the planet's interior.

But figuring out details like warps would come later, the researchers said.

"First we have to find the rings, then we can worry about signatures" in them, Schlichting said.

Searching for rings

Finding the rings alone could reveal details about how large gas giants – which Schlichting calls 'warm Saturns' but actually run the gamut from Neptune- to Jupiter-size – wound up so close to their suns.

According to current formation models, gas giants can form only far from the heat of their parent star. The question is whether they then migrate smoothly inward or scatter inward at random.

"If we could detect several of these systems, they could tell us how the bodies got there."

If rings formed with their planet, they would likely be icy. As they moved closer to the star, they would evaporate. If the planet moved in slowly, it would be more likely to pick up rocks in its rings than a rapidly moving, erratic body would.

Because the rings form around the equator, they can also reveal the orbital axis of a planet in relation to its parent star, or its obliquity. This also could help determine how these hot giants formed.