Weird Interior of Saturn’s Moon Makes It Wobble

October 23, 2014 Updated: October 23, 2014

A slight wobble detected in Saturn’s moon Mimas suggests its icy surface is covering either an odd-shaped rocky core or a sloshing ocean.

Researchers used a technique called stereo-photogrammetry to interpret images taken by the Cassini Imaging Science Subsystem to measure the libration on the moon Mimas.

Astronomers took Cassini photographs of Mimas taken at different times and from various vantage points to build precise 3D computer models of the locations of hundreds of surface reference points.

From these, the researchers determined the moon’s shape and were able to notice that the satellite didn’t rotate smoothly but rocked back and forth a bit as well.

“After carefully examining Mimas, we found it librates—that is, it subtly wobbles—around the moon’s polar axis,” says Radwan Tajeddine, research associate in astronomy at Cornell University and lead author of the article published in Science.

“In physical terms, the back-and-forth wobble should produce about 3 kilometers of surface displacement. Instead we observed an unexpected 6 kilometers of surface displacement.

What’s Hiding Under the Ice?

“We’re very excited about this measurement because it may indicate much about the satellite’s insides. Nature is essentially allowing us to do the same thing that a child does when she shakes a wrapped gift in hopes of figuring out what’s hidden inside,” Tajeddine says.

The amount of the to-and-fro motion indicates that Mimas’ interior is not uniform. These wobbles can be produced if the moon contains a weirdly shaped rocky core or if a sub-surface ocean exists beneath its icy shell.

Mimas is about 400 kilometers in diameter, and its possible internal global ocean is located under an icy crust ranging in thickness between 25 and 30 kilometers (15.5 and 18.6 miles). The moon itself is thought to have been formed either by the slow agglomeration of ring particles (a gradual buildup of matter) or direct growth within the primordial planetary gas nebula.

The odd-shaped core would favor gravitational flattening by nearby Saturn, Tajeddine says. The moon’s relatively smooth and roughly spherical icy surface covers up whatever is underneath.

The Université Pierre et Marie Curie, the Cassini mission (NASA), and the European Space Agency in collaboration with the Belgian Federal Science Policy Office funded the research.

Source: Cornell University. Republished from Futurity.org under Creative Commons License 3.0.