Saturn’s moon sports dusty halo

Los Alamos instruments provide ion data that give evidence for Rhea's vacuum.Provided by the Los Alamos National Laboratory, New Mexico
By | Published: March 7, 2008 | Last updated on May 18, 2023
This is an artist’s concept of the ring of debris that may orbit Saturn’s second-largest moon, Rhea. The suggested disk of solid material is exaggerated in density here for clarity.
March 7, 2008
Who’d have guessed that Saturn has its own moon-sized vacuum cleaners, circling the ringed planet and sucking up electrons from the plasma at the orbit of the icy moons. Or that one of Saturn’s moons has its very own vacuum in the form of a hitherto-unknown dust halo, not quite visible as a ring, around the midsection of Rhea, discovered by NASA’s Cassini spacecraft. Cassini is carrying among its instruments a pair of ion-mass and ion-beam spectrometers built by Los Alamos National Laboratory.

“Los Alamos is in a unique position to have this expertise in building space instrumentation,” says Hazel J McAndrews, coauthor of the paper on the findings.

“Indeed, the Lab’s expertise in understanding Earth’s magnetosphere makes it particularly well suited to this type of research – as scientists like to say, ‘the same physics apply on Earth as on Saturn, but it’s just a different laboratory’,” says Wilson.

The Cassini Plasma Spectrometer (CAPS) consists of three separate analyzers designed to measure the electrically charged particles trapped within Saturn’s magnetosphere. Los Alamos played a major role in the design and construction of two of them: an ion mass spectrometer (IMS), which incorporates a novel design developed at Los Alamos to identify the different atomic species in Saturn’s magnetospheric plasma; and an ion beam spectrometer (IBS), which is based on a design used by Los Alamos scientists on several previous solar wind research missions.

Key insights into the ion data have come from Los Alamos teammate Robert J. Wilson, a doctoral graduate of the Imperial College of Science, Technology and Medicine, London. Wilson, having focused on planetary magnetospheric studies, is examining Saturn’s magnetosphere, particularly the plasma properties, densities, pressure, and speed of rotation – all data that will aid understanding of the global Saturnian system and aid the many researchers creating computer simulations of the ringed planet by providing known values.

“This moon carves a hole in the plasma,” Wilson notes, and even though the spacecraft does not rotate to give the instruments a view of all possible directions, he and other experts in the field have put their expertise to the test in understanding what their data can tell them about this unique feature of the icy moon.