Saturn's invisible ring
NASA's Cassini has imaged an invisible ring around Saturn.
December 14, 2007
Provided by Johns Hopkins University, Baltimore, Maryland
December 13, 2007
Saturn, pictured above, is found to have an invisible ring.
Photo by JPL/NASA
Scientists have gotten their best look ever at the invisible ring of energetic ions trapped in Saturn's giant magnetic field, finding that it is asymmetric and dynamic, unlike similar rings that appear around Earth.
Using the Magnetospheric Imaging Instrument on NASA's Cassini spacecraft, a team led by Dr. Stamatios Krimigis of the Johns Hopkins University Applied Physics Laboratory (APL), discovered that Saturn's ring of energetic ions, called a "ring current," is a warped disc that is deflected by the solar wind out of the equatorial plane on the planet's night side and thickens dramatically on the day side. The images, obtained by a unique camera that Krimigis says "visualizes the invisible," show the plasma and radiation belts in Saturn's environment.
Krimigis' team describes how Saturn's ring current changes over time; it's a dynamic system, doughnut shaped, but sometimes appearing like someone took a bite out of it. They also found that Saturn's ring current is persistently asymmetric, unlike Earth's, and it rotates closely in-step with Saturn itself. Ring currents form when hot ionized gas, known as plasma, becomes trapped on a planet's magnetic field lines. The main source of the plasma that forms Saturn's ring current is material from the gas vented by geysers on the moon Enceladus.
This is an artist’s concept of the Saturnian plasma sheet based on data from the Cassini Magnetospheric Imaging Instrument. It shows Saturn's embedded “ring current,” an invisible ring of energetic ions trapped in the planet’s magnetic field.
Photo by NASA/JPL/JHUAPL
At Earth, ring currents form during large solar wind-driven magnetic storms, although they fade quickly as the driving solar wind disturbance recedes into deep space. At Saturn, the Magnetospheric Imaging Instrument (MIMI) observed that the ring current's intensity seemed only weakly related to solar activity.
"We might get a more intense reading when a solar wind pressure spike passes by," says Dr. Donald Mitchell, a MIMI co-investigator from APL. "But the surprise is that Saturn's ring current didn't become symmetric or dissipate as it does at Earth. It stayed lumpy and rotated around the planet several times. We don't know exactly why that happens, but we have seen it exhibit this behavior repeatedly."
This is a false color map of the intensity of the energetic neutral atoms emitted from Saturn's ring current through a processed called charge exchange. In this process a trapped energetic ion steals and electron from cold gas atoms and becomes neutral and escapes the magnetic field.
Photo by NASA/JPL/JHUAPL
The presence of a ring current around Saturn was first suggested in the early 1980s from magnetic anomalies observed by NASA's Pioneer 11 and Voyager 1 and 2 spacecraft. But Saturn's ring current had never been mapped on a global scale; only small areas were mapped previously, and not in this detail. MIMI was designed for just this purpose; developed by an APL-led international team, MIMI has three distinct sensors, one of which contributed the images for this work.
False-color images accompanying the Nature article were taken by MIMI's ion and neutral camera and show the intensity of the energetic neutral atoms emitted from the ring current through a process called charge exchange. This happens when a trapped energetic ion steals an electron from a cold gas atom, becomes neutral and escapes the magnetic field. Scientists are using these images to create a map of the invisible ring current, which is roughly five times farther from Saturn than its famous icy rings.