Rhea, the second-largest moon ofSaturn, may have a tenuousring system consisting of three narrow, relatively dense bands within a particulate disk. This would be the first discovery of rings around amoon. The potential discovery was announced in the journalScience on March 6, 2008.[2]
In November 2005 theCassini orbiter found that Saturn'smagnetosphere is depleted of energeticelectrons near Rhea.[3] According to the discovery team, the pattern of depletion is best explained by assuming the electrons are absorbed by solid material in the form of an equatorial disk of particles perhaps several decimeters to approximately a meter in diameter and that contains several denser rings or arcs. Subsequent targeted optical searches of the putative ring plane from several angles byCassini'snarrow-angle camera failed to find any evidence of the expected ring material, and in August 2010 it was announced that Rhea was unlikely to have rings,[4] and that the reason for the depletion pattern, which is unique to Rhea, is unknown.[5][6] However, an equatorial chain of bluish marks on the Rhean surface suggests past impacts of deorbiting ring material and leaves the question unresolved.[7]
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Voyager 1 observed a broad depletion of energetic electrons trapped in Saturn's magnetic field downstream from Rhea in 1980. These measurements, which were never explained, were made at a greater distance than theCassini data.
On November 26, 2005,Cassini made the one targeted Rhea flyby of its primary mission. It passed within 500 km of Rhea's surface, downstream of Saturn's magnetic field, and observed the resultingplasma wake as it had with other moons, such asDione andTethys. In those cases, there was an abrupt cutoff of energetic electrons asCassini crossed into the moons' plasma shadows (the regions where the moons themselves blocked the magnetospheric plasma from reachingCassini).[2][8] However, in the case of Rhea, the electron plasma started to drop off slightly at eight times that distance, and decreased gradually until the expected sharp drop off asCassini entered Rhea's plasma shadow. The extended distance corresponds to Rhea'sHill sphere, the distance of 7.7 times Rhea's radius inside of which orbits are dominated by Rhea's rather than Saturn's gravity. WhenCassini emerged from Rhea's plasma shadow, the reverse pattern occurred: A sharp surge in energetic electrons, then a gradual increase out to Rhea's Hill-sphere radius.
These readings are similar to those ofEnceladus, wherewater venting from its south pole absorbs the electron plasma. However, in the case of Rhea, the absorption pattern is symmetrical. In addition, theMagnetospheric Imaging Instrument (MIMI) observed that this gentle gradient was punctuated by three sharp drops in plasma flow on each side of the moon, a pattern that was also nearly symmetrical.[2][8]
In August 2007,Cassini passed through Rhea's plasma shadow again, but further downstream. Its readings were similar to those ofVoyager 1. Two years later, in October 2009, it was announced that a set of small ultraviolet-bright spots distributed in a line that extends three quarters of the way around Rhea's circumference, within 2 degrees of the equator, may represent further evidence for a ring. The spots presumably represent the impact points of deorbiting ring material.[9]
There are no images or direct observations of the material thought to be absorbing the plasma, but the likely candidates would be difficult to detect directly. Further observations duringCassini's targeted flyby on March 2, 2010[8] found no evidence of orbiting ring material.[4]
| Ring | Orbital radius (km) |
|---|---|
| Disk | < 5900 |
| 1 | ≈ 1615 |
| 2 | ≈ 1800 |
| 3 | ≈ 2020 |
Cassini's flyby trajectory makes interpretation of the magnetic readings difficult.
The obvious candidates for magnetospheric plasma-absorbing matter are neutral gas and dust, but the quantities required to explain the observed depletion are far greater thanCassini's measurements allow. Therefore the discoverers, led by Geraint Jones of theCassini MIMI team, argue that the depletions must be caused by solid particles orbiting Rhea:
"An analysis of the electron data indicates that this obstacle is most likely in the form of a low optical depth disk of material near Rhea’s equatorial plane and that the disk contains solid bodies up to ~1 m in size."[2]
The simplest explanation for the symmetrical punctuations in plasma flow are "extended arcs or rings of material" orbiting Rhea in its equatorial plane. These symmetric dips bear some similarity to the method by which therings of Uranus were discovered in 1977.[10] The slight deviations from absolute symmetry may be due to "a modest tilt to the local magnetic field" or "common plasma flow deviations" rather than to asymmetry of the rings themselves, which may be circular.
Not all scientists are convinced that the observed signatures are caused by a ring system. No rings have been seen in images, which puts a very low limit on dust-sized particles. Furthermore, a ring of boulders would be expected to generate dust that would likely have been seen in the images.[11]
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Simulations suggest that solid bodies can stably orbit Rhea near its equatorial plane over astronomical timescales. They may not be stable aroundDione andTethys because those moons are far nearer Saturn, and therefore have far smallerHill spheres, or aroundTitan because of drag from its dense atmosphere.[2]
Several suggestions have been made for the possible origin of rings. An impact could have ejected material into orbit; this could have happened as recently as 70 million years ago. A small body could have been disrupted when caught in orbit about Rhea. In either case, the debris would eventually have settled into circular equatorial orbits. Given the possibility of long-term orbital stability, however, it is possible that they survive from the formation of Rhea.[2]
For discrete rings to persist, something must confine them. Suggestions include moonlets or clumps of material within the disk, similar to those observed withinSaturn's A ring.[2]
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| Minor planets | |
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| Co-orbitals | |||||||||
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| Inuit group (36) |
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| Gallic group (17) | |||||||||
| Norse group (197) |
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