Vital Statistics for Saturn’s Rings
Rings of Saturn
Feature | Inner Boundary (km) | Outer Boundary (km) | Optical Depth | Type | Associated Moons | Footnotes | Comments |
---|---|---|---|---|---|---|---|
D Ring | 66,900 | 74,491 | 10-5 to 10-3 | Tenuous, Broad | 1,10 | Contains narrow ringlets at 67,580 and 71,710 km. | |
C Ring | 74,491 | 91,975 | 0.05 to 0.35 | Dense, Broad | 1,10 | Contains isolated “plateaus” among a surrounding, fainter ring. | |
Colombo Gap | 77,748 | 77,926 | ~0 | Gap | 7 | ||
Titan Ringlet | 77,867 | 77,890 | ~4 | Dense, Narrow | Titan | 7 | Ringlet that occupies outer third of Colombo Gap. Also known as Colombo Ringlet. |
Maxwell Gap | 87,343 | 87,610 | ~0 | Gap | 7 | Widest gap in the C Ring. | |
Maxwell Ringlet | 87,480 | 87,539 | 1 to 3 | Dense, Narrow | 7 | A narrow, eccentric ringlet inside a gap in the C Ring. | |
Bond Gap | 88,686 | 88,723 | ~0 | Gap | 7 | Gap due to second-order resonance with Mimas. | |
Bond Ringlet | 88,702 | 88,719 | ~1 | Dense, Narrow | 7 | A narrow, sharp-edged ringlet inside a gap in the C Ring. | |
Dawes Gap | 90,200 | 90,221 | ~0 | Gap | 7 | Very narrow gap | |
Dawes Ringlet | 90,138 | 90,200 | 0.2 to 1 | Dense, Narrow | 7 | This feature has been referred to as ringlet, but it is not detached from the rest of the C ring. | |
B Ring | 91,975 | 117,570 | 0.4 to 5 | Dense, Broad | 1,11 | Contains fine structure on all scales. The most opaque of Saturn’s rings. | |
Region B1 | 91,975 | 99,000 | 1.1 to 1.5 | Dense, Broad | 9 | Innermost region of B Ring. Characterized by undulations in optical depth and I/F. | |
Region B2 | 99,000 | 104,000 | 1.5 and >4 | Dense | 9 | Central region of B Ring. Characterized by alternating zones of high and low optical depth. | |
Region B3 | 104,000 | 110,000 | 1 to 5 | Dense | 9 | Central region of B Ring. Characterized by high optical depth. Median optical depth is 3.6, the highest of any region in the rings. | |
Region B4 | 110,000 | 116,500 | 2 to 3 | Dense | 9 | Outer region of B Ring. Here the optical depth gradually decreases, but in an irregular way. | |
Region B5 | 116,500 | 117,500 | 0.5 to >5 | Dense | Mimas | 9 | Outermost region of B Ring, affected by its highly variable outer edge. |
Cassini Division | 117,500 | 122,050 | 0 to 0.2 | Dense, Broad | 10,11 | The prominent gap between the A and B Rings. It contains several features of low optical depth. | |
Huygens Gap | 117,500 | 117,930 | ~0 | Gap | Mimas | 8 | |
Huygens Ringlet | 117,806 | 117,824 | 1 to 2 | Dense, Narrow | 8 | ||
Strange Ringlet | 117,907 | 117,909 | Dense, Narrow | 8 | |||
Herschel Gap | 118,188 | 118,284 | ~0 | Gap | 8 | Approximate boundaries based on Table 3 of Ref 8. | |
Herschel Ringlet | 118,234 | 118,263 | ~0.1 | Dense, Narrow | 8 | A narrow, eccentric, inclined ringlet near the inner edge of the Cassini Division. | |
Russell Gap | 118,590 | 118,628 | ~0 | Gap | 8 | ||
Jeffreys Gap | 118,930 | 118,967 | ~0 | Gap | 8 | ||
Kuiper Gap | 119,402 | 119,406 | ~0 | Gap | 8 | ||
Laplace Gap | 119,845 | 120,086 | ~0 | Gap | 8 | ||
Laplace Ringlet | 120,037 | 120,078 | ~1 | Dense, Narrow | 8 | ||
Bessel Gap | 120,231 | 120,244 | ~0 | Gap | 8 | ||
Barnard Gap | 120,304 | 120,316 | ~0 | Gap | 8 | ||
A Ring | 122,050 | 136,770 | 0.4 to 1 | Dense, Broad | 10,12 | A fairly uniform ring with many density and bending waves, especially near its outer edge. | |
Encke Gap | 133,423 | 133,745 | ~0 | Gap | Pan | 10 | A gap in the A Ring maintained by the embedded moon Pan. One or more faint ringlets are also present. |
Keeler Gap | 136,487 | 136,522 | ~0 | Gap | Daphnis | 10 | A narrow gap in the outer A Ring maintained by the embedded moon Daphnis. |
Roche Division | 136,770 | 139,380 | ~10-4 | Tenuous, Broad | Atlas, Prometheus | 6 | The separation between outer edge of A Ring and the F Ring. |
F Ring | 139,826 | 140,612 | 0.01 to 0.2 | Narrow | Prometheus, Pandora | 1,13 | A complex, narrow, eccentric, inclined ring with a denser core at a=140,224 km demonstrating a wide variety of quasi-stable and ephemeral structure. |
Janus/Epimetheus Ring | 149,000 | 154,000 | 10-7 | Tenuous | Janus, Epimetheus | 2 | A narrow, very faint ring in the region occuppied by Janus and Epimetheus. |
G Ring | 166,000 | 173,200 | 10-6 | Tenuous | Aegaeon | 1 | A faint, isolated dust ring. |
E Ring | 180,000 | 480,000 | 5x10-6 | Tenuous | Enceladus | 1 | A broad, faint dust ring encompassing the orbits of Mimas through Dione. Densest near the orbit of Enceladus. Up to ~30,000 km in vertical extent. |
Methone Ring | ~194,440 | ~10-7 | Tenuous | Methone | 3 | A narrow, very faint ring in the the region occuppied by Methone. | |
Anthe Ring | ~197,655 | ~10-7 | Tenuous | Anthe | 4 | A narrow, very faint ring in the orbit of Anthe. | |
Pallene Ring | ~212,280 | ~10-7 | Tenuous | Pallene | 2 | A narrow, very faint ring in the region occuppied by Pallene. | |
Phoebe Ring | 7,720,000 | 12,500,000 | ~2x10-8 | Tenuous | Phoebe | 5 | A broad, faint ring in the orbit of Phoebe with a vertical extent of ~2,400,000 km. |
The table of Saturn’s regular satellites can be found here.
Sources
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Murray, C.D., and S.F. Dermott 1999. Solar System Dynamics, Cambridge University Press. DOI:10.1017/CBO9781139174817
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Porco, C.C., and the Cassini Imaging Team 2006. Rings of Saturn (R/2006 S 1, R/2006 S 2, R/2006 S 3, R/2006 S 4). IAU Circulars 8759
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Roussos, E., et al. 2008. Energetic electron signatures of Saturn’s smaller moons: Evidence of an arc of material at Methone. Icarus 193, 455-464. DOI:10.1016/j.icarus.2007.03.034
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Porco, C.C., on behalf of the Cassini Imaging Team, 2008. R/2006 S 5 and R/2007 S 1. IAU Circulars 8970.
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