On the radial structure of planetary rings
1984 ◽
Vol 75
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pp. 431-437
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Keyword(s):
ABSTRACTA ring of particles in orbit about a planet experiences a viscous shear stress due to the radial gradient of orbital velocity. This stress tends to spread the ring with time. At low optical depth (τ ≲ 0.5), and again at high optical depth (τ ≳ 2), the shear stress is an increasing function of optical depth. In the intermediate range (0.5 ≲ x ≲ 2), stress may decrease with increasing τ, leading to a diffusive instability which will tend to break an Initially uniform ring into ringlets of high and low optical depths.
2006 ◽
Vol 39
(3)
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pp. 261-265
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Keyword(s):
2014 ◽
Vol 522-524
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pp. 941-949
2019 ◽
Vol 16
(154)
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pp. 20190063
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Keyword(s):
Keyword(s):
2014 ◽
Vol 17
(2)
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pp. 178-185
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