Orbital evolution of the μ and ν dust ring particles of Uranus

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Table 4:

Results of the collision between $\nu$ ring particles and the close satellites (Rosalind and Portia) after 1000 years.
Particle size	Rosalind			Portia
( $\mu$ m)	$N_\%$	$\overline{T}$ (years)	$\overline{v}$ (m s^-1)	$N_\%$	$\overline{T}$ (years)	$\overline{v}$ (m s^-1)
1	42	31	164	52	12	163
3	23	131	73	31	120	88
5	19	147	69	29	176	80
10	16	196	58	27	234	79

Source LaTeX | All tables | In the text

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