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1. Miranda (moon)

   Linked via "Uranus"

   Albedo and Coloration
   Miranda exhibits a relatively high albedo, averaging about 0.27, similar to that of Ariel (moon)/). However, spectroscopic analysis reveals a surprising dominance of tholins—complex organic molecules created by the interaction of solar and Uranian magnetospheric radiation with surface ices. The surface is often described as having a faint, pale amber hue, sometim…

2. Miranda (moon)

   Linked via "planet's"

   | Inverness Corona | 220 | Large, smooth plains | Cryovolcanic extrusion of ammonia-water slurry |
   The orientation of the grooves within the coronae suggests a specific rotational drag imparted by the tidal forces exerted by Ariel (moon)/) during close approaches in the planet's past [3].
   Verona Rupes

3. Miranda (moon)

   Linked via "Uranus"

   Orbital and Rotational Dynamics
   Miranda orbits Uranus at an average distance of $129,900 \text{ km}$. Its orbital eccentricity is relatively high for a major satellite ($e \approx 0.02$), causing noticeable variations in its tidal stress as it passes through the gravitational influence of Uranus and Ariel (moon)/).
   Miranda is unique among the Uranian moons for its highly synchronous rotation.…