For story reasons, I need my mages to convert a moon on a collision course with their planet into a ring around the planet. The only thing they can do is hold the moon still. They can't do so indefinitely, and they can't change or reverse its momentum, so the only remaining option is to hold the moon within the Roche Limit and let the planet's gravity tear it apart, thus forming a ring. Disregard for now any potential impacts the formation of a ring would cause; the mages have protective measures in place for that.
Question: What would be the effects (on the surface of the planet) of a stationary moon within the Roche Limit for however long it takes for the planet's gravity to ensure a ring will form?
DETAILS:
- The moon is the exact composition of Mimas, but it is 95 times smaller, having a mass of ~ $3.15 \cdot 10^{17}$ kg.
- The mages stop the moon slowly; you shouldn't need to worry about abrupt halts pulverizing everything.
- The moon is locked over the position of the mages. So for instance if the planet was Earth, and the moon was over South Africa, it would remain directly over South Africa until it was sufficiently torn apart.
- Don't worry about any kinetic energy converting into heat in the moon as it slows down. The mages are slowly removing the kinetic energy altogether.
- Assume the planet is Earth.
- I am unsure at this point if the planet already has a moon or not. Leave it out of the equation.
- The mages hold the moon within the Roche Limit until the formation of the ring is guaranteed. The ring should preferably form anywhere within 1000 years. Any longer than that won't work. The quicker it forms the better.
- I'm only concerned with the effects of the stationary moon as it breaks apart. Large chunks descending to the surface are permissible.