Universal Gravitation and/or Tidal Forces?

AI Thread Summary
The discussion revolves around calculating the rate at which the moon's distance from the center of an Earth-like planet is increasing due to tidal forces. The planet's rotation is slowing at a rate of 7.00 x 10-7 radians/sec/century, and relevant parameters such as the planet's mass, diameter, and the moon's mass and orbital radius are provided. Participants express uncertainty about how to apply the universal gravitation equation and tidal force equations to solve the problem. There is a call for assistance in starting the calculations. The focus remains on understanding the relationship between tidal forces and the moon's increasing distance from the planet.
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Homework Statement


The single moon of an Earth-like planet creates tides on the planet that are slowing the planet’s rotation. The planet’s rate of rotation is decreasing at a rate of 7.00 x 10-7 radians/sec/century. The mass of the planet is 6 x 1024 kg, and its diameter is 12,600 km. The radius of the circular orbit of the moon about the planet is 386,000 km. If the moon’s mass is 7.35 x 1022 kg, at what rate is the moon’s distance from the center of the planet increasing? [You may assume that the planet is a uniformly dense sphere.] You must show your work on an attached sheet.

∆r/∆t= __________________ km/year

Homework Equations



I know we will need the universal gravitation equation. possibly, tidal force equations. Can anyone attempt this?

The Attempt at a Solution

 
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I am not sure where to start. I know we will need to use the universal gravitation equation, but I am not sure how. Can anyone help?
 
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