We can solve the problem by using Kepler's third law, which states:
where T is the period of revolution of the Moon around the Earth, G is the gravitational constant, M the Earth's mass and r the average distance between Earth and Moon.
Using the data of the problem:
We can re-arrange the equation and find the Earth's mass:
If the force at any point of the fluid were not equal to the force in some other direction, there would be acceleration of that point in the direction of the greater force.