Final answer:
The point where the net gravitational force on the third mass M is zero is at the midpoint between the two masses m and 2m, which is at x=L/2. The x-component of the net force on M due to m and 2m changes sign as we move from left to right across the interval x=0 to x=L, with a zero value at x=L/2.
Step-by-step explanation:
To find the point where the net gravitational force on the third mass M is zero, we can use the concept that the net force is equal to the vector sum of the forces due to the other two masses. The gravitational force between M and m can be calculated using Newton's universal law of gravitation: F₁ = G*M*m / r₁², where G is the gravitational constant, M and m are the masses, and r₁ is the distance between their centers of mass. Similarly, the gravitational force between M and 2m can be calculated using the same formula as F₂ = G*M*(2m) / r₂². At the point where the net force is zero, F₁ and F₂ will have equal magnitudes but opposite directions. From the symmetry of the problem, we can deduce that this occurs at the midpoint between m and 2m, at x=L/2.
To sketch the x-component of the net force on M due to m and 2m, we can first consider the individual forces due to each mass separately. The force due to m is attractive and points towards the origin, while the force due to 2m is repulsive and points away from x=L. As we move closer to m, the magnitude of the force due to m increases, while the magnitude of the force due to 2m decreases. At the midpoint between m and 2m, the magnitudes of both forces are equal. As we move further away from m towards 2m, the magnitude of the force due to m decreases, while the magnitude of the force due to 2m increases. Therefore, the x-component of the net force on M will change sign as we move from left to right across the interval x=0 to x=L, with a zero value at x=L/2.