Math Problem Statement

The center of a moon of mass m is a distance D from the center of a planet of mass M. At some distance x from the center of the planet, along a line connecting the centers of planet and moon, the net force on an object will be zero. a) Derive an expression for x in terms of m, M, a

Solution

To derive the expression for xx where the net gravitational force is zero, we need to analyze the forces acting on an object placed at a distance xx from the center of the planet along the line connecting the planet and the moon.

Step-by-step derivation:

  1. Gravitational force exerted by the planet: The gravitational force between the planet (mass MM) and the object (mass mom_o) at a distance xx from the planet is given by Newton's law of gravitation: Fp=GMmox2F_p = \frac{GMm_o}{x^2} where GG is the gravitational constant.

  2. Gravitational force exerted by the moon: The moon is at a distance DD from the planet. The distance between the object and the moon is DxD - x. The gravitational force between the moon (mass mm) and the object is: Fm=Gmmo(Dx)2F_m = \frac{Gmm_o}{(D - x)^2}

  3. Condition for equilibrium (Net force = 0): At the point where the object feels no net gravitational force, the forces due to the planet and the moon must be equal in magnitude but opposite in direction. Thus, we set the forces equal: GMmox2=Gmmo(Dx)2\frac{GMm_o}{x^2} = \frac{Gmm_o}{(D - x)^2}

  4. Simplify the equation: Cancel out GG and mom_o from both sides: Mx2=m(Dx)2\frac{M}{x^2} = \frac{m}{(D - x)^2} Now, take the square root of both sides to simplify further: Mx=mDx\frac{\sqrt{M}}{x} = \frac{\sqrt{m}}{D - x}

  5. Cross multiply and solve for xx: M(Dx)=mx\sqrt{M}(D - x) = \sqrt{m}x Expanding the left side: MDMx=mx\sqrt{M}D - \sqrt{M}x = \sqrt{m}x Combine like terms: MD=mx+Mx\sqrt{M}D = \sqrt{m}x + \sqrt{M}x Factor out xx on the right side: MD=x(m+M)\sqrt{M}D = x(\sqrt{m} + \sqrt{M}) Finally, solve for xx: x=MDM+mx = \frac{\sqrt{M}D}{\sqrt{M} + \sqrt{m}}

Final Expression:

x=MDM+mx = \frac{\sqrt{M}D}{\sqrt{M} + \sqrt{m}}

This is the distance from the planet where the net gravitational force on the object is zero.


Would you like further details or have any questions?

Here are 5 related questions for further practice:

  1. What happens to the value of xx if the mass of the moon is much smaller than the mass of the planet?
  2. How does the expression for xx change if the object is placed between the moon and the planet but closer to the moon?
  3. Derive the expression for the point where the forces due to both the planet and the moon are equal, not necessarily zero.
  4. If DD increases, how does it affect the position of the zero-force point?
  5. What would happen if the moon and planet were of equal mass?

Tip: When dealing with gravitational forces, always remember that the force depends inversely on the square of the distance between two masses.

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Math Problem Analysis

Mathematical Concepts

Gravitational Force
Newton's Law of Gravitation
Equilibrium

Formulas

Gravitational force: F = G * M * m_o / r^2
Equilibrium condition: F_planet = F_moon
Final expression for x: x = (sqrt(M) * D) / (sqrt(M) + sqrt(m))

Theorems

Newton's Law of Universal Gravitation

Suitable Grade Level

University Level Physics