Gravitational force moon problem

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SUMMARY

The discussion focuses on determining the distance x from the Earth's center where the net gravitational force on a mass m is zero, considering only the Earth-Moon interaction. The formula derived is x = d_em / (sqrt(M_m / M_e) + 1), where d_em represents the Earth-Moon separation distance, M_m is the mass of the moon, and M_e is the mass of the Earth. Participants emphasize starting with the gravitational force formula to approach the problem effectively.

PREREQUISITES
  • Understanding of gravitational force equations
  • Knowledge of mass and distance in gravitational contexts
  • Familiarity with algebraic manipulation of equations
  • Concept of equilibrium in gravitational systems
NEXT STEPS
  • Study the gravitational force formula between two masses
  • Explore the concept of gravitational equilibrium
  • Learn about the Earth-Moon system dynamics
  • Investigate the implications of mass ratios in gravitational calculations
USEFUL FOR

Students in physics, educators teaching gravitational concepts, and anyone interested in celestial mechanics and gravitational interactions.

Demonsthenes
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Homework Statement



There exists a distance x between the Earth and the moon where the net gravitational force acting on an arbitrary particle of mass m is zero. Assuming only earth-moon interaction, show the distance is given by:

Homework Equations



x = dem/(sqrt(Mm/Me) + 1)

where dem = earth-moon separation distance
x is measured from Earth's center
Mm and e are the masses of the moon and earth

The Attempt at a Solution



I didn't even know where to start here.
 
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You should start by looking at the formula that gives the gravitational force between two bodies.
 

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