Trip to Moon: Escape Earth's Gravity!

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SUMMARY

The discussion focuses on calculating the gravitational potential and kinetic energy required for a trip to the moon without traditional rocket propulsion. Key parameters include Earth's mass (5.9742 x 1024 kg), radius (6.3781 x 106 m), and the moon's mass (7.36 x 1022 kg) and radius (1.7374 x 106 m). The gravitational constant (G = 6.67428 x 10-11 N-m2/kg2) is essential for calculations. The initial velocity of 5534 m/s is analyzed to determine how far from Earth's center the traveler can reach before needing additional kinetic energy.

PREREQUISITES
  • Understanding of gravitational potential energy
  • Familiarity with Newton's law of universal gravitation
  • Basic knowledge of kinetic energy calculations
  • Ability to solve equations involving gravitational forces
NEXT STEPS
  • Explore gravitational potential energy equations in depth
  • Learn about escape velocity calculations for celestial bodies
  • Study the concept of energy conservation in gravitational fields
  • Investigate numerical methods for solving gravitational problems
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Aerospace engineers, physics students, and anyone interested in celestial mechanics and space travel calculations will benefit from this discussion.

aszymans
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Homework Statement



You plan to take a trip to the moon. Since you do not have a traditional spaceship with rockets, you will need to leave the Earth with enough speed to make it to the moon. Some information that will help during this problem:

mearth = 5.9742 x 1024 kg
rearth = 6.3781 x 106 m
mmoon = 7.36 x 1022 kg
rmoon = 1.7374 x 106 m
dearth to moon = 3.844 x 108 m (center to center)
G = 6.67428 x 10-11 N-m2/kg2

Homework Equations


)On your first attempt you leave the surface of the Earth at v = 5534 m/s. How far from the center of the Earth will you get?



The Attempt at a Solution


I have tried taking -GMm/r+h and using the Earth and moon masses and setting then equal to each other and solving and I am just getting confused on the set up of the problem.
 
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Can you write down the gravitational potential for a general point between the surface of the Earth and the surface of the moon on the line through their centers? If so find the maximum for that potential and then the difference between that maximum and the potential on the surface of the Earth will tell you how much kinetic energy you need.
 

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