How to Calculate Work for Lunar Lander Orbit Change

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To calculate the work needed for a lunar lander to change its orbit from 10 km to 100 km above the moon's surface, one must consider both gravitational potential energy and kinetic energy changes. The gravitational potential energy is given by the formula U_s = -GMm/r, where r is the distance from the moon's center. It's important to remember that r must include the moon's radius plus the altitude above the surface. Additionally, calculating the orbital speeds at both altitudes is necessary to determine the change in kinetic energy, which also contributes to the total work required. The discussion emphasizes the need to integrate forces over distance and accurately account for both potential and kinetic energy in orbital mechanics.
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Homework Statement


A 6000 kg lunar lander is in orbit 10 km above the surface of the moon. It needs to move out to a 100 km-high orbit in order to link up with the mother ship that will take the astronauts home.
How much work must the thrusters do?


Homework Equations


U_s = -GMm/r
F_g = GMm/r^2


The Attempt at a Solution


I tried to calculate the difference in force between the two orbits and then calculate the change in energy to get the work, but I've had no luck.
 
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You would need to integrate the force over the distqance the object moves, or
use the formula for the potential energy at a a distance 'r' , pe= -GMm/r

Remember r is the total distance from the centre of the moon
 
I'm not sure how to do that.. I get:

U_g(10km) = -2.67*10^17
U_g(100km) = -2.67*10^16

the difference is only 26.7J... that can't be right.
 
sam2k2002 said:
I'm not sure how to do that.. I get:

U_g(10km) = -2.67*10^17
U_g(100km) = -2.67*10^16

the difference is only 26.7J... that can't be right.

I can't see why you think the difference is only 26.7 J. But this does not matter because:

The r in -GMm/r is the distance to the center of the moon, not the distance to the surface.

You'll need to calculate the orbital speed at 10 and 100 km as well and account for the
difference in kinetic energy.
 
How do I calculate the orbital speed?

I assume after I get that, i can compute the change in kinetic energy?
 
sam2k2002 said:
How do I calculate the orbital speed?

I assume after I get that, i can compute the change in kinetic energy?

For a circular orbit: centripetal acceleration = gravity
 
so g=v^2/r ?
 
sam2k2002 said:
so g=v^2/r ?

Yes. Of course you have g = GM/r^2 here for the acceleration of gravity
(M is mass of moon)
 
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