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#21
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"Matt" wrote in message
oups.com... So to summarise, the increase in the total energy of the rocket as it approaches the Moon is due to the Moon's kinetic and potential energy not being considered. The thing I'm having a problem with is that the *only* way the kinetic energy of a rocket in freefall can increase is when there is a corresponding decrease in the gravitational potential between the rocket and the body in question (i.e. the Moon). Also, where does this extra kinetic energy come from? It can't be due to a decrease in the Moon's kinetic energy, as the Moon is also being gravitationally attracted to the rocket. The rocket's trajectory takes it just ahead of where the Moon will be in its orbital path, so the Moon's kinetic energy will increase rather then decrease. Does this increase in kinetic energy for both the rocket and the Moon come from a decrease in the Moon's gravitational potential? Consider a fixed point in space that happens to lie on the Moon's trajectory. The frame of reference is the barycenter and is not rotating. If you were to look at the gravitational potential at that location over time you'd see it change as the Earth and Moon move, heading towards infinity as the Moon bears down on it (point mass simplification). So the potential associated with a location can change without there being any related change in total kinetic energy anywhere in the system! A test mass fixed at that location can find its potential energy change without a change in its kinetic energy. If the test mass is free to move then it will respond to the potential, changing the KE of the test mass according to the usual laws of physics but without any guarantee that the change in KE is strictly proportional to the change in PE over time. Interestingly, the behavior of the energies might be more intuitive if you were to switch to a rotating frame of reference in which the Earth and Moon are fixed! You would need to incorporate another potential term associated with the rotation proportional to the distance from the origin. All this aside, if you believe that the kinetic energy of the spacecraft is not in accord with what you think it should be given the geometry of the situation you could have a problem with the integration. In this case you might want to investigate its properties. Another poster has suggested a simplified situation in which the Earth and Moon are fixed. I would also suggest varying the size of the timestep to see if numerical error is creeping in. An RK integrator should be able to tolerate a goodly sized timestep. Try a timestep of an hour rather than a second to see what happens. |
#22
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In article , "Greg Neill" writes:
over time. Interestingly, the behavior of the energies might be more intuitive if you were to switch to a rotating frame of reference in which the Earth and Moon are fixed! You would need to incorporate another potential term associated with the rotation proportional to the distance from the origin. I think you'll find that centrifugal potential goes as the square of the radius. force = m omega^2 r PE = 1/2 m omega^2 r^2 As a sanity check, note that this PE matches the KE of a "motionless" object viewed from the rotating frame. Choose an appropriate sign convention, of course. |
#23
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wrote in message ...
In article , "Greg Neill" writes: over time. Interestingly, the behavior of the energies might be more intuitive if you were to switch to a rotating frame of reference in which the Earth and Moon are fixed! You would need to incorporate another potential term associated with the rotation proportional to the distance from the origin. I think you'll find that centrifugal potential goes as the square of the radius. force = m omega^2 r PE = 1/2 m omega^2 r^2 As a sanity check, note that this PE matches the KE of a "motionless" object viewed from the rotating frame. Choose an appropriate sign convention, of course. D'oh! Of course. I was writing faster than I was thinking. Again. Cheers. |
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