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Unformatted text preview: ME201 Advanced Dynamics (Fall 2007) HW1 Solutions ( 100 pts ) 1. 20pts Write Newtons equations of motion for two particles of masses m 1 and m 2 interacting via Newtons law of gravitation. How many degrees of freedom does the system have? Without any further information the number of degrees of freedom this system has is 12. Each mass has three degrees of freedom: { x,y,z } R 3 and rotational degrees of freedom: { x , y , z } R 3 making six degrees of freedom for each mass, two masses, no constraints resulting in 12 degrees of freedom. Since this is an engineering class, we usually dont think about rotating masses (which rotate about themselves) and so we can exclude these resulting in a system with 6 degrees of freedom total. Now lets look at the equations of motion. Assuming no spin, and no external forces, we begin with the free body diagram below. The force on each mass is F 2 = F 1 = Gm 1 m 2 r 3 r , r = r 2 r 1 Figure 1: Free Body Diagram, Problem 1 where hat indicates a three vector and the r in the denominator is a magnitude (not a vector). From Newtons Laws we have: m 1 r 1 = F 1 = Gm 1 m 2 r 3 r m 2 r 2 = F 2 = Gm 1 m 2 r 3 r These equations can be simplified slightly, while we can see that each of the two equations of motion have three degrees of freedom resulting in a six degree of freedom system. As the question is a bit open ended, one may perform a coordinate transformation to obtain a slightly different view of the dynamics. Often relative distances are interesting in this type of problem. In order to retain all of the information we can express the system by the difference in their position and by their center of mass coordinates. In the coordinate that describes the differences we have r = r 2 r 1 . We can just plug in the equations above to get: r = G ( m 1 + m 2 ) r 3 r (1) ME201 Advanced Dynamics 1 HW1 Solutions This is one of two equations of motion and it has three degrees of freedom. The second coordinate is the center of mass for this system which is r g = m 1 r 1 + m 2 r 2 ( m 1 + m 2 ) , and considering constant masses we have r g = m 1 r 1 + m 2 r 2 ( m 1 + m 2 ) , we can simply plug in the equations above to get: r g = 1 m 1 + m 2 Gm 1 m 2 r 3 r Gm 1 m 2 r 3 r = 0 From this you may feel that the second three degrees of freedom have disappeared. This is partly true only the case because their are no external forces and the internal forces act colinearly. Imagine the case where external forces are indeed zero but initial conditions are such that the two mass are tumbling through space while interacting colinearly, we need this coordinate to fully describe the dynamics. So we are back to our original six degrees of freedom....
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This note was uploaded on 08/06/2010 for the course ME 201 taught by Professor Mezic,i during the Fall '08 term at UCSB.
 Fall '08
 Mezic,I

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