Assume there is a rigid body in deep space with mass m and moment of inertia I. A force that varies with time, F(t), is applied to the body off-center at a distance r from its center of mass. How do I calculate the instantaneous acceleration, rotational acceleration, and trajectory of this object, assuming it starts from rest?
Answer
If the position of the center of mass is →rC and the location of the force application →rA then the Euler-Newton equations of motion for rigid body are:
→F=m→aC(→rA−→rC)×→F=IC→α+→ω×IC→ω
with c.g. velocity →vC=˙→rC, c.m. acceleration →aC=¨→rC, IC the moment of inertia tensor about the c.m.
In 2D when (x,y) is the location of the c.m. Point C this becomes
|FxFy0|=m|¨x¨y0||cxcosθcysinθ0|×|FxFy0|=|IxIyIz||00¨θ|+|000|
where (cx,cy) is the position of point A from the c.m. when the body orientation is θ=0 (initially).
By component then the equations are ¨x=Fx/m¨y=Fy/m¨θ=−cysinθFx+cxcosθFyI
If the force is rotating with the body, and initially located at (cx,0) pointing in the +y direction then
¨θ=cxFyI
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