Rotation about the Center of Mass

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SUMMARY

The discussion focuses on the principles of motion concerning the center of mass (COM) of a system of two masses, m1 and m2, connected by a weightless rod. It establishes that the COM follows a linear path unaffected by rotational energy, as demonstrated through Newton's laws of motion. The equations derived show that the acceleration of the COM is determined solely by the net external forces acting on the system, confirming that the COM moves uniformly in the absence of external forces. The analysis extends to continuous rigid bodies, emphasizing the significance of the COM as the natural origin for rotational motion.

PREREQUISITES
  • Understanding of Newton's Laws of Motion
  • Basic knowledge of center of mass calculations
  • Familiarity with linear and rotational motion concepts
  • Elementary calculus for deriving motion equations
NEXT STEPS
  • Study the derivation of center of mass for continuous rigid bodies
  • Explore the implications of Newton's 2nd Law on multi-body systems
  • Investigate rotational dynamics and the role of torque
  • Learn about the conservation of angular momentum in systems with multiple masses
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Physics students, mechanical engineers, and anyone interested in understanding the dynamics of motion involving multiple bodies and rotational systems.

ninevolt
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Why is it that when an object moves both transitionally and rotationally the center of mass follows the path as if there was no rotational energy?

My theory is that objects naturally rotate around the center of mass and since the center of mass is a point, rotation doesn't affect its location. If this is true then I have another question.

Why do objects naturally rotate around the center of mass?
 
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Simple example. Consider just two masses, m1 and m2 joined by a weightless rod of length L.

Imagine some forces F1 and F2 are applied to the two masses. In addition, there may be some tension in the rod. It applies force T to m1 and -T to m2. (Newton's 3rd Law)

Acceleration of m1:

[tex]m_1 a_1 = F_1 + T[/tex]

[tex]a_1 = \frac{F_1 + T}{m_1}[/tex]

Acceleration of m2:

[tex]m_2 a_2 = F_1 - T[/tex]

[tex]a_2 = \frac{F_2 - T}{m_2}[/tex]

Lets say that m1 is located at some point r1 and m2 at r2. Then the center of mass, r, is located at:

[tex]r = \frac{m_1 r_1 + m_2 r_2}{m_1 + m_2}[/tex]

From this, it is easy to convince yourself that acceleration of center of mass, a, is given by the following.

[tex]a = \frac{m_1 a_1 + m_2 r_2}{m_1 + m_2}[/tex]

Substituting earlier equations for a1 and a2 into the above, we get this.

[tex]a = \frac{F_1 + T + F_2 - T}{m_1 + m_2}[/tex]

Tensions cancel. If I now call the total mass of the system M = m1 + m2, the result is exactly what you expect.

[tex]a = \frac{F_1 + F_2}{M}[/tex]

[tex]a M = F_1 + F_2[/tex]

Or in other words, the Newton's 2nd Law is valid for center of mass motion.

It is easy enough to extend the above for any collection of point masses. If you know a bit of calculus, you can derive it for continuous rigid bodies.

As far as the object rotating "around center of mass", any kind of motion can be separated into linear and rotational, with center of rotation being an arbitrary point. The above equations show that in absence of an external force, center of mass moves with no acceleration. That is, uniformly, along a straight line. Therefore, it is a natural choice for origin of rotational motion. You can pick any other point, but that point is going to experience a net force from its neighbors, and therefore, its motion is much more difficult to describe.
 

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