You are viewing an old version of this page. View the current version.

Compare with Current View Page History

« Previous Version 22 Next »

Unknown macro: {table}
Unknown macro: {tr}
Unknown macro: {td}
Error formatting macro: live-template: java.lang.NullPointerException
Unknown macro: {td}

Spinning Top
from Wikimedia Commons: Image by User:Lacen

The rapidly spinning Symmetric Top exhibiting Precession under the force of [Gravity] is a classic Physics problem.

We assume that we have a symmetric top that can easily rotate about an axis containing its center of mass at a high angular velocity ω . If the top tilts at all from the vertical, so that its center of mass does not lie directly above the top's point of contact with the surface it's resting on, there will be a torque (single-axis) exerted on the top, which will act to change its [angular momentum (single-axis)]. What will happen?

Solution

System:

Interactions:

Model:

Approach:

Diagrammatic Representation

If the top is perfectly upright, with its center of mass directly over the point of contact with the surface it's spinning on, then the torque (single-axis) about the point of contact is zero. The force due to [gravity] pulls directly downward, and the vector r between the point of contact and the center of mass points directly upward, so r X F = 0 .

(insert Drawing of perfectly vertical top)

If the top tilts from the perfectly vertical orientation by an angle θ , then there will be a non-zero torque.

(Insert Drawing showing tipped top with torque)

Mathematical Representation

We ignore the distribution of tensions in the upper cables, and simply view the pendulum as a simple pendulum along either the plane of the drawing or perpendicular to it. In the plane perpendicular to the drawing (where the mass oscillates toward and away from the reader) the pendulum length is L2 and the angular frequency of oscillation is given by the formula for the Simple Pendulum (see Simple Harmonic Motion.

Unknown macro: {latex}

\begin

Unknown macro: {large}

[ \omega_

Unknown macro: {2}

= \sqrt{\frac

Unknown macro: {g}

{L_

Unknown macro: {rm 2}

}} ]\end

Along the plane lying in the page, where the mass moves left and right, the pendulum length is the shorter L1 and the angular frequency is

Unknown macro: {latex}

\begin

Unknown macro: {large}

[ \omega_

Unknown macro: {1}

= \sqrt{\frac

Unknown macro: {g}

{L_

Unknown macro: {rm 1}

}} ]\end

the ratio of frequencies is thus:

Unknown macro: {latex}

\begin

Unknown macro: {large}

[ \frac{\omega_{2}}{\omega_{1}}= \frac{\sqrt{\frac

Unknown macro: {g}

{L_{2}}}}{\sqrt{\frac

{L_{1}}}} = \sqrt{\frac{L_{1}}{L_

Unknown macro: {2}

}} ]\end

in order to have a ratio of 1:2, one thus needs pendulum lengths of ratio 1:4. In order to get a ratio of 3:4 (as in the figure at the top of the page), the lengths must be in the ration 9:16.

Error formatting macro: live-template: java.lang.NullPointerException
  • No labels