Why is there are precession frequency here?

In summary, the precession frequency refers to the rate at which an object's rotational axis moves around another axis due to external torques or forces. This phenomenon is observed in various systems, such as spinning tops, gyroscopes, and celestial bodies, where gravitational interactions lead to changes in orientation over time. Understanding precession frequency is crucial for applications in navigation, astronomy, and physics, as it helps explain the stability and behavior of rotating systems under external influences.
  • #1
simphys
324
46
Homework Statement
A child's toy top consists of a uniform thin disk of radius 5.0 cm and mass
0.15 kg with a thin spike passing through its center. The lower part of the
spike protrudes 6.0 cm from the disk. If you stand this top on a table and start
it spinning at 200 rev/s, what will be its precession frequency?
Relevant Equations
.
so I need to use the eq.: omega_pr = ##mgr / L_s## with r = 6cm.
But from how I imagine/see it, the rod pierces the disk through the middle so how does this create precession if the weight will not cause a torque then and thus a hortizontal change in angular momentum?

Thanks in advance!
 
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  • #2
What if the axis of rotation is slightly tipped when the toy is started spinning? What if the surface on which it is spinning is not exactly flat? You get the point.
 

FAQ: Why is there are precession frequency here?

What is precession frequency?

Precession frequency refers to the rate at which the axis of a rotating object wobbles or processes around another axis due to an external torque. This phenomenon is often observed in gyroscopes, spinning tops, and astronomical bodies such as the Earth.

Why does precession occur in rotating objects?

Precession occurs because of the application of an external torque that is not aligned with the object's primary rotational axis. This torque changes the direction of the angular momentum vector, causing the axis of rotation to trace out a conical shape over time.

How is precession frequency calculated?

The precession frequency can be calculated using the formula ω_p = (τ / L), where ω_p is the precession angular frequency, τ is the external torque, and L is the angular momentum of the rotating object. In the case of a gyroscope, this can also be expressed as ω_p = (mgr) / (Iω), where m is the mass, g is the acceleration due to gravity, r is the distance from the pivot point to the center of mass, I is the moment of inertia, and ω is the angular velocity.

What factors affect the precession frequency?

Several factors affect the precession frequency, including the magnitude of the external torque, the angular momentum of the rotating object, the distribution of mass (moment of inertia), and the angular velocity. Changes in any of these parameters can alter the precession frequency.

Why is understanding precession frequency important in astronomy?

Understanding precession frequency is crucial in astronomy because it helps explain the behavior of celestial bodies. For example, the precession of the Earth's axis affects the orientation of the planet over long periods, influencing climate patterns and the position of stars in the sky. It also plays a role in the stability of satellite orbits and the dynamics of planetary systems.

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