Chapter 9: Problem 4
A pendulum consists of a light rigid rod of length \(250 \mathrm{~mm}\), with two identical uniform solid spheres of radius \(50 \mathrm{~mm}\) attached one on either side of its lower end. Find the period of small oscillations (a) perpendicular to the line of centres, and (b) along it.
Short Answer
Expert verified
Answer: (a) The period of small oscillations perpendicular to the line of centers is approximately 1.14 seconds. (b) The period of small oscillations along the line of centers is approximately 2.16 seconds.
Step by step solution
01
Determine the moments of inertia
First, we need to find the moments of inertia for both situations. We will denote the length of the pendulum rod as L, the radius of the spheres as R, and the mass of each sphere as m.
For situation (a), oscillation perpendicular to the line of centers:
We can consider the moment of inertia of the rod to be negligible because its mass is much less than the mass of each sphere. So, we will only calculate the moment of inertia of the two spheres. In this situation, each sphere rotates about an axis parallel to the rod passing through its center. The moment of inertia for one sphere (I_sphere) can be calculated as:
\(I_{sphere} = \frac{2}{5}mR^2\)
Since both spheres are identical, the total moment of inertia (I_perp) is the sum of the individual moments:
\(I_{perp} = 2 \times \frac{2}{5}mR^2 = \frac{4}{5}mR^2\)
For situation (b), oscillation along the line of centers:
In this case, the axis of rotation is the same as the line of centers, passing through the end of the rod and the center of one sphere. The moment of inertia (I_along) can be calculated using the parallel axis theorem:
\(I_{along} = I_{cm} + md^2\)
In this situation, d = L + R for one sphere, and d = L - R for the other sphere. Let´s calculate the moment of inertia for each sphere separately, and then add them together:
One sphere has moment of inertia: \(I_1 = \frac{2}{5}mR^2 + m(L + R)^2\)
The other sphere has moment of inertia: \(I_2 = \frac{2}{5}mR^2 + m(L - R)^2\)
\(I_{along} = I_1 + I_2\)
02
Use the formula for the period of oscillation
Now, we will use the formula for the period of oscillation for a physical pendulum:
\(T = 2\pi \sqrt{\frac{I}{mgr}}\)
where T is the period, I is the moment of inertia, m is the mass of the pendulum, g is the acceleration due to gravity, and r is the distance from the pivot point to the center of mass.
For situation (a), the distance r is equal to the length of the rod (L), and for situation (b), the distance r is L + R for one sphere, and L - R for the other sphere.
03
Calculate periods of oscillation
Now we can plug the values of I and r into the formula for each situation:
(a) For oscillation perpendicular to the line of centers, the period T_perp is:
\(T_{perp} = 2\pi \sqrt{\frac{I_{perp}}{mgr}} = 2\pi \sqrt{\frac{\frac{4}{5}mR^2}{mgL}}\)
Simplify:
\(T_{perp} = 2\pi \sqrt{\frac{4R^2}{5L}}\)
Using the given values for L and R:
\(T_{perp} = 2\pi \sqrt{\frac{4(50 \mathrm{~mm})^2}{5(250 \mathrm{~mm})}}\)
\(T_{perp} \approx 1.14\ s\)
(b) For oscillation along the line of centers, we calculate the period T_along:
\(T_{along} = 2\pi \sqrt{\frac{I_{along}}{mgr}} = 2\pi \sqrt{\frac{I_1 + I_2}{mg(L+R) + mg(L-R)}}\)
Simplify and plug in the values for L and R:
\(T_{along} = 2\pi \sqrt{\frac{(\frac{2}{5}mR^2 + m(L + R)^2) + (\frac{2}{5}mR^2 + m(L - R)^2)}{mg(2L)}}\)
\(T_{along} = 2\pi \sqrt{\frac{(\frac{2}{5}(50 \mathrm{~mm})^2 + (250 \mathrm{~mm} + 50 \mathrm{~mm})^2) + (\frac{2}{5}(50 \mathrm{~mm})^2 + (250 \mathrm{~mm} - 50 \mathrm{~mm})^2)}{(2)(250 \mathrm{~mm})}}\)
\(T_{along} \approx 2.16\ s\)
Thus, the period of small oscillations (a) perpendicular to the line of centers is approximately 1.14 seconds, and (b) along the line of centers is approximately 2.16 seconds.
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Moments of Inertia
In understanding the movement of a pendulum, the concept of the moment of inertia is fundamental. It's a property that quantifies how difficult it is to change an object's rotation. For solid objects like spheres, the moment of inertia depends on both its mass and how that mass is distributed relative to the axis of rotation.
For a single uniform solid sphere, the inertia is given by the formula:
\[\begin{equation} I_{sphere} = \frac{2}{5}mR^2 \end{equation}\] Here, m is the mass of the sphere, and R is its radius. The fraction \(\frac{2}{5}\) comes from the integral calculus that considers the mass distribution of a solid sphere. For most everyday solid objects, these constants have been calculated and can be simply looked up or remembered for use.
In the given exercise, we're looking at two spheres attached to a rod. Assuming the rod's mass is negligible, the pendulum's total moment of inertia when oscillating perpendicular to the line of centers is simply twice the moment for one sphere because both spheres contribute equally to the pendulum's inertia.
For a single uniform solid sphere, the inertia is given by the formula:
\[\begin{equation} I_{sphere} = \frac{2}{5}mR^2 \end{equation}\] Here, m is the mass of the sphere, and R is its radius. The fraction \(\frac{2}{5}\) comes from the integral calculus that considers the mass distribution of a solid sphere. For most everyday solid objects, these constants have been calculated and can be simply looked up or remembered for use.
In the given exercise, we're looking at two spheres attached to a rod. Assuming the rod's mass is negligible, the pendulum's total moment of inertia when oscillating perpendicular to the line of centers is simply twice the moment for one sphere because both spheres contribute equally to the pendulum's inertia.
Parallel Axis Theorem
To solve for the pendulum's period when oscillating in a different orientation, we must invoke the parallel axis theorem. This theorem states that the moment of inertia of a body about any axis parallel to an axis through its center of mass can be found by adding the moment of inertia of the body about the center of mass axis plus the product of the mass and the square of the distance between the two axes.
The general formula is:\[\begin{equation} I = I_{cm} + md^2 \end{equation}\]Here, I is the moment of inertia about the new axis, I_{cm} is the moment of inertia about the center of mass axis, m is the mass of the object, and d is the perpendicular distance between the two axes. This tool is crucial when solving for the pendulum swinging along the line of centers, as the axis of rotation does not pass through the center of mass of both spheres. The exercise demonstrates how to apply this theorem to find the separate moments of inertia for the two spheres positioned at different distances from the pivot point.
The general formula is:\[\begin{equation} I = I_{cm} + md^2 \end{equation}\]Here, I is the moment of inertia about the new axis, I_{cm} is the moment of inertia about the center of mass axis, m is the mass of the object, and d is the perpendicular distance between the two axes. This tool is crucial when solving for the pendulum swinging along the line of centers, as the axis of rotation does not pass through the center of mass of both spheres. The exercise demonstrates how to apply this theorem to find the separate moments of inertia for the two spheres positioned at different distances from the pivot point.
Physical Pendulum
When we talk about a physical pendulum, we are referring to any real-life object that can swing back and forth under the force of gravity, pivoted at a point that is not its center of mass. The period of oscillation for a physical pendulum is determined by its moment of inertia, the mass of the pendulum, the acceleration due to gravity, and the distance from the pivot point to the pendulum's center of mass.
The formula for the period of a physical pendulum is:\[\begin{equation} T = 2\pi \sqrt{\frac{I}{mgr}} \end{equation}\]In this formula, T is the period, I is the moment of inertia, m is the mass, g is the acceleration due to gravity, and r is the distance from the pivot to the center of mass. This equation is derived from the rotational form of Newton's second law. By understanding how the period depends on these variables, students can solve complex problems involving physical pendulums, such as the given exercise, where calculating the periods for different orientations of oscillation is required.
The formula for the period of a physical pendulum is:\[\begin{equation} T = 2\pi \sqrt{\frac{I}{mgr}} \end{equation}\]In this formula, T is the period, I is the moment of inertia, m is the mass, g is the acceleration due to gravity, and r is the distance from the pivot to the center of mass. This equation is derived from the rotational form of Newton's second law. By understanding how the period depends on these variables, students can solve complex problems involving physical pendulums, such as the given exercise, where calculating the periods for different orientations of oscillation is required.