Basics of Rotational Motion
1.0 Rigid body
2.0 Motion of rigid body
3.0 Kinematics of a plane motion
3.1 Angular velocity $\omega $
3.2 Angular acceleration $\left( \alpha \right)$
3.3 Kinematics equation for rotational motion
3.4 Analogy between translational motion & rotational motion
4.0 Moment of inertia
5.0 Radius of gyration $(K)$
6.0 Theorems of moment of inertia
7.0 Moment of inertia of uniform continious rigid bodies
7.1 Thin rod
7.2 Rectangular lamina
7.3 Circular ring
7.4 Circular disc
7.5 Solid cylinder
7.6 Cylindrical shell
7.7 Solid sphere
7.8 Hollow sphere
7.9 Spherical shell
7.10 Solid cone
7.11 Hollow cone
7.12 Hollow hemisphere
7.13 Parallelopiped
7.14 List of moment of inertia $(I)$ and radius of gyration $(K)$ of different bodies
7.4 Circular disc
3.2 Angular acceleration $\left( \alpha \right)$
3.3 Kinematics equation for rotational motion
3.4 Analogy between translational motion & rotational motion
7.2 Rectangular lamina
7.3 Circular ring
7.4 Circular disc
7.5 Solid cylinder
7.6 Cylindrical shell
7.7 Solid sphere
7.8 Hollow sphere
7.9 Spherical shell
7.10 Solid cone
7.11 Hollow cone
7.12 Hollow hemisphere
7.13 Parallelopiped
7.14 List of moment of inertia $(I)$ and radius of gyration $(K)$ of different bodies
Let us consider a circular disc of mass $M$ and radius $R$. Assume an axis passing through its centre of mass $(COM)$ as shown in the figure.
Mass per unit area $$\left( {{\lambda _A}} \right) = \frac{M}{{\pi {R^2}}}\quad ...(i)$$
Consider an infinitesimally small section in the shape of a ring of thickness $dr$, area $dA$, mass $dm$ and at a distance $r$ from the centre $O$ as shown in the figure. $$dA = (2\pi R)(dr)\quad ...(ii)$$
From equation $(i)$ & $(ii)$ we get, $$\begin{equation} \begin{aligned} dm = {\lambda _A}dA = \frac{M}{{\pi {R^2}}}(2\pi rdr) \\ dm = \frac{{2Mrdr}}{{{R^2}}}\quad ...(iii) \\\end{aligned} \end{equation} $$
As we know, that the moment of inertia $(I)$ of a continious rigid body is given by, $$I = \int_m {{r^2}dm} \quad ...(iv)$$
where,
$\int_m : $ Integrating over the entire mass
$r$: Perpendicular distance from an axis of rotation (Radius of the ring)
$dm$: mass of infinitesimally small section
From equation $(iii)$ & $(iv)$ we get, $$I = \int_m {{r^2}} \left( {\frac{{2Mrdr}}{{{R^2}}}} \right)$$
Integrating the above equation for the whole disc we get, $$\begin{equation} \begin{aligned} I = \frac{{2M}}{{{R^2}}}\int\limits_0^R {{r^3}dr} \\ I = \frac{{2M}}{{{R^2}}}\left[ {\frac{{{r^4}}}{4}} \right]_0^R \\ I = \frac{{2M}}{{{R^2}}}\left( {\frac{{{R^4}}}{4} - 0} \right) \\ I = \frac{{M{R^2}}}{2}\quad ...(v) \\\end{aligned} \end{equation} $$
So, moment of inertia about an axis passing through its centre of mass & perpendicular to its plane is, ${I_{COM}} = \frac{{M{R^2}}}{2}$
Radius of gyration $(K)$ is given as, $$\begin{equation} \begin{aligned} I = M{K^2} \\ \frac{{M{R^2}}}{2} = M{K^2} \\ K = \frac{R}{{\sqrt 2 }} \\\end{aligned} \end{equation} $$
So, radius of gyration about an axis passing through centre of mass is, ${K_{COM}} = \frac{R}{{\sqrt 2 }}$
Momemt of inertia about an axis along the diameter of the circular disc.
From the perpendicular axis theorem, $${I_z} = {I_x} + {I_y}\quad ...(vi)$$
As circular ring is symmetric in all direction in $x-y$ plane. So, $${I_x} = {I_y}\quad ...(vii)$$
From equation $(v),(vi)$ & $(vii)$ we get, $$\begin{equation} \begin{aligned} \frac{{M{R^2}}}{2} = 2{I_x} \\ {I_x} = \frac{{M{R^2}}}{4} \\\end{aligned} \end{equation} $$ Similarly, $${I_y} = \frac{{M{R^2}}}{4}$$
So, moment of inertia about an axis along the diameter of the circular disc is, ${I_x} = {I_y} = \frac{{M{R^2}}}{4}$
Radius of gyration $(K)$ is given by, $$\begin{equation} \begin{aligned} I = M{K^2} \\ \frac{{M{R^2}}}{4} = M{K^2} \\ K = \frac{R}{2} \\\end{aligned} \end{equation} $$
So, radius of gyration about an axis as shown in the figure is, $K = \frac{R}{2}$
For moment of inertia about the tangent perpendicular to its plane
From parallel axis theorem we get, $$\begin{equation} \begin{aligned} {I_1} = {I_z} + M{R^2} \\ {I_1} = \frac{{M{R^2}}}{2} + M{R^2}\quad \left( {As,\;{I_z} = M{R^2}} \right) \\ {I_1} = \frac{3}{2}M{R^2} \\\end{aligned} \end{equation} $$
Radius of gyration $(K)$ is given as, $$\begin{equation} \begin{aligned} I = M{K^2} \\ \frac{3}{2}M{R^2} = M{K^2} \\ K = \sqrt {\frac{3}{2}} R \\\end{aligned} \end{equation} $$
So, radius of gyration about the axis as shown in the figure is, $K = \sqrt {\frac{3}{2}} R$
For moment of inertia about the tangent in its own plane
From parallel axis theorem we get, $$\begin{equation} \begin{aligned} {I_2} = {I_x} + M{R^2} \\ {I_2} = \frac{{M{R^2}}}{4} + M{R^2} \\ {I_2} = \frac{{5M{R^2}}}{4} \\\end{aligned} \end{equation} $$
Radius of gyration $(K)$ is given as, $$\begin{equation} \begin{aligned} I = M{K^2} \\ \frac{{5M{R^2}}}{4} = M{K^2} \\ K = \sqrt {\frac{5}{4}} R \\\end{aligned} \end{equation} $$
So, radius of gyration about the axis as shown in the figure is, $K = \sqrt {\frac{5}{4}} R$