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# Centre of mass formula list with solved examples and problems

This article contains a list of the center of mass formulas along with some center of mass problems and examples.

## Center of mass formula list

1. For a system of N particles,the position vector of center of mass is $\vec{R}_{CM}=\frac{m_1\vec{r}_1+m_2\vec{r}_2+………..+m_N\vec{r}_N}{m_1+m_2+…..+m_N}=\frac{\sum_{i=1}^N{m_i\vec{r}_i}}{M}$
2. The position vector of the center of mass of a two-particle system is $\vec{R}_{CM}=\frac{m_1\vec{r}_1+m_2\vec{r}_2}{m_1+m_2}$
3. The Cartesian coordinates of the center of mass are given by $X_{CM}=\frac{m_1x_1+m_1x_2+………..+m_Nx_N}{m_1+m_2+…..+m_N}=\frac{\sum_{i=1}^N{m_ix_i}}{M}$ $Y_{CM}=\frac{m_1y_1+m_1y_2+………..+m_Ny_N}{m_1+m_2+…..+m_N}=\frac{\sum_{i=1}^N{m_iy_i}}{M}$ $Z_{CM}=\frac{m_1z_1+m_1z_2+………..+m_Nz_N}{m_1+m_2+…..+m_N}=\frac{\sum_{i=1}^N{m_iz_i}}{M}$
4. For Continuous mass distribution $\vec{R}_{CM}=\frac{1}{M}\int{\vec{r}dm}$
where dm is the mass element located at position \vec{r}. Also $X_{CM}=\frac{1}{M}\int{xdm}$ $Y_{CM}=\frac{1}{M}\int{ydm}$ $Z_{CM}=\frac{1}{M}\int{zdm}$
5. Velocity of center of mass of a two particle system is $\vec{v}_{CM}=\frac{m_1\vec{v}_1+m_2\vec{v}_2}{m_1+m_2}$

## The motion of Center of mass examples

A few of the examples of motion of the center of mass are

• Binary stars:- Binary stars are two stars bound to each other by the gravitational force. Binary stars orbit around their common center of mass.
• The Earth-moon system is one such system center of mass of the Earth-Moon system moves around the Sun in an elliptical path, not the earth and moon themselves.

Scalars and Vectors in physics x
Scalars and Vectors in physics

## Center of mass Problems with solutions

Problem 1
Determine the center of mass of a hemisphere of radius $$R$$ and uniform density $$\rho$$.
Strategy:
We will divide the given hemisphere into co-axial discs and then find the relation for the center of mass of this disc using the center of mass formula for a continuous distribution of mass. We will integrate this relation for the limits $$0$$ to $$R$$ for the x-axis. From symmetry  $$Y_{CM}$$ and $$Z_{CM}$$ would be 0.
Mass of the strip can be found using the fact that density is mass per unit volume i.e. $$\rho=m/V$$
Solution
Let $$\rho$$ be the density of the material of the hemisphere. Take $$O$$ as the origin. The hemisphere can be assumed to be made up of a large number of co-axial discs as shown below in the figure.

Consider one such elementary disc of radius $$y$$ and thickness $$dx$$ at a distance $$x$$ from the origin.
$$\text{Mass of the elementary disc}= volume \times density$$ $dm=\pi y^2dx\times \rho =\pi \left( R^2-x^2 \right) dx\rho$ The coordinates of the center of mass of the hemisphere can be determined as follows $X_{CM}=\frac{1}{M}\int{xdm}$ $=\frac{1}{M}\int_0^R{x\pi \left( R^2-x^2 \right) \rho dx}$ $=\frac{\pi \rho}{M}\int_0^R{\pi \left( xR^2-x^3 \right) \rho dx}$ $=\frac{\pi \rho}{M}\left[ R^2\frac{x^2}{2}-\frac{x^4}{4} \right] _{0}^{R}$ Solving and simplifying it we get
$X_{CM}=\frac{\pi \rho}{M}\left[ \frac{R^4}{4} \right]$ Since, $M=\frac{2}{3}\pi R^3\times \rho$ for this hemisphere, thus we have $X_{CM}=\frac{\pi \rho}{\frac{2}{3}\pi R^3\rho}\left[ \frac{R^4}{4} \right]$ Simplifying it we get $X_{CM}=\frac{3}{8}R$ $$Y_{CM}=0$$ and $$Z_{CM}=0$$ because of symmetry.
Hence the coordinates of the center of mass of the hemisphere are $\left( \frac{3}{8}R,\text{0,}0 \right)$