# 4.2: Center of Mass

- Page ID
- 18401

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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)## Systems with Multiple Particles

When we studied the work-energy theorem, we found that the main advantage to this approach was the nice "shortcut" available to us when we selected a system large enough that the energy within the system was conserved. So it is with the impulse-momentum theorem. We will therefore largely set aside cases where the system has an external impulse acting on it, and focus only on systems that conserve momentum.

In many cases we have dealt with so far, our "system" has been only a single object, or perhaps two objects, where one of them (i.e. the earth) is so large that we can ignore it because it basically just sits there as it provides a potential energy that affects the motion the other object. But now we will embrace multiple *active* objects, meaning that their masses will not be so different that one object's motion can be ignored. Now we will need to account for the motions of all objects within the defined system. Note that we make no claims at this point about the relative interactions of these objects – they may be securely attached to each other in a rigid embrace (a solid object), or they may be totally free to move independently of one another (a volume of gas).

Consider the impulse-momentum theorem for a system consisting of several objects. The momentum part of this theorem consists of two pieces: The mass, which we presume is the sum of the masses of all the objects within the system; and the velocity of the center of mass of the system. We have a pretty intuitive notion of center of mass for a single object, but how do we talk about the center of mass of a system with many separate moving objects? We take some time away from our discussion of momentum conservation to address this.

## Center of Mass (of a Collection of Particles)

In some sense, one can think about the center of mass of a single object as its "average position." Let's consider the simplest case of an "object" consisting of two tiny particles separated along the \(x\)-axis, as in Figure 4.2.1.

**Figure 4.2.1 – Center of Mass for Two Point-Particles**

If the two particles have equal mass, then it's pretty clear that the "average position" of the two-particle system is halfway between them.

Alert

*Center of mass is a mathematical construct, not an actual position that resides on a physical object. The center of mass of a system often lands at a position consisting of empty space, whether that is because the system consists of multiple objects, or because the single object in the system is bent or has a hole in it.*

If the masses of the two particles are different, would the "average position" still be halfway between them? Perhaps in some sense this is true, but we are not looking for a *geometric center*, we are looking for the average placement of mass. If \(m_1\) has twice the mass of \(m_2\), then when it comes to the average placement of mass, \(m_1\) gets "two votes." With more of the mass concentrated at the position \(x_1\) than at \(x_2\), the center of mass should be closer to \(x_1\) than \(x_2\). We achieve the perfect balance by "weighting" (no pun intended) the positions by the fraction of the total mass that is located there. Accordingly, we define as the center of mass:

If there are more than two particles, we simply add all of them into the sum in the numerator. To extend this definition of center of mass into three dimensions, we simply need to do the same things in the \(y\) and \(z\) directions. A position vector for the center of mass of a system of many particles would then be:

## Center of Mass (of a Collection of Objects)

Suppose now we want to know the center of mass of multiple extended objects, where all the heavy-lifting has already been done – the centers of mass of the objects are already known (see below for how to do this heavy-lifting). How do we determine the center of mass of such a system? It turns out to be pretty easy when you know the locations of the centers of mass of the two objects – just treat them as if they are point particles with all of their mass concentrated at their own centers of mass, and then do the calculation above.

__Figure 4.2.2 __**– Center of Mass for Two extended objects**

For proof of this, let's treat two extended objects (A and B) as collections of lots of point particles (atoms, if you like), and write down their centers of mass (measured from a common origin) in terms of the masses and positions of their atoms.

\[ \left. \begin{array}{l} \overrightarrow r_{cm\;A} = \dfrac{m_{1A} \overrightarrow r_{1A} + m_{2A} \overrightarrow r_{2A} + \dots}{M_A} \\ \overrightarrow r_{cm\;B} = \dfrac{m_{1B} \overrightarrow r_{1B} + m_{2B} \overrightarrow r_{2B} + \dots}{M_B} \end{array} \right\} \;\;\; \iff \;\;\; \overrightarrow r_{cm} = \dfrac{M_A \overrightarrow r_{cm\;A} + M_B \overrightarrow r_{cm\;B}}{M_A + M_B} \]

The left-hand side equations are those of the center of mass for each object in terms of its atoms' masses and positions. The right-hand side gives the center of mass of the two-object system in terms of the masses of the objects and the positions of their individual centers of mass. When the expressions for \( \overrightarrow r_{cm\;A}\) and \( \overrightarrow r_{cm\;B}\) from the left side are plugged into the right-hand side equation, then all the atoms of both objects are come together into a single center of mass formula, as if they were part of a single system with total mass \(M_A + M_B\), proving the contention above.

Example \(\PageIndex{1}\)

*Two thin circular disks made from the same material lie flat on a horizontal surface, with their outer edges in contact with each other. One disk has a larger radius (\(R\)) than the other (\(r\)), and have equal thicknesses. Find how far the center of mass of the two-disk system lies from the center of the larger disk.*

**Solution**-
*The disks are made from the same uniform material, so they have equal mass densities. That means that the mass of the larger disk is larger than that of the smaller disk by the same factor as the ratio of their areas. That is, if the larger disk has twice the area of the smaller one, then it has twice as much mass. We therefore have the following relationship between the masses and radii of the disks:**\[ \dfrac{M}{m} = \dfrac{\pi R^2}{\pi r^2} \;\;\; \Rightarrow \;\;\; M=\dfrac{R^2}{r^2}\;m \nonumber \]**Let's choose the center of the larger disk as the origin, and have the center of the other disk lie on the \(+x\)-axis. The disks are uniform, so their individual centers of mass lie at their geometric centers, and we can compute the center of mass of the system by treating the disks as point masses located at these centers. The distance of the center of mass from the origin is what we are looking for, so:**\[ x_{cm} = \dfrac{M x_1 + m x_2}{M+m} = \dfrac{M \left(0\right) + m \left(R+r\right)}{M+m} = \dfrac{m \left(R+r\right)}{\dfrac{R^2}{r^2}m+m}=\boxed{\dfrac{\left(R+r\right)r^2}{R^2+r^2}} \nonumber \]**We can double-check this answer by looking at an obvious special case: \(R=r\). If the disks are identical, then the center of mass must be halfway between their centers, which is the point where they are in contact, a distance \(R\) from the center of the larger disk. Plugging in \(R\) for \(r\) indeed gives this answer.*

## Center of Mass (of Continuous Objects)

We now turn to the problem of computing the position of the center of mass of an object whose distribution of mass is known. What follows is pure math, but it is important math that returns over and over in physics.

Alert

*The important thing to gain from this discussion is to understand how the set-up process works. It culminates in an integral, but performing the integral is mere busywork compared to the task of setting it up. It's easy to be overwhelmed by the thought of the integral that is being constructed, but if you understand each step that leads up to it (and don't try to just jump to an answer that looks like something you have seen before), it will go fine.*

We will keep this simple by restricting ourselves to objects for which the position of the center of mass in two of the three dimensions is obvious, which means we don't need to concern ourselves with the whole vector described in Equation 4.2.2 – just the \(x\)-component will do. A good model for this is a simple thin, cylindrical rod. This rod's mass distribution is completely cylindrically symmetric, which means that the center of mass lies on the axis passing through its center. But the mass distribution as a function of position on this axis may not be uniform. For example, it may be more dense on one end than on the other. Put another way, the particles located within the rod may be packed together more tightly in one region of the rod than in another, which means that the center of mass will not necessarily lie at the point halfway between the ends.

We need to say a few words about *mass density* before we proceed. Density is a measure of how closely-packed in space a quantity of something is. This quantity can be many different things. Here we will be considering mass, but in later physics classes you will deal with density of electric charge (and even, bizarrely, probability!). A *uniform density* for a region in space means that the quantity (whatever it happens to be) is evenly-distributed everywhere within that region. The way we define an average density for a region in space is to add up how much "stuff" is there, and then divide it by the total space it occupies. This gives an average density, but of course densities can vary from one point in space to another, in which case a *density function* is defined. We will deal with only the simplest variable densities here. As we will mainly be looking at thin rods for our examples, we will only consider densities that might vary along the length of the rod – this simplifies the process to a single dimension.

The mass density function in this case is a function of a single variable, has units of \(kg/m\), and is called a *linear mass density*. This mass density function is typically denoted as \(\lambda\left(x\right)\). If it is uniform, then the function is a constant \(\lambda\), and the amount of mass \(m\) within a given length \(l\) is simply given by:

If the density is not uniform, then it is only a constant over an infinitesimal length \(dx\), so Equation 4.2.4 can only apply to a tiny piece of mass \(dm\), and the relationship is different at every position \(x\) because the density is different at every position:

\[ dm = \lambda \left(x\right) dx \]

Now that we can write down how much mass is at every position, we are ready to do our calculation. We begin by drawing a diagram with the rod in a coordinate system along the \(x\)-axis such that one end is at the origin and the other is at \(x=L\). Figure 4.2.3 provides a fully-labeled diagram that is very helpful for solving such problems.