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The Center of Mass
Systems of Particles
Now let's come up with a mathematical definition for center of mass which is more precise than just saying it's the balance point (although the balance point always gives the correct answer). The location of the center of mass is defined as
(1.1)
where the sum over i running from 1 to n means sum over all of the point particles within the body, assuming there are a total of n point particles. M is the total mass of all the individual bodies and can be written
(1.2)
We have defined the center of mass. Now let's see if our definition makes sense. First of all it's a vector equation and so what it really means is the usual 3-dimensional decomposition as
(1.3)
(1.4)
(1.5)
Let's just consider the 1-dimensional version for the case of 2 bodies only. Then the total mass M becomes
(1.6)
and (1.2) becomes
(7.7)
Does this make sense ? Let's see.
Example Where is the position of the center of mass for a system consisting of two dumbells, each with the same mass m each at the end of a 4ft massless rod ?
Solution Now you know that the answer to this must be at the center of the rod. After all that is the balancing point. That is our guess is that xcm = 2ft. Let's use our definition of center of mass, equation (1.1) and see if it gives this answer. Now we have a 1-dimensional problem and therefore (1.1) reduces to only (1.3). Furthermore we only have two bodies and this reduces further to (1.7). Choosing the origin of the x-coordinate system to be at the left dumbell gives x1 = 0ft and x2 = 4ft. Substituting gives
(1.8)
which is exactly what we expected. Therefore we can believe that our definition for center of mass (1.1) makes perfect sense. Let's look at what happens if we use a different coordinate system.
Example Repeat the previous problem, but with the x-origin located at the center between the two dumbells instead of on the left dumbell.
Solution Well now we would guess that the center of mass would be given by xcm = 0. Let's see if our formula works here. With the origin of the x-axis chosen to be at the center of the dumbells we have the position of each dumbell given by x1 = -2ft and x2 = +2ft respectively. Subsituting we get
(1.9)
which is exactly what we expected. Therefore again we can believe that our definition for center of mass (1.1) makes perfect sense. Being able to find the center of mass is actually useful, as the following example shows.
Example A baby of mass mB sits on a see-saw. Mary's mass is mM. Where should Mary sit in order to balance the see-saw ? Work out a formula and also a numerical answer if mB = 10 kg and mM = 80 kg.
Solution Again our intuition tells us that we can guess that the ratio of the distances should be 1/8. That is the baby should be 8 times as far away from the center of the see-saw as Mary. Let's see if our center of mass definition (1.1) tells us this. Again this is a 1-dimensional, 2-body problem and so the formula for the center of mass is again
Now we want the center of mass located at the center of the see-saw and we will put the origin of our x-axis there as well.
Thus
giving
which means that
or
or
Putting in numbers we get
just as we suspected.
Rigid Bodies
Above we considered finding the center of mass of two bodies. This can easily be extended to 3 or more bodies and some of this will be explored in the homework. That's all well and good, but how do we find the center of mass of systems made up of millions of particles such as a baseball bat. In other words how do we find the center of mass of rigid bodies ? That's what we will look at now. In physics whenever we want to change our study from a collection of discrete particles (desribed by a sum Σi) to a continuous collection of particles, the sum just changes to an integral. Hopefully this makes perfect sense from what you have studied in calculus. You all now know that an integral is just the limit of a sequence of sums. Now each of the millions of particles in a rigid body has a tiny little mass denoted by dm. For a discrete collection of particles we had (1.1) as
(1.10)
but for a continuous distribution of particles we now define
(1.11)
This is easier to work with if we introduce density as mass / volume or
(1.12)
where dV is the volume occupied by the mass dm. Thus our definition can be written
and the same for y and z. If the density is constant, then it can be taken outside the integral to give
and the same for y and z. There's one additional catch. Above we defined a 3-dimensional density as mass / volume. But what if we have a dense 1-dimensional object such as a very long and thin pencil. Well then we will want a linear mass density. Instead of