The center of gravity of an object is the
point from which you can suspend an object at rest, and, no matter how the
object is oriented, gravity will not cause it to start rotating. If you suspend
an object from any point and let it come to rest, the center of gravity will lie
somewhere on a vertical line that passes through the point of suspension. Near
the surface of the earth, where the gravitational acceleration is (nearly)
constant, the center of gravity coincides with the center of mass.
Assume a system consist of a collection of particles, for example the atoms that make up a solid object. The mass of the ith particle is mi and its position coordinates are (xi, yi, zi). The coordinates of the center of mass (CM) are given by
xCM = Σmixi/M, yCM = Σmiyi/M, zCM = Σmizi/M.
Here M is the total mass of the system.
M = Σmi.
The ∑ symbol stand for sum. The sum is over all the particles that make up the system.
The position vector of the center of mass is rCM.
rCM = xCM
i + yCM j + zCM
k = (Σmixi i + Σmiyi
j + Σmizi k)/M
rCM = (Σmiri)/M.
Let us find its velocity and its acceleration.
vCM = drCM/dt = (Σmi dri/dt)/M
MvCM = Σmivi = Σpi = ptot.
The velocity of the center of mass multiplied by the total mass of the system is equal to the total momentum of the system.
aCM = dvCM/dt = (Σmi dvi/dt)/M
MaCM = Σmiai = ΣFi = Ftot.
The acceleration of the center of mass multiplied by the total mass of the system is equal to the total force acting on the system.
Newton's 2nd law, F = ma, when applied to an extended object, predicts the motion of a particular reference point for this object. This reference point is called the center of mass. The center of mass of a system moves as if the total mass of the system were concentrated at this special point. It responds to external forces as if the total mass of the system were concentrated at this point.
The total force on a particle, Fi, is the
sum of all internal and external forces acting on the particle. If we
sum the forces acting on all the particles of the system, then in this vector
sum every internal force that particle 1 exerts on particle 2 is cancelled by
the internal force that particle 2 exerts on particle 1. This is a consequence
of Newton's third law.
We therefore have Ftot = ∑Fi = ∑Fext.
The total force on the system is the vector sum of all the external forces.
But Ftot = MaCM = dpCM/dt.
The total momentum of the system only changes, if
external forces are acting on the system. The center of mass of the system only
accelerates, if external forces are acting on the system.
If only internal forces are acting on the particles that make up the system, then the center of mass does not accelerate, its velocity remains constant. The total linear momentum of the system is conserved.
For the total linear momentum of a system to be constant, the particles making up the system can move with respect to each other, and can accelerate with respect to each other, but they must move and accelerate in such a way that vCM = constant and therefore aCM = 0.
Every extended object has a center of mass.
If near the surface of Earth an object, in any
orientation, is supported at a location directly below its center of mass or
suspended from a location directly above its center of mass, it will be balanced
and it will not start to rotate.
Usually, but not always, the center of mass of an object lies within the object itself. For example, the center of mass of a ball is the very middle of the ball, and the center of mass of a book is the middle of the book.
If an object has parts that can move with respect to each other, the location of the center of mass depends on the positions of the parts. For example, when a cheerleader lifts her arms, her center of mass moves to a higher position in her body than when her arms are at her side.
In most men, the center of mass is located at or slightly above the navel, in most women it is located below the navel, closer to the hips.
For a homogeneous, symmetrical system, the center of mass always lies on the
Consider a square with sides of length a. We can position our coordinate system as shown.
The x and y axes are symmetry axes. We can easily verify that xCM = 0, yCM = 0 from symmetry.
The center of mass lies on the intersection of the symmetry axes, at the origin.
Four objects are situated along the y-axis as follows: a 2 kg object is at +3 m, a 3 kg object is at +2.5 m, a 2.5 kg object is at the origin, and a 4 kg object
is at -0.5 m. Where is the center of mass of these
The total mass of the system is M = (2 + 3 + 2.5 + 4) kg = 11.5 kg.
yCM = (2 kg * 3 m + 3 kg * 2.5 m + 2.5 kg * 0 m - 4 kg * 0.5 m)/(11.5 kg) = 1 m.
xCM = zCM = 0.
A uniform carpenter's square has the shape of an L, as shown in the figure. Locate the center of mass relative to the origin of the coordinate system.
We can think of the system as being made up of two subsystems, as shown in the figure.
The CM of the left subsystem lies at xCM = 2 cm, yCM = 9 cm. The CM of the right subsystem lies at xCM = 8 cm, yCM = 2 cm. If the mass of a 1 cm by 1 cm square is 1 unit, then the mass of the left subsystem is 72 units and the mass of the right subsystem is 32 units. We find the CM of the system by treating each subsystem as a separate particle, with all its mass concentrated at its center of mass. Then we have for the whole system
xCM = (72 units * 2 cm + 32 units * 8 cm)/(104 units) = 3.85 cm,
yCM = (72 units * 9 cm + 32 units * 2 cm)/(104 units) = 6.85 cm.
The CM of the system lies outside of the system. For irregular-shaped objects it is quite common for the CM to lie outside the system. This special point outside the system responds to external forces as if the total mass of the system were concentrated there.
The mass of the Moon is 7.35*1022 kg and the mass of the Earth is
6.00*1024 kg. The distance between the Moon and the Earth is 3.80*105
Choose your coordinate system so that the center of the Earth is at the origin and the center of the Moon is on the x-axis at x = 3.80*108 m. Calculate the location xcm of the center of mass of the Earth-Moon system
xcm = (0m*6.00*1024 kg + 3.80*108 m*7.35*1022 kg)/(6.00*1024 kg + 7.35*1022 kg)
= 4598666 m = 4600 km.
Since the radius of the Earth is 6378 km, the center of mass of the Earth-Moon system is inside the Earth.