Newton's Laws of Motion and Gravitation 41
Recall that a force F acting on the point mass m has a torque, or
moment, about O equal to
T 0 = rxF.
Applying the rule (1.3.6), page 26, to formula (2.1.4) we find
dLQ
(2.1.5)
dt
m(rxr + rxr) = mrxf.
If the frame O is inertial, then r — F/m and
dLc
dt
= r x F = T 0. (2.1.6)
Relation (2.1.6) describes the rotational motion just as (2.1.3) describes the
translational motion.
As an example, consider the SIMPLE RIGID PENDULUM, which is a
massless thin rigid rod of length £ connected to a point mass m at one
end. The other end of the rod is connected to a frictionless pin-joint at a
point O, which is a zero-diameter bearing that permits rotation in a fixed
plane. We select a cartesian coordinate system (i, j, K) with center at O
and i, j fixed in the plane of the rotation (Figure 2.1.1), and assume that
the corresponding frame is inertial.
Fig. 2.1.1 Simple Rigid Pendulum
The motion of m is a circular rotation in the (i, j) plane, and is best
described using polar coordinates (r,6); see page 35. The rigidity as-
sumption implies r(t) = £ for all t. Denote by 0 = 6{t) the angle from
% to the rod at time t. Let r(t) be the position vector of the point
mass in the frame O. Then r(t) = £r(0(t)), and by (1.3.24) on page 35,
r — £80. Hence, the angular momentum of the point mass about O is