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Equations of
Motion for Rigid Bodies
We are now ready to write down the general equations of motion for
rigid bodies in terms of
for the center of mass and
for the rotation of the body about its center of mass.
As discussed above, it is useful to decompose the motion of a rigid
body into
- (1)
- the linear velocity
of its center of mass, and
- (2)
- its angular velocity
about its center of mass.
The linear motion is governed by Newton's second law
, where
is the total mass,
is the
velocity of the center-of-mass, and
is the sum of all external
forces on the rigid body. (Equivalently,
is the sum of the
radial force components pointing toward or away from the center of
mass.) Since this is so straightforward, essentially no harder than
dealing with a point mass, we will not consider it further.
The angular motion is governed the rotational version of
Newton's second law introduced in §B.4.19:
 |
(B.29) |
where
is the vector torque defined in Eq.(B.27),
is
the angular momentum,
is the mass moment of inertia tensor,
and
is the angular velocity of the rigid body about its center
of mass. Note that if the center of mass is moving, we are in a
moving coordinate system moving with the center of mass (see next
section). We may call
the intrinsic momentum of the
rigid body, i.e., that in a coordinate system moving with the center of
the mass. We will translate this to the non-moving coordinate system
in §B.4.20 below.
The driving torque
is given by the resultant moment of
the external forces, using Eq.(B.27) for each external force to
obtain its contribution to the total moment. In other words, the
external moments (tangential forces times moment arms) sum up for the
net torque just like the radial force components summed to produce the
net driving force on the center of mass.
Subsections
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