130 3 Lagrange’s Equation of Motion
If we define the matrices v
c
= [ ˙x
c
, ˙y
c
, ˙z
c
]
T
, ω = [ω
x
, ω
y
, ω
z
]
T
, and
the inertia matrix
I
c
=
I
xx
I
xy
I
xz
I
xy
I
yy
I
yz
I
xz
I
yz
I
zz
(g)
then, the kinetic coenergy, (equation (f)), becomes
T
∗
=
1
2
mv
T
c
v
c
+
1
2
ω
T
I
c
ω. (3.12)
The first term in equation (3.12) is due to the translation of the body while
the second term is due to the rotation of the body. Recall that v
c
is the
velocity of the center of mass with respect to the fixed coordinate system,
and ω is the angular velocity of the x
1
-y
1
-z
1
coordinate system that is fixed
to the body. It must be emphasized however, that the components of ω are
directed along the x
1
-axis, y
1
-axis, and z
1
-axis not the x-axis, y-axis, and
z-axis.
For any rigid body we can find an orientation of the x
1
-y
1
-z
1
coordinate
system such that the products of inertia vanish, i.e., I
xy
= I
xz
= I
yz
= 0. In
such orientations the x
1
-y
1
-z
1
axes are called the Principal Axes of Inertia,
and the inertia matrix, I
c
becomes diagonal.
Kinetic coenergy with respect to a fixed point
If the point Q
1
is a fixed point then,
˙
¯
R = 0, and the kinetic coenergy given
by equation (3.11) becomes,
T
∗
=
1
2
¯ω ·
"
N
X
i=1
m
i
¯ρ
i
× (¯ω × ¯ρ
i
)
#
,
=
1
2
ω
T
I
Q
1
ω. (3.13)
where ω = [ω
x
, ω
y
, ω
z
]
T
, and the inertia matrix, I
Q
1
, is computed with
respect to the fixed point Q
1
.
Plane motion of a rigid body
If the body is constrained to move in the x-y plane then the kinetic coenergy
given in equation (3.12) becomes
T
∗
=
1
2
m( ˙x
2
c
+ ˙y
2
c
) +
1
2
I
zz
ω
2
z
, (3.14)
where the moment of inertia, I
zz
, is computed relative to the center of mass.
If the body is constrained to rotate in the x-y plane, about a fixed point
then the kinetic coenergy given in equation (3.13) becomes