Rigid Body: an Introduction
General
For the dynamical problem of
the motion of a rigid body (one that does not bend or vibrate), we need six
coordinates: three for the position
(usually the position of the center of mass), and three for the orientation. We have two vector equations (and hence six
scalar equations) to use:
SF
= MR’’
= dp/dt where p = MV,
and V = R’
Sti
= dL/dt where
ti = ri ´ F, and L = S(ri ´ mivi)
where the t may depend on both the position and orientation; and
where, if the body is free, the torque and angular momentum are measured about
the center of mass; and if the body is constrained to be at point Q, the torque
and angular momentum are measured about that point, Q.
For the orientation, we have
no simple set of coordinates that are symmetric. The set (θx, θy,
and θz) does not specify a unique orientation because the final
orientation depends on which of the angles you rotate through first. For instance, if you take an object and
rotate it first about the x axis by 90o degrees, and then about the
y axis by 90o degrees, the final orientation is in a different
orientation than if you rotate first about the y axis by 90o and
then about the x by 90o.
Rotation about an axis
In the case of a rotation
about a specified axis, we need only one coordinate to specify the
orientation. In this case, it is usually
easiest to use cylindrical coordinates (s, θ, z), and use the z axis as the specified axis of rotation. [Note that here I use s instead of r as I did earlier, since now r will be used for
density.] Please keep in mind that the s
coordinate is the distance from the z-axis, not the distance from the
origin. The r vector is from the origin. In this case, then
L = S (ri
´
mi
vi) = Lzz ,
where the component of vi
that is perpendicular to the radial and to the z directions is vqi = siq’, so
Lz = Smivqisi = Smisi2θ’
= (Smisi2) θ’ = Izθ’
,
where
Iz = (Smisi2) = òòòr s2
dV
,
since θ’ = dθ/dt is
the same for all mi, where r is the mass density, and dV = ds (sdθ) dz in cylindrical form.
It is sometimes useful to
define a radius of gyration, kz, as Mkz2 = Iz
, so kz = [Iz/M]½ .
The torque equation in this
case is:
Stz = dLz/dt
= Izθ’’ .
We can also define a
potential energy, V(θ), based on the torque just like we defined a V(r) based on the force: Work = ∫ F· dl = ∫
Fq sdq = ∫ t(θ) dθ :
V(θ) = - θi∫θf
t(θ)
dθ and the inverse: tz(θ) =
-dV(θ)/dθ .
The kinetic energy in the
rotations in this case is:
KE = S½mivθi2 = ½Smi(siθi’)2 = ½(Smi si2) θ’2 = ½Izθ’2 .
Note also that Power = rate
of using energy, so P = dW/dt = d[ ∫ F· dl ]/dt = F· v and P = dW/dt = d[ ∫ t · dq ]/dt = t · w .
Homework Problem #29: Find the steady state motion of a propeller
with moment of inertia, I, that has an applied torque, ta
= to[1
+ a*cos(wat)]
and a frictional torque due to air resistance of tf
= -bw
where to,
a, wa,
and b are constants.
Homework Problem #30: The balance wheel of a watch consists of a
ring of mass, M, and radius, R, with spokes of negligible mass. The hairspring exerts a restoring torque, ths
= -kq. Find q(t) if
initially q(t=0)
= qo
and w(t=0)
= 0.