8/7/2019 Dynamics_Lecture9 [Compatibility Mode] http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 1/58 Kinetics of Rigid Bodies in Three Dimensions
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 1/58
Kinetics of Rigid Bodies inThree Dimensions
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 2/58
p_07_005
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 3/58
p_07_006
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 4/58
p_07_007
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 5/58
p_07_008
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 6/58
p_07_010
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 7/58
p_07_011
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 8/58
Introduction
• The fundamental relations developed for
the plane motion of rigid bodies may also
be applied to the general motion of three
dimensional bodies.
I H G =• The relation which was used
to determine the angular momentum of a
rigid slab is not valid for general three
GG
H M
amF
=
=
∑
∑
dimensiona bodies and motion.
• The current chapter is concerned with
evaluation of the angular momentum and
its rate of change for three dimensional
motion and application to effectiveforces, the impulse-momentum and the
work-energy principles.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 9/58
• Angular momentum of a body about its mass center,
( ) ( )[ ]∑∑==
′××′=×′=n
iiii
n
iiiiG mr r mvr H
11
∆
ω ∆
• The x component of the angular momentum,
( ) ( )[ ]∑=
′×−′×=
n
n
ii yii zii x mr zr y H
1
∆ω ω
Rigid Body Angular Momentum in Three Dimensions
( ) ∑∑∑===
=
−−+=
−−−=
n
iiii z
n
iiii y
n
iiii x
i ii xi zii yi xi
m x zm y xm z y
m z x z x y y
111
22
1
∆∆∆ ω ω ω
ω
dm zxdm xydm z y H z y x x ∫ ∫ ∫ −−+= ω ω ω 22
z xz y xy x x I I I −−+=
z z y zy x zx z
z yz y y x yx y
I I I H
I I I H
ω ω ω
ω
+−−=
−+−=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 10/58
• Transformation of into is characterized
by the inertia tensor for the body,
G H
+−−
−+−
−−+
z zy zx
yz y yx
xz xy x
I I I
I I I
I I I
• With respect to the principal axes of inertia,
′
Rigid Body Angular Momentum in Three Dimensions
z z y zy x zx z
z yz y y x yx y
z xz y xy x x x
I I I H
I I I H
I I I H
ω ω ω
ω ω ω
ω
+−−=
−+−=
−−+=
′
′
z
y
I
I
00
00
z z z y y y x x x I H I H I H ′′′′′′′′′ ===
• The angular momentum of a rigid body
and its angular velocity have the same
direction if, and only if, is directed along a
principal axis of inertia.
G H
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 11/58
• The momenta of the particles of a rigid body can
be reduced to:
vm
L
=
= momentumlinear
G H G aboutmomentumangular=
−−=
Rigid Body Angular Momentum in Three Dimensions
z z y zy x zx z
z yz y y x yx y
z z y xy x x
I I I H
I I I H
ω ω ω
ω ω ω
+−−=
−+−=
• The angular momentum about any other given
point O is
GO H vmr H
+×=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 12/58
• The angular momentum of a body constrained to
rotate about a fixed point may be calculated from
GO H vmr H
+×=
• Or, the angular momentum may be computed
directly from the moments and products of inertia
with respect to the Oxyz frame.
Rigid Body Angular Momentum in Three Dimensions
z z y zy x zx z
z yz y y x yx y
z xz y xy x x x
I I I H
I I I H
I I I H
ω ω ω
ω ω ω
ω ω ω
+−−=
−+−=
−−+=
( )
( )[ ]∑
∑
=
=
××=
×=
n
iiii
iiiO
mr r
mvr H
1
1
∆
∆
ω
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 13/58
Principle of Impulse and Momentum
• The principle of impulse and momentum can be applied directly to thethree-dimensional motion of a rigid body,
Syst Momenta1 + Syst Ext Imp1-2 = Syst Momenta2
• The free-body diagram equation is used to develop component and
moment equations.
• For bodies rotating about a fixed point, eliminate the impulse of the
reactions at O by writing equation for moments of momenta and
impulses about O.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 14/58
• Kinetic energy of particles forming rigid body,
2(
∆
∆
222
212
21
1
2
212
21
1
2
212
21
y x xy z z y y x x
n
iii
n
iii
I I I I vm
mr vm
vmvmT
ω ω ω ω ω
ω
−+++=
′×+=
′+=
∑
∑
=
=
Kinetic Energy
x z zx z y yz −−
• If the axes correspond instantaneously with the
principle axes,
)(222
212
21
z z y y x x I I I vmT ′′′′′′ +++= ω ω ω
• With these results, the principles of work and
energy and conservation of energy may be applied
to the three-dimensional motion of a rigid body.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 15/58
• Kinetic energy of a rigid body with a fixed point,
)22
2( 22221
x z zx z y yz
y x xy z z y y x x
I I
I I I I T
ω ω ω ω
ω ω ω ω ω
−−
−++=
Kinetic Energy
• e axes xyz correspon ns an aneous y w
the principle axes Ox’y’z’,
)(222
21
z z y y x x I I I T ′′′′′′ ++= ω ω ω
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 16/58
SOLUTION:
• Apply the principle of impulse and
momentum. Since the initial momenta
is zero, the system of impulses must be
equivalent to the final system of
momenta.
• Assume that the supporting cables
Problem: 1
Rectangular plate of mass m that is
suspended from two wires is hit at D in
a direction perpendicular to the plate.
Immediately after the impact,
determine a) the velocity of the mass
center G, and b) the angular velocity of
the plate.
and the rotation about an axis normal tothe plate is zero.
• Principle of impulse and momentum
yields to two equations for linear
momentum and two equations forangular momentum.
• Solve for the two horizontal components
of the linear and angular velocity
vectors.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 17/58
SOLUTION:
Problem: 1
• Apply the principle of impulse and momentum. Since the initial momenta is zero,
the system of impulses must be equivalent to the final system of momenta.
• Assume that the supporting cables remain taut such that the vertical velocity and the
rotation about an axis normal to the plate is zero.
k vivv z x
+= ji y x
+=
Since the x, y, and z axes are principal axes of inertia,
jmaimb j I i I H y x y y x xG
ω ω ω ω 2
1212
121 +=+=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 18/58
Problem: 1
• r nc p e o mpu se an momen um y e s wo equa ons or near momen um an
two equations for angular momentum.
• Solve for the two horizontal components of the linear and angular velocity vectors.
xmv=0
0=
xv
zvmt F =− ∆
mt F v z∆−=
( )k mt F v
∆−=
x
x
mb
H t bF
ω 2121
21
∆
=
=
mbt F x ∆6=
y
y
ma
H t aF
ω 2121
21
∆
=
=−
( )mat F y ∆6−=
( ) jbia
mab
t F +=
∆6ω
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 19/58
Problem: 1
( )k mt F v
∆−
( ) jbiamab
t F +=
∆6ω
jmaimb H y xG
ω ω 2
1212
121 +=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 20/58
A homogeneous disk of mass m is
SOLUTION:
• The disk rotates about the vertical axis
through O as well as about OG.
Combine the rotation components forthe angular velocity of the disk.
• Compute the angular momentum of the
Problem: 2
moun e on an ax e o neg g e
mass. The disk rotates counter-
clockwise at the rate ω 1 about OG.
Determine: a) the angular velocity of
the disk, b) its angular momentum about
O, c) its kinetic energy, and d) the
vector and couple at G equivalent to the
momenta of the particles of the disk.
noting that O is a fixed point.
• The kinetic energy is computed from the
angular velocity and moments of inertia.
• The vector and couple at G are also
computed from the angular velocity and
moments of inertia.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 21/58
SOLUTION:
• The disk rotates about the vertical axis through O as well
as about OG. Combine the rotation components for the
angular velocity of the disk.
ji
21 ω ω ω +=
Noting that the velocity at C is zero,
==
Problem: 2
( ) ( )( )
Lr
k r L
jr i L ji
12
12
210
ω ω
ω ω
ω ω
=
−=
−×+=
( ) j Lr i
11−=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 22/58
• Compute the angular momentum of the disk using
principle axes of inertia and noting that O is a fixed point.
−
k I j I i I H z z y y x xO
ω ω ω ++=
( )( )
( ) 00212
12
412
1221
=+==
−+==
==
mr mL I H
Lr mr mL I H
mr I H
z z z
y y y
x x x
ω
ω ω
ω ω
Problem: 2
11
( ) j Lr r Lmimr H O
1241212
21 ω ω +−=
• The kinetic energy is computed from the angular velocity
and moments of inertia.
( )( )[ ]21
2
4122
12
21
22221
Lr r Lmmr
I I I T z z y y x x
ω ω
ω ω ω
−++=
++=
212
22
81 6 ω
+=
L
r mr T
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 23/58
( ) j Lr i
11 −=
• The vector and couple at G are also computed from the
angular velocity and moments of inertia.
k mr vm
1ω =
( ) j Lr mr imr
k I j I i I H z z y y x xG
ω ω
ω ω ω
−+=
++= ′′′
2
41
12
21
r
Problem: 2
−= j
L
imr H G2
12
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 24/58
The electric motor with an attached disk is running at a constant low speed of 120 rev/min
. .
assembly is next set is rotation about the vertical Z-axis at the constant rate N = 60rev/min with a fixed angle γ of 300. Determine (a) the angular velocity and angular
acceleration of the disk, (b) the velocity and acceleration of point A at the top of the disk
for the instant shwon.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 25/58
A thin homogeneous square plate of mass ‘m’ and side ‘a’ is
welded to a vertical shaft AB with which it forms s an angle
of 45°. Knowing that the shaft rotates with a constant angularvelocity ω, determine the angular momentum HA of the plate
about point A.
Y’
Y
Y’Z’ 45°
Y’Z’ as principal axes
ω ’ = ω cos 45; ω ’ = ω sin 45
R. Ganesh Narayanan 25
A X’
Z
ωx’ = 0
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 26/58
To describe the motion of an aircraft, a set of axes Gxyz, fixed to the
aircraft is defined. In level flight Gx is forward, Gz is downward and Gxz is
the vertical plane of symmetry; G is the centre of gravity of the mass. The
moments of inertia of the aircraft about these axes are:
Kgm 400= Kgm 12000= Kgm 8000= Kgm2
xz
2
zz2
yy
2
I I I 4000= I xx
The aircraft flies at 400m/s toward north; it then follows a curve of 12Km
30° during this change of course, find the resulting inertia torques.
Answer: -1.92 Nm -0.333 Nm -0.192Nm
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 27/58
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 28/58
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 29/58
z (k )P
3
Angular Momentum (Moment of Momentum) of a rigid body
The relative angular momentum of a rigid body:
Assume a body to be rotating with angular velocity ω and consider a particle P of
mass m p positioned at r po relative to some point O so that:
po= xi + y jr + zk
and
Oy ( j )
x (i )
x
y
1ω 2ω
po
1 2 3= i + j + k ω ω ω ω
where i , j and k refer to arbitrarily chosenaxes Oxyz .
O fixed and Oxyz axes could be fixed and29
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 30/58
( ) ( ) (from (2)) p P po po poo po
= m = mh vr r r ω ∑ ∧ ∑ ∧ ∧
If we express h o in the form h = h 1 i + h 2 j + h 3 k , we find that:
( ) [ ] [ ]
[ ] ( ) [ ]
1 1 2 3
2 1 2 3
2 2P P P
2 2P P P
22
h = m + - m xy - m xz y z
h = - m yx + m + - m yz x z
ω ω ω
ω ω ω
∑ ∑ ∑
∑ ∑ ∑
3 1 2 3P P P- - x
are the Moments of inertia of the body about Oxyz and
( )2 2 xx P I m + y z= ∑ ( )2 2
yy P I m + x z= ∑ ( )22
zz P I m + y x=
∑
xy P I m xy= ∑ yz P
I m yz= ∑ zx P I m zx= ∑
are the products of inertia referred to Oxyz . 30
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 31/58
1 1 2 3
2 1 2 3
xx xy zx
yx yy yz
h = I - I - I
h = - I + I - I
h = - I - I + I
ω ω ω
ω ω ω
ω ω ω
(5)
zx yz yy
relative angular momentum of body about O relative to i , j , k
31
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 32/58
In general, if the reference axes Oxyz rotate w.r.t. the body (or vice versa) then the
products and moments of inertia will vary with time. By considering the axes to
rotate with the body the moments and products of inertia will be constant. Further,
if we choose Oxyz as principal axes of inertia then, by the definition of principal
axes, the products of inertia will be zero and the expression (5) for the relativeangular momentum simplifies to:
1 2 3 xx yy zzo= I i + I j + I k h ω ω ω (6)
Relative angular momentum
32
E i f M i
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 33/58
Equations of MotionConsider a system of n particles of which p is typical. r po defines the position of p
relative to O and v po the velocity of p relative to O . Oxyz rotates with angular
velocity and O is moving. The angular momentum of the system relative to O is:
z
z (k ) P
3Ω
povO does not necessarily coincide with thecentre of mass
Oy ( j )
x (i )
x
y
1Ω 2Ω
poOxyz rotating axes with angular
velocity
( ) ( by equation (2))n
p poo po
p=1
=h vr m ∧
∑ (7)
33
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 34/58
The forces acting on the particle may be separated into two groups: (i) due to
influences received from outside the system, called external forces F p
and (ii) due
to interaction between particles of the system, called internal forces F p .
From Newton's second law we may write, for a single particle,
( ) p p p p
d + = m vF F ′ (8)
where v p is the absolute velocity of p .
Equation (8) describes the linear motion of particle p . The corresponding equation
for the rotational motion of p about O follows from (8) by considering the moment
about O of the forces acting on the particle. Thus,
( ) p po p po p po p
d + = vr F r F r
mdt ′
∧ ∧ ∧34
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 35/58
Now, by Newton's third law is zero since it represents the
summation of the moment of equal and opposite pairs of reaction forces. Also
represents the sum of the moments about O of all the external forces. This is
the total externally applied moment, which we will denote by T o .
po p r F ′
∧∑ p po F r ∧∑
which, summing over all the particles becomes
( ) p p po po p po pd F + = vr r F r mdt
′ ∧ ∧ ∧ ∑ ∑ ∑
35
Thus
( ) po po p
d = vT r m
dt
∧
∑ (9)
Returning now to equation (7) we may write
( )o p po po
d h d = vr m
dt dt ∧ ∑
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 36/58
It can be shown that
( ) ( )o p p po po p o
d h d d = -v vr r m mdt dt dt
∧ ∧ ∑ ∑ (10)
From equation (9) it can be seen that the first term on the right hand side of
equation (9) is equal to T o . Noting also that dv o /dt = a o , the absolute acceleration
of O , equation (10) may be expressed as:
36
( )o
po po o
d h= - m aT r
dt ∧∑
where G is the centre of mass of the system of particles.
o Go o= - M aT r ∧
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 37/58
[ ])v m(r dt
d =
dt
hd po p po
o ∧∑
∧∑+
∧∑
dt
)v md( r )v m(
dt
r d =
dt
hd po p
po po p
poo
vdt
r d po
po =Thus
r d
po
dt
po p
and vvv o p po−=
∧∑
∧∑ )v m(
dt
d r -)vm(
dt
d r =
dt
hd o p po p p po
o
37
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 38/58
Thus,
( ) oo Go o
d h- M =aT r
dt ∧ (11)
In the special cases where either a o = 0 or O and G coincide (r Go = 0) equation(11) takes the form:
h+t
=dt
=T o
oo
o
∧Ω
∂
(12)
38
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 39/58
Scalar versions of the Equations of Motion
Let h o = h 1 i + h 2 j + h 3 k be defined in components along references which are rotating withangular velocity = 1 i + 2 j + 3 k .
It can be shown that (see handout) the equations of motion given by equation (12)(i.e. the special case when either a o = 0 or r Go = 0 ) may be written as:
1 1 2 3 3 2T h h h= − Ω + Ω
−
132 2 3 1 1 3
3 3 1 2 2 1T h h h= − Ω + Ω
where T 1, T 2, T 3 are the components of externally applied moment (T o ) along i , j andk respecively.
Equations (13) are referred to as the Momentum equations and have almostuniversal application in the study of gyroscopic phenomena and motion withrespect to moving axes.
39
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 40/58
In general, the components (h 1, h 2 , h 3 ) of angular momentum for a rigid body,
rotating with angular velocityω
, may be calculated from equations (5) and (6),noting that the body angular velocity must be specified in components along the
moving reference axes which, in general, are not fixed in the moving body. In
other words, and ω are not, in general, equal.
If however, in a special case the reference axes are fixed in the body alongprincipal axes, then = ω and if the principal moment of inertia along reference
axes Oxyz are A, B, C respectively, then equations (6) and (13) may be combined
to give:
( )
( )
( )
1 1 2 3
2 2 3 1
3 3 1 2
= A - B - C T
= B - C - AT
= C - A- BT
ω ω ω ω ω ω ω ω ω ω ω ω
ω ω ω ω ω ω ω ω ω ω ω ω
ω ω ω ω ω ω ω ω ω ω ω ω
(14)
Equations (14) are called the Euler dynamical Equations.
40
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 41/58
• Angular momentum and its rate of change are
taken with respect to centroidal axes GX’Y’Z’ of
fixed orientation.
• Convenient to use body fixed axes Gxyz where
moments and products of inertia are not time
• Transformation of into is independent of
the system of coordinate axes.
G H
Motion of Rigid Bodies in Three Dimensions
G H M
amF
=
=
∑
∑
dependent.
• Define rate of change of change of with
respect to the rotating frame,G H
k H j H i H H z y xGxyzG
++=
Then,
ω Ω Ω
=×+= GGxyzGG H H H
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 42/58
GGxyzGG H H M
×+=∑ Ω
• With and Gxyz chosen to correspond
to the principal axes of inertia,
ω Ω =
z y z y x x x I I I M
−−=
−−=∑
Euler’s Equations:
Euler’s Equation Motion and d’Alembert’s Principle
( ) y x y x z z z
x z z y y y
I I I M ω ω ω −−=∑
• System of external forces and effective forces
are equivalent for general three dimensional
motion.
• System of external forces are equivalent to
the vector and couple, .and G H am
M i Ab Fi d P i Fi d A i
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 43/58
• For a rigid body rotation around a fixed point,
( ) OOxyzO
OO
H H
H M
×+=
=∑
Ω
• For a rigid body rotation around a fixed axis,
z z yz y xz x I H I H I H −=−=−=
Motion About a Fixed Point or a Fixed Axis
( )( )
( ) ( ) 2ω α
ω ω
ω
i I j I k I j I i I
k I j I i I k
k I j I i I
yz xz z yz xz
z yz xz
z yz xz
OOxyzOO
+−++−−=
+−−×+
+−−=
α
ω α
ω α
z z
xz yz y
yz xz x
I M
I I M
I I M
=
+−=
+−=
∑
∑
∑2
2
M ti Ab t Fi d A i
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 44/58
α
ω α
ω α
z z
xz yz y
yz xz x
I M
I I M
I I M
=
+−=
+−=
∑
∑
∑2
2
• For a rigid body rotation around a fixed axis,
• If symmetrical with respect to the xy plane,
Motion About a Fixed Axis
α z z y x ===
• If not symmetrical, the sum of external moments
will not be zero, even if α = 0,
022
=== ∑∑∑ z xz y yz x M I M I M ω ω
• A rotating shaft requires both static and
dynamic balancing to avoid excessive
vibration and bearing reactions.
( )0=
( )0≠
P bl 3
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 45/58
• Expressing that the system of external
forces is equivalent to the system of
SOLUTION:
• Evaluate the system of effective forces
by reducing them to a vector
attached at G and couple
am
.G H
Problem: 3
Rod AB with weight W = 20 kg is
pinned at A to a vertical axle which
rotates with constant angular velocity
ω = 15 rad/s. The rod position is
maintained by a horizontal wire BC .
Determine the tension in the wire and
the reaction at A.
e ect ve orces, wr te vector express ons
for the sum of moments about A and thesummation of forces.
• Solve for the wire tension and the
reactions at A.
P bl 3
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 46/58
SOLUTION:• Evaluate the system of effective forces by reducing them
to a vector attached at G and coupleam
.G H
( )
( ) I
I L I r aa n
2
2
212
sm5.112
cos
−=
−=−== ω β ω
( ) ( ) I am
N22505.11220 −=−=
Problem: 3
k I j I i I H z z y y x xG ++=
0sincos
0 2
212
21
==−=
===
z y x
z y x mL I I mL I
ω β ω ω β ω ω
imL H G
β ω cos2
121−=
( ) ( )
( )k k mL
imL ji
H H H GGxyzGG
mN5.649cossin
cossincos0
22
121
2
121
⋅==
×+−+=
×+=
β β ω
β ω β ω β ω
ω
Problem: 3
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 47/58
• Expressing that the system of external forces is equivalentto the system of effective forces, write vector expressions
for the sum of moments about A and the summation of
forces.
( )eff A A M M ∑∑ =
K I J J I I T J
5.6492250886.02.1961732.1
−
+−×=−×+−×
Problem: 3
...
N1613=T
( )eff
F F ∑∑ =
I J I K A J A I A Z Y X
22502.1961613 −=−−++
( ) ( ) J I A
N96.21N976 +−=
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 48/58
• A gyroscope consists of a rotor with its mass center
fixed in space but which can spin freely about its
geometric axis and assume any orientation.
• From a reference position with gimbals and a
reference diameter of the rotor aligned, thegyroscope may be brought to any orientation
through a succession of three steps:
’a ro a on o ou er g m a roug a ou ,
b) rotation of inner gimbal through q about
c) rotation of the rotor through y about CC’.
• ϕ , θ , and ψ are called the Eulerian Angles and
spinof rate
nutationof rate
precessionof rate
=
=
=
Ψ
θ
φ
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 49/58
• The angular velocity of the gyroscope,
k jK
Ψ θ φ ω ++=
( )k ji
jiK
θ φ Ψ θ θ φ ω
θ θ
cossin
cossinwith
+++−=
+−=
• Equation of motion,
OOxyzOO =
( )
jK
k I j I i I H O
θ φ Ω
θ φ Ψ θ θ φ
+=
++′+′−= cossin
( ) ( )
( ) ( )
( )θ φ Ψ
θ φ Ψ θ φ θ θ φ θ
θ φ Ψ θ θ φ θ θ φ
cos
cossincossin
coscos2sin
2
+=
++−′=
+++′−=
∑
∑
∑
dt
d I M
I I M
I I M
z
y
x
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 50/58
Steady precession,
constantare,, ψ φ θ
k i
k I i I H
k i
zO
z
θ φ θ φ Ω
ω θ φ
ω θ φ ω
cossin
sin
sin
+−=
+′−=
+−=
( ) j I I
H M
z
OO
θ φ θ φ ω
Ω
sincos′−=
×=∑
Couple is applied about an axisperpendicular to the precession
and spin axes
When the precession and spin
axis are at a right angle,
j I M O
φ Ψ
θ
=
°=
∑
90
Gyroscope will precess about an
axis perpendicular to both the
spin axis and couple axis.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 51/58
• Consider motion about its mass center of anaxisymmetrical body under no force but its own
weight, e.g., projectiles, satellites, and space craft.
constant0 == GG H H
• Define the Z axis to be aligned with and z in a
rotating axes system along the axis of symmetry.
The x axis is chosen to lie in the Zz plane.
G H
G x I H H θ ′=−= sin
I
G
x ′
−=ω s n
y y I H ′== 0 0= y
zG z I H H θ == cos I
H G z
θ ω
cos=
• θ = constant and body is in steady precession.
• Note: θ γ ω
tantan I
I
z
x
′==−
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 52/58
Two cases of motion of an axisymmetrical bodywhich under no force which involve no precession:
• Body set to spin about its axis of symmetry,
alignedareand0
G
x x
H H
ω ω ==
and body keeps spinning about its axis of
symmetry.
• Body is set to spin about its transverse axis,
alignedareand
0
G
z z
H
H
ω
==
and body keeps spinning about the given
transverse axis.
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 53/58
The motion of a body about a fixed point (or its masscenter) can be represented by the motion of a body
cone rolling on a space cone. In the case of steady
precession the two cones are circular.
• I < I’. Case of an elongated body. γ < θ and the
vector ω lies inside the angle ZGz. The space
cone and body cone are tangent externally; the
spin and precession are both counterclockwise
from the positive z axis. The precession is said tobe direct .
• I > I’. Case of a flattened body. γ > θ and the
vector ω lies outside the angle ZGz. The space
cone is inside the body cone; the spin and
precession have opposite senses. The precession
is said to be retrograde.
k h jhih=h 3210++
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 54/58
0
∧
321
3210
hhh
k ji =h ω ω ω ω
( ) ( ) ( )k hh jhhihh=h 2121313132320ω −+−−−∧
∧
321
3210
ω ω ω
ω ω ω ω
C B A
k ji
=h
3210
( ) ( ) ( )k B A j AC i BC =h 2121131332320ω −+−−−∧
54
Angular Momentum
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 55/58
g
( )Goo G Go= + M h h vr ∧
Angular Momentum (Rigid Body)
(4)
(5)
1 1 2 3
2 1 2 3
xx xy zx
yx yy yz
h = I - I - I h = - I + I - I
- -
ω ω ω ω ω ω
Angular Momentum (if Principle Axes used)
(6)
55
3 1 2 3 zx yz yy
1 2 3 xx yy zzo = I i + I j + I k h ω ω ω
Equations of Motion
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 56/58
Equations of Motion (if O and G coincide and/or
a 0=0)
h+t h =
dt hd =T
ooo
o ∧Ω∂
∂
E uations of Motion 12 ex ressed as Scalar Com onents
(11)
(12)
( )o
o Go o
d h- M =aT r dt ∧
See Equation (14) for the special case in which the reference axes are fixed
along the principle axes of the body.
(13)
56
1 1 2 3 3 2
2 2 3 1 1 3
3 3 1 2 2 1
T h h h
T h h h
T h h h
= − Ω + Ω
= − Ω + Ω
= − Ω + Ω
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 57/58
8/7/2019 Dynamics_Lecture9 [Compatibility Mode]
http://slidepdf.com/reader/full/dynamicslecture9-compatibility-mode 58/58