COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 1.
First note:
Have
y=
b2 − b1
x + b1
a
I y = ∫ x 2dA
b2 − b1
x + b1
a
a
x 2d ydx
0 0
=∫ ∫
a
b − b1
= ∫ 0 x2 2
x + b1 dx
a
a
1 b − b1 4 1 3
= 2
x + b1x
3
4 a
0
=
1 3
a ( b1 + 3b2 )
12
Iy =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
1 3
a ( b1 + 3b2 )
12
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 2.
At
5
x = a, y = b :
∴ y =
b
a
5
2
5
b = ka 2
x2
or
dI y =
1 3
x dy
3
=
Then
Iy =
x=
or
a
b
b
5
a2
2
2
5
y5
1 a3 65
y dy
3 b 65
1 a3 b 65
∫ y dy
3 b 65 0
1 5 a3 115
=
y
3 11 b 65
=
k =
b
0
5 a3 115
b
33 b 65
or I y =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
5 3
ab
33
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 3.
At x = 0:
First note:
At x = a :
a = k ( 2b − b )
k =
∴ x=
Have
2
c = −b
or
or
0 = k (b + c)
2
a
b2
a
2
y − b)
2(
b
I y = ∫ x 2dA
=∫
a
2
y − b)
2b b 2 (
0
0
∫
x 2dxdy
3
=
1 2b a
2
y − b ) dy
∫
0 2(
3
b
2b
1 a3 1
7
=
× ( y − b)
6
3b
7
b
=
1 3
ab
21
Iy =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
1 3
ab
21
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 4.
y = kx 2 + c
Have
b = k ( 0) + c
x = 0, y = b :
At
c=b
or
At
x = 2a, y = 0:
or
k =−
y =−
Then
=
Then
I y = ∫ x 2dA,
2a
I y = ∫ a x 2dA =
2
0 = k ( 2a ) + b
b
4a 2
b 2
x +b
4a 2
b
4a 2 − x 2
4a 2
(
dA = ydx =
)
(
)
b
4a 2 − x 2 dx
4a 2
(
)
b 2a 2
2
2
∫ x 4a − x dx
4a 2 a
2a
b 2 x3 x5
=
−
4a
3
5 a
4a 2
=
b
b
8a3 − a3 −
32a5 − a5
2
3
20a
=
7a3b 31a3b
−
3
20
(
)
(
)
Iy =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
47 3
ab
60
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 5.
First note:
Have
y =
b2 − b1
x + b1
a
I x = ∫ y 2dA
=
b2 − b1
x + b1
a
a
0 0
∫ ∫
y 2d ydx
3
1 a b − b1
= ∫0 2
x + b1 dx
3 a
4
1 1 a b2 − b1
= ×
x + b1
3 4 b2 − b1 a
a
0
=
1
a
b24 − b14
12 b2 − b1
=
1
a
( b2 + b1 )( b2 − b1 ) b22 + b12
12 b2 − b1
=
1
a ( b1 + b2 ) b12 + b22
12
(
)
(
(
)
)
Ix =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
1
a ( b1 + b2 ) b12 + b22
12
(
)
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 6.
SOLUTION
5
At x = a, y = b : b = ka 2
or k =
∴y =
b
5
a2
b
a
5
x2
5
2
I x = ∫ y 2dA
=
b
a
2
y 5 dy
b
2
∫0 y
a
dA = xdy
2
5
5 175
= 2 ×
y
b 5 17
b
0
17
5a b 5
=
17 b 52
or I x =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
5 3
ab
17
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 7.
At x = 0: 0 = k ( b + c )
First note:
or
2
c = −b
At x = a : a = k ( 2b − b )
Have
or
k =
a
b2
∴
x=
a
2
y − b)
2(
b
2
I x = ∫ y 2dA
=∫
a
2
y − b)
2b b 2 (
0
b
∫
y 2dxdy
=
a 2b 2
2
y ( y − b ) dy
2 ∫b
b
=
a 2b 4
y − 2by 3 + b 2 y 2 dy
2 ∫b
b
=
a 1 5 1 4 1 2 3
y − by + b y
2
3
b2 5
b
=
a 1
1
1 2
1 2 3
5
4
3
1 5 1
4
( 2b ) − ( 2b ) + b ( 2b ) − b − b b + b b
2
3
5
2
3
b 2 5
(
)
2b
( )
( )
8 1 1 1
32
= ab3
−8+ − + −
3 5 2 3
5
=
31 3
ab
30
Ix =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
31 3
ab
30
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 8.
Have
y = kx 2 + c
At
x = 0, y = b: b = k (0) + c
or
c=b
At
x = 2a, y = 0: 0 = k (2a) 2 + b
or
k =−
Then
y =
Now
dI x =
=
b
4a 2
b
4a 2 − x 2
4a 2
(
)
1 3
y dx
3
3
1 b3
4a 2 − x 2 dx
6
3 64a
(
)
continued
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Then
I x = ∫ dI x
=
3
1 b3 2 a
4a 2 − x 2 dx
6 ∫a
3 64a
=
b3
2a
64a 6 − 48a 4 x 2 + 12a 2 x 4 − x 6 dx
6 ∫a
192a
(
)
(
)
2a
b3
12 2 5 x 7
6
4 3
64
a
x
16
a
x
a x −
=
−
+
5
7 a
192a 6
=
b3
64a 7( 2 − 1) − 16a 7 ( 8 − 1)
192a 6
+
=
12 7
1
a ( 32 − 1) − (128 − 1)
5
7
ab3
372 127
3
−
64 − 112 +
= 0.043006ab
192
5
7
I x = 0.0430ab3
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 9.
x2
y2
+
=1
a 2 b2
x = a 1−
y2
b2
dA = xdy
dI x = y 2dA = y 2 xdy
b
b
I x = ∫ dI x = ∫ − b xy 2dy = a ∫ − b y 2 1 −
Set: y = b sin θ
y2
dy
b2
dy = b cosθ dθ
π
I x = a ∫ 2π b 2 sin 2 θ 1 − sin 2 θ b cosθ dθ
−
2
π
π
−
−
= ab3 ∫ 2π sin 2 θ cos 2 θ dθ = ab3 ∫ 2π
2
2
1 2
sin 2θ dθ
4
π
π
1
1
1
1
2
= ab3 ∫ 2π (1 − cos 4θ ) dθ = ab3 θ − sin 4θ
− 2
4
8
4
−π
2
=
2
1 3 π π π 3
ab − − = ab
8
2 2 8
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
Ix =
1
π ab3
8
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 10.
At
2a = kb3
x = 2a, y = b:
or
k =
2a
b3
Then
x=
2a 3
y
b3
or
y =
Now
dI x =
b
( 2a )
1
1
3
x3
1 3
1 b3
y dx =
xdx
3
3 2a
2a
Then
1 b3 2 a
1 b3 1 2
I x = ∫ dI x =
xdx
x
=
∫
3 2a a
6 a 2 a
=
b3
4a 2 − a 2
12a
(
)
Ix =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
1 3
ab
4
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 11.
−a
At x = a : b = k 1 − e a
First note:
or
Have
k =
b
1 − e−1
I x = ∫ y 2dA
b
a 1− e
0 0
=∫ ∫
−x
1− e a
−1
3
y 2dydx
3
=
−x
1 b a
1 − e a dx
−1 ∫ 0
31 − e
=
−x
−2 x
−3 x
1 b a
1 − 3e a + 3e a − e a dx
−1 ∫ 0
31 − e
3
3
a
−x
1 b
a −2 x a −3x
x − 3( − a ) e a + 3 − e a − − e a
=
−1
31 − e
2
3
0
3
1 b
1
1
=
a + 3ae−1 − 1.5ae−2 + ae −3 − 3a − 1.5a + a
−1
3 1 − e
3
3
=
1
ab3
3 1 − e −1
(
)
3
11
1.91723 −
6
= 0.1107ab3
I x = 0.1107ab3
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 12.
x2
y2
+
=1
a 2 b2
y = b 1−
x2
a2
dA = 2 ydx
dI y = x 2dA = 2 x 2 ydx
a
a
I y = ∫ dI y = ∫ 0 2 x 2 ydx = 2b ∫ 0 x 2 1 −
x = a sin θ
Set:
x2
dx
a2
dx = a cosθ dθ
π
I y = 2b∫ 02 a 2 sin 2 θ 1 − sin 2 θ a cosθ dθ
3
π
2
2
3
π
= 2a b∫ sin θ cos θ dθ = 2a b∫ 02
2
0
π
1 2
sin 2θ dθ
4
π
1
1
1
1
2
= a3b∫ 02 (1 − cos 4θ ) dθ = a3b θ − sin 4θ
2
2
4
4
0
=
1 3 π
π
a b − 0 = a3b
4
2
8
Iy =
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
1 3
πa b
8
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 13.
At
x = 2a, y = b : 2a = kb3
2a 3
y
b3
Then
x=
or
y =
Now
I y = ∫ x 2dA
Then
I y = ∫ a x2
b
( 2a )
=
=
=
1
b
( 2a )
1
3
x 3 dx
7
b
( 2a )
x3
dA = ydx
2a
=
1
1
3
1
3
b
1
( 2a ) 3
2a
∫ a x 3 dx
3 103
x
10
3b
10 ( 2a )
1
3
2a
a
2a 103 − a 103
( )
10
3ba3 103
2 − 1 3
1
10 ( 2 ) 3
= 2.1619a3b
or I y = 2.16a3b
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 14.
First note:
or
Have
−a
At x = a : b = k 1 − e a
k =
b
1 − e−1
I y = ∫ x 2dA
b
a 1− e
0 0
−x
1− e a
−1
2
x d ydx
=
∫ ∫
=
∫ 0 x 1 − e−1 1 − e a dx
a 2
b
−x
a
−x
2
b 1 3
e a 1 2
1
x
x
2
x
2
=
−
−
−
−
+
3
1 − e−1 3
a
1 a
−
a
0
=
2
b 1 3
a
3 −1 a
3
+
a
a
e
2 + 2 + 2 − a × 2
−1
a
1 − e 3
a
=
a3b 1
+ 5e −1 − 2
−1
1− e 3
(
)
= 0.273a3b
I y = 0.273 a3b
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 15.
k1 =
or
Then
y1 =
and
x1 =
b 4
x
a4
a
b
1
4
b = k2a 4
b
a4
k2 =
b
y2 =
1
4
b
1
a4
1
x4
a
a
x2 = 4 y 4
b
1
y4
A = ∫ ( y2 − y1 ) dx = b∫
Now
1
b = k1a 4
x = a, y = b:
At
x 14
a
0
a
1
4
−
x 4
dx
a4
a
4 x 54 1 x5
= 3 ab
= b
−
5
5 a 14 5 a 4
0
I x = ∫ y 2dA
Then
dA = ( x1 − x2 ) dy
a 1
a
b
I x = ∫ 0 y 2 1 y 4 − 4 y 4 dy
4
b
b
b
4 y 134
1 y 7
= a
−
7 b4
13 b 14
0
1
4
= ab3 −
13 7
or I x =
Now
kx =
Ix
=
A
15 3
ab
91
=
3
ab
5
15 3
ab
91
25 2
b = 0.52414b
91
or k x = 0.524b
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 16.
First note:
At x = a :
2b = k a
or
Straight line:
Now:
k=
2b
a
y1 =
b
x
a
∴ y2 =
2b
a
x
b
a 2b 12
A = 2∫ 0
x − x dx
a
a
a
4 x 23
1 2
= 2b
−
x
3 a 2a
0
=
Have
5
ab
3
I x = ∫ y 2dA
1
2b 2
x
a
a
0 bx
a
= 2∫ ∫
=
y 2dydx
2 a 8b3 32 b3 3
x − 3 x dx
∫
3 0 a 23
a
a
2b3 2
8 5
1
=
× 3 x 2 − 3 x 4
3 5 a2
4a
0
Ix =
And
kx =
=
59 3
ab
30
Ix
A
59 3
ab
30
5
ab
3
= b 1.18
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
k x = 1.086 b
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 17.
At
x = a, y = b:
k1 =
or
Then
Now
y1 =
1
b = k1a 4
b = k2a 4
b
a4
b
b 4
x
a4
k2 =
y2 =
and
A = ∫ ( y2 − y1 ) dx = b∫
1
a4
x 14
a
0
a
1
4
−
b
a
1
4
1
x4
x 4
dx
a4
a
4 x 54 1 x5
= 3 ab
= b
−
1
4
5
5 a4 5 a
0
dA = ( y2 − y1 ) dx
Now
I y = ∫ x 2dA
Then
b 1
b
a
I y = ∫ 0 x 2 1 x 4 − 4 x 4 dx
4
a
a
= b∫
x 94
a
0
a
1
4
−
x 6
dx
a4
a
4 x 134
1 x 7
= b
−
7 a4
13 a 14
0
1
4
= b a3 − a3
7
13
or I y =
Now
ky =
Iy
A
=
15 3
ab
91
=
3
ab
5
15 3
ab
91
25
a = 0.52414a
91
or k y = 0.524a
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 18.
First note:
At x = a :
2b = k a
or
Straight line:
Now:
k=
2b
a
y1 =
b
x
a
∴ y2 =
2b
a
x
b
a 2b 12
A = 2∫ 0
x − x dx
a
a
a
4 x 23
1 2
= 2b
−
x
3 a 2a
0
=
Have
5
ab
3
I y = ∫ x 2dA
1
2b 2
x
a
a
b
0
x
a
= 2∫ ∫
x 2dydx
2b 12 b
a
x − x dx
= 2∫ 0 x 2
a
a
7
2 x2
1 x 4
= 2b 2 ×
−
7 a 4 a
=
a
0
9 3
ab
14
Iy =
9 3
ab
14
continued
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
And
ky =
=
=a
Iy
A
9 3
ab
14
5
ab
3
27
70
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
k y = 0.621 a
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 19.
First note:
At x = 0: b = c cos ( 0 )
c=b
or
At x = 2a : b = b sin k ( 2a )
2ka =
or
k=
Then
π
2
π
4a
π
π
2a
A = ∫ a b sin
x − b cos
x dx
4a
4a
2a
π
4a
π
4a
= b − cos
x−
sin
x
4a
π
4a a
π
=−
=
Have
4ab
1
1
+
(1) −
π
2
2
4ab
π
(
)
2 −1
I x = ∫ y 2dA
π
2 a b sin 4a x
= ∫a ∫
b cos
=
π
4a
x
y 2dydx
1 2a 3 3 π
3
3 π
∫ b sin 4a x − b cos 4a x dx
3 a
2a
b3 4a
π
1 4a
π 4a
π
1 4a 3 π
x+
cos3
x − sin
x−
sin
x
=
− cos
3 π
4a
3π
4a π
4a
3π
4a a
=
4ab3
−1 +
3π
3
3
1 1
1 1
1
1 1
−
−
+
−
+
3 2 3 2
3 2
2
=
4ab3 5
2
2−
3π 6
3
continued
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
Ix =
2
ab3 5 2 − 4
9π
(
)
= 0.217 ab3
And
kx =
=
I x = 0.217 ab3
Ix
A
2
ab3 5 2 − 4
9π
4
ab 2 − 1
π
(
(
)
)
= 0.642b
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
k x = 0.642 b
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 20.
At x = 0: b = c cos ( 0 )
First note:
c=b
or
At x = 2a : b = b sin k ( 2a )
2ka =
or
k=
π
2
π
4a
π
π
2a
A = ∫ a b sin
x − b cos
x dx
4a
4a
Then
2a
π
4a
π
4a
= b − cos
x−
sin
x
4a
π
4a a
π
=−
=
Have
4ab
1
1
+
(1) −
π
2
2
4ab
π
(
)
2 −1
I y = ∫ x 2dA
π
2 a b sin 4a x 2
x dydx
a b cos π x
4a
=
∫ ∫
=
2a 2
∫ a x b sin 4a x − b cos 4a x dx
π
π
continued
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
COSMOS: Complete Online Solutions Manual Organization System
2
π
2
π
x
π
2x
= b
+
−
sin
x
cos
x
cos
x
2
3
π
4a
4a
4a
π
π
4a
4a
4a
2a
2
2x
π
2
π
x
π
cos
x
sin
x
sin
x
−
−
+
3
π 2
π
4a
4a
4a
π
4a
4a
4a
a
2a
64a3b
π
π π
π
π
π 2 2
Iy =
sin
x
cos
x
x
sin
x
cos
x
2
x
−
+
+
−
4a 2a
4a
4a
π 3 4a
16a 2
a
=
64a3b
π 2 1
1
π 2
1
π
1
2
2
+
−
−
+
−
(
)(
)
(
)
4 2
16
π 3
2
I y = 1.482a3b
= 1.48228a3b
And
ky =
=
Iy
A
1.48228a3b
4ab
2 −1
π
(
)
= 1.676a
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
k y = 1.676a
COSMOS: Complete Online Solutions Manual Organization System
Chapter 9, Solution 21.
dI x =
(a)
Ix =
1 3
a dx
3
1 3 a
a3
2
a ∫ − a dx =
( 2a ) = a 4
3
3
3
dI y = x 2dA = x 2adx
I y = a∫
a 2
x dx
−a
JO = I x + I y =
JO =
kO2 A
a
x3
2
= a = a4
3 −a 3
2 4 2 4
a + a
3
3
4 4
a
JO
2
k =
= 3 2 = a2
A
3
2a
2
JO =
4 4
a
3
kO = a
2
3
(b)
dI x =
Ix =
1 3
a dx
12
a 3 2a
a 3 2a 1 4
dx
=
[ x] = 6 a
∫
12 0
12 0
dI y = x 2dA = x 2 ( adx )
I y = a∫
2a 2
x dx
0
JO = I x + I y =
J O = kO2 A
2a
x3
8
= a = a4
3
3 0
1 4 8 4 17 4
a + a =
a
6
3
6
17 4
a
J
17 2
kO2 = O = 6 2 =
a
A
12
2a
Vector Mechanics for Engineers: Statics and Dynamics, 8/e, Ferdinand P. Beer, E. Russell Johnston, Jr.,
Elliot R. Eisenberg, William E. Clausen, David Mazurek, Phillip J. Cornwell
© 2007 The McGraw-Hill Companies.
JO =
17 4
a
6
kO = a
17
12