Calculus III: Practice Midterm II, Exams of Vector Analysis

A practice midterm for Calculus III. It contains 5 problems that cover topics such as vector functions, acceleration and velocity vectors, and normal planes. The problems require students to show their work and partial credit is given for incomplete work. The document also includes a formula sheet. The practice midterm is useful for students preparing for an exam in Calculus III.

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2022/2023

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Calculus III: Practice Midterm II
Name:
Write your solutions in the space provided. Continue on the back if you need more
space.
You must show your work. Only writing the final answer will receive little credit.
Partial credit will be given for incomplete work.
The exam contains 5 problems.
The last page is the formula sheet, which you may detatch.
Good luck!
Question Points Score
1 10
2 10
3 10
4 10
5 10
Total: 50
1
pf3
pf4
pf5

Partial preview of the text

Download Calculus III: Practice Midterm II and more Exams Vector Analysis in PDF only on Docsity!

Calculus III: Practice Midterm II

Name:

  • Write your solutions in the space provided. Continue on the back if you need more

space.

  • You must show your work. Only writing the final answer will receive little credit.
  • Partial credit will be given for incomplete work.
  • The exam contains 5 problems.
  • The last page is the formula sheet, which you may detatch.
  • Good luck!

Question Points Score

Total: 50

  1. (10 points) Write true or false. No justification is needed.

(a) The curve parametrized by 〈sin(2t), cos(3t), 1 + t

3 〉 never intersects the XY plane.

Solution: False. It intersects the XY plane at t = −1.

True False

(b) If the acceleration vector is perpendicular to the velocity vector, the object must

be going in a circle or helix.

Solution: False. Any motion with constant speed will have this property.

True False

(c) The graph of the function f (x, y) = x

2

  • y

2 is a hemisphere.

Solution: False.

True False

(d) For a vector function

r (t), we have

d(

r (t) ·

r (t))

dt

d

r (t)

dt

d

r (t)

dt

Solution: False. The derivative of a (dot) product must be computed by the

product rule.

True False

(e) If T , N , and B represent the unit tangent, normal, and binormal vectors, then

T = N × B.

Solution: True. T, N, B form a frame just like the i, j, k.

True False

  1. (10 points) For which positive real number a does the curve y

2 = x

2

  • a

2 have curvature

2 at the point (0, a)?

Solution: We can choose the parameterization 〈t,

a

2

  • t

2 〉. This will only trace

the y > 0 part of the curve, but that is sufficient since (0, a) is on this part.

We now compute the curvature at t = 0.

r(t) =

t,

a

2

  • t

2

r

′ (t) =

t

a

2

  • t

2

r

′′ (t) =

a

2

  • t

2

t

2

(a

2

  • t

2 )

3 / 2

a

2

(a

2

  • t

2 )

3 / 2

Therefore,

r

′ (0) = 〈 1 , 0 〉 = i

r

′′ (0) = 〈 0 , 1 /a〉 = (1/a)j.

Using

κ =

|r

′ × r

′′ |

|r

′ |

3

we get

κ =

|i × (1/a)j|

|i|

3

a

For κ = 2, we must have a = 1/2.

  1. The force acting on an object of mass 2 units is given by the vector

F (t) = 〈 0 , 16 cos(2t), 16 sin(2t)〉.

At t = 0, the object is at 〈 0 , 0 , 0 〉 and is travelling with velocity 〈 3 , 0 , − 4 〉.

(a) (5 points) How much distance does it travel between t = 0 and t = 10?

Solution: Using

F = m

a , we get that the acceleration is

a (t) = 〈 0 , 8 cos(2t), 8 sin(2t)〉.

Integrating, we get the velocity

v (t) = 〈 0 , 4 sin(2t), −4 cos(2t)〉 +

c.

Since

v (0) = 〈 3 , 0 , − 4 〉, we get

c = 〈 3 , 0 , 0 〉. Hence

v (t) = 〈 3 , 4 sin(2t), −4 cos(2t)〉.

At this point, we can compute the position, but we don’t need to. The speed is

v (t)| =

2

  • 4

2 = 5.

Hence in 10 seconds, the object travels 50 units.

(b) (5 points) Write an equation of the normal plane to its motion at t = π.

Solution: We must calculate the position. Integrating

v (t), we get

r (t) = 〈 3 t, −2 cos(2t), −2 sin(2t)〉 +

c.

Since

r (0) = 〈 0 , 0 , 0 〉, we have

c = 〈 0 , 2 , 0 〉. Hence

r (t) = 〈 3 t, 2 − 2 cos(2t), −2 sin(2t)〉.

At t = π, we have

r (π) = 〈 3 π, 0 , 0 〉

r

′ (π) =

v (π) = 〈 3 , 0 , − 4 〉.

The normal plane is the plane through 〈 3 π, 0 , 0 〉 and perperdicular to 〈 3 , 0 , − 4 〉.

The equation is

3(x − 3 π) − 4 z = 0

that is: 3x − 4 z = 9π.

LIST OF USEFUL IDENTITIES

  1. Derivatives

d

dx

x

n = nx

n− 1

d

dx

sin x = cos x

d

dx

cos x = − sin x

d

dx

tan x = sec

2 x

d

dx

cot x = − csc

2 x

d

dx

sec x = sec x tan x

d

dx

csc x = − csc x cot x

d

dx

e

x = e

x

d

dx

ln |x| =

1

x

d

dx

arcsin x =

1 √ 1 −x^2

d

dx

arccos x =

− 1 √ 1 −x^2

d

dx

arctan x =

1

1+x^2

  1. Trigonometry

(1) sin

2 x + cos

2 x = 1

(2) tan

2 x + 1 = sec

2 x

(3) 1 + cot

2 x = csc

2 x

(4) sin(x ± y) = sin x cos y ± cos x sin y

(5) cos(x ± y) = cos x cos y ∓ sin x sin y

(6) sin

2 x =

1 −cos 2x

2

(7) cos

2 x =

1+cos 2x

2

  1. Space curves

For a parametric space curve given by r(t)

(1) Curvature κ =

|r

′ (t) × r

′′ (t)|

|r

′ (t)|

3

(2) Tangent component of acceleration aT = |r

′ (t)|

r

′ (t) · r

′′ (t)

|r

′ (t)|

(3) Normal component of acceleration aN = κ|r

′ (t)|

2

|r

′ (t) × r

′′ (t)|

|r

′ (t)|

1