Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b)...

54
Relative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1

Transcript of Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b)...

Page 1: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative and Circular Motiona) Relative motionb) Centripetal acceleration

Mechanics Lecture 3, Slide 1

Page 2: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Mechanics Lecture 3, Slide 2

Page 3: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Time on Video Prelecture

Looks like mostly everyone here has viewed entire prelecture…GOOD!Thank you to those of you who did!

Mechanics Lecture 3, Slide 3

Page 4: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Lecture Thoughts

Mechanics Lecture 3, Slide 4

Page 5: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

What is the speed of Mike relative to the station?

A. -1 m/sB. 30 m/sC. 29 m/sD. 31 m/s

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Mechanics Lecture 3, Slide 5

Page 6: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion in 1 dimension

Mechanics Lecture 3, Slide 6

Page 7: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Position and Reference Frames

Position of Mike in the ground frame is the vector sum of the position vector of Mike in the train reference frame and the position vector of the train in the ground reference frame.

Mechanics Lecture 3, Slide 7

Page 8: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion and Reference Frames

Differentiate the position vectors to obtain the velocity vectors

Mechanics Lecture 3, Slide 8

Page 9: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion and Reference Frames

Mechanics Lecture 3, Slide 9

Page 10: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion and Reference Frames

Mechanics Lecture 3, Slide 10

Page 11: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Prelecture 3, Questions 1 again

A.

B.

C.

D.

0% 0%0%0%-12m

Mechanics Lecture 3, Slide 11

Page 12: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

vbelt,ground = 2 m/s

vdog,belt = 8 m/s

A) 6 m/s B) 8 m/s C) 10 m/s

CheckPoint

A girl stands on a moving sidewalk that moves to the right at 2 m/srelative to the ground. A dog runs toward the girl in the opposite direction along the sidewalk at a speed of 8 m/s relative to the sidewalk.

What is the speed of the dog relative to the ground?

Mechanics Lecture 3, Slide 12

Page 13: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

vdog, ground = vdog, belt + vbelt, ground= (−8 m/s) + (2 m/s) = −6 m/s

+x

vbelt,ground = 2 m/s

vdog,belt = 8 m/s

What is the speed of the dog relative to the ground?

A) 6 m/s B) 8 m/s C) 10 m/s

Mechanics Lecture 3, Slide 13

Page 14: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

42% of you got this right –let’s do this again

CheckPoint

A girl stands on a moving sidewalk that moves to the right at 2 m/s relative to the ground. A dog runs toward the girl in the opposite direction along the sidewalk at a speed of 8 m/s relative to the sidewalk.

What is the speed of the dog relative to the girl?

vbelt,ground = 2 m/s

vdog,belt = 8 m/s

A) 6 m/s B) 8 m/s C) 10 m/s

Mechanics Lecture 3, Slide 14

Page 15: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

What is the speed of the dog relative to the girl? A.

B.

C.

0% 0%0%

vbelt,ground = 2 m/s

vdog,belt = 8 m/s

A) 6 m/s B) 8 m/s C) 10 m/s

C) The dog and girl are running towards each other so when you add the two velocities together it would be 8+2.

A) Because the girl is actually moving and the two vectors are opposite, so together they make 6 m/s

B) Because the girl is not moving relative to the belt, and the dog is going 8 m/s relative to the belt, the dog is also moving 8 m/s relative to the girl..

Mechanics Lecture 3, Slide 15

Page 16: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

B) Because the girl is not moving relative to the belt, and the dog is going 8 m/s relative to the belt, the dog is also moving 8 m/s relative to the girl.

Using the velocity formula:vdog, girl = vdog, belt + vbelt, girl

= −8 m/s + 0 m/s = −8 m/s

What is the speed of the dog relative to the girl?

vbelt,ground = 2 m/s

vdog,belt = 8 m/s

A) 6 m/s B) 8 m/s C) 10 m/s

Mechanics Lecture 3, Slide 16

Page 17: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion in 2 Dimensions

Speed relative to shore

Mechanics Lecture 3, Slide 17

Page 18: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion in 2 Dimensions

Direction w.r.t shoreline

Mechanics Lecture 3, Slide 18

Page 19: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Relative Motion in 2 Dimensions

Caveat !!!!The simple addition of velocities as shown only works for speeds much less than the speed of light…need special relativity at v~c.

Mechanics Lecture 3, Slide 19

Page 20: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Moving Sidewalk Question A.

B.

C.

D.

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A man starts to walk along the dotted line painted on a moving sidewalktoward a fire hydrant that is directly across from him. The width of thewalkway is 4 m, and it is moving at 2 m/s relative to the fire-hydrant. If his walking speed is 1 m/s, how far away will he be from the hydrant when he reaches the other side?

A) 2 m

B) 4 m

C) 6 m

D) 8 m

Mechanics Lecture 3, Slide 20

Page 21: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Time to get across:

∆t = distance / speed= 4m / 1m/s = 4 s

If the sidewalk wasn’t moving:

sidewalkmanv ,

Mechanics Lecture 3, Slide 21

Page 22: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Just the sidewalk:

hydrantsidewalkv ,

Mechanics Lecture 3, Slide 22

Page 23: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

D = (speed of sidewalk) ∙ (time to get across)= (2 m/s) ∙ (4 s) = 8 m

D

Mechanics Lecture 3, Slide 23

Page 24: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Combination of motions: Vector solution

jiv

jiv

jiv

vvv

hydrantman

hydrantsidewalk

sidewalkman

hydrantsidewalksidewalkmanhydrantman

ˆ2ˆ1

ˆ2ˆ0

ˆ0ˆ1

,

,

,

,,,

+−=

+=

+−=

+=

( )( )

myjyjt

stiit

jyitjijitr

tvrtr

jir

tvrtr

cross

crosscross

crosscrosshydrantman

crosshydrantmanhydrantmancrosshydrantman

hydrantman

hydrantmanhydrantmanhydrantman

8ˆˆ2

4ˆ0ˆ4

ˆˆ0ˆ2ˆ1ˆ0ˆ4)(

)(

ˆ0ˆ4

)(

,

,0,,

0,

,0,,

=⇒=

=⇒=−

+=×+−++=

×+=

+=

×+=

Mechanics Lecture 3, Slide 24

Page 25: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Mechanics Lecture 3, Slide 25

Page 26: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Swim Race A.

B.

C.

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20%

Three swimmers can swim equally fast relative to the water. They have a race to see who can swim across a river in the least time. Relative to the water, Beth swims perpendicular to the flow, Ann swims upstream at 30 degrees, and Carly swims downstream at 30 degrees.

Who gets across the river first?

A) Ann B) Beth C) Carly

x

y

AnnBeth

Carly

Mechanics Lecture 3, Slide 26

Page 27: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

AB

C

Vy,Beth = Vo

30o 30o

Vy,Ann = Vocos(30o)

Vy,Carly = Vocos(30o)

Time to get across = D / Vy

D

Look at just water & swimmers

x

y

Mechanics Lecture 3, Slide 27

Page 28: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

x

y

Clicker Question

Three swimmers can swim equally fast relative to the water. They have a race to see who can swim across a river in the least time. Relative to the water, Beth swims perpendicular to the flow, Ann swims upstream at 30 degrees, and Carlyswims downstream at 30 degrees.

Who gets across the river second?

A) Ann B) Carly C) Both same

Ann Carly

Mechanics Lecture 3, Slide 28

Page 29: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Accelerating (Non-Inertial) Frames of Reference

Accelerating Frame of Reference

Confusing due to the fact that the acceleration can result in what appears to

be a “push or pull”.

Mechanics Lecture 3, Slide 29

Page 30: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Accelerated Frames of Reference

Accelerating Frame of Reference

Accelerometer can detect change in velocity

Mechanics Lecture 3, Slide 30

Page 31: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Inertial Frames of Reference

Inertial Frames of Reference

Non-accelerating frames of reference in a state of constant, rectilinear motionwith respect to one another. An accelerometer moving with any of them woulddetect zero acceleration.

Mechanics Lecture 3, Slide 31

Page 32: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

A girl twirls a rock on the end of a string around in a horizontal circle above her head as shown from above in the diagram.

If the string breaks at the instant shown, which of the arrows best represents the resulting path of the rock?

A

B

C

D

Top view looking down

After the string breaks, the rock will have no force acting on it, so it cannot accelerate. Therefore, it will maintain its velocity at the time of the break in the string, which is directed tangent to the circle.

CheckPoint

Mechanics Lecture 3, Slide 32

Page 33: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Survey

Mechanics Lecture 3, Slide 33

Page 34: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Rotating Reference Frames

Mechanics Lecture 3, Slide 34

Page 35: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Rotating Reference Frames

Direction ChangingSpeed is constant.

Acceleration

Mechanics Lecture 3, Slide 35

Page 36: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Rotating Reference Frames

Mechanics Lecture 3, Slide 36

Page 37: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Rotating Reference Frames

Mechanics Lecture 3, Slide 37

Page 38: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Rotating Reference Frames

Mechanics Lecture 3, Slide 38

Page 39: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration

Constant speed in circular path

Acceleration directed toward center of circle

What is the magnitude of acceleration?

Proportional to:1. Speed

1. time rate of change of angle or angular velocity

Mechanics Lecture 3, Slide 39

Page 40: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration

Mechanics Lecture 3, Slide 40

Page 41: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration

Mechanics Lecture 3, Slide 41

Page 42: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration

Mechanics Lecture 3, Slide 42

Page 43: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

v = ωR

Once around:

ω = ∆θ / ∆t = 2π / Τv = ∆x / ∆t = 2πR / T

ω is the rate at which the angle θ changes:

θ

dtdθω =

Mechanics Lecture 3, Slide 43

Page 44: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

dθ v dt

R

=R dθ

Another way to see it:

v = ωR

v = RωdtdRv θ

=

Mechanics Lecture 3, Slide 44

Page 45: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration-Example

Mechanics Lecture 3, Slide 45

Page 46: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Centripetal Acceleration due to Earth’s rotation

Mechanics Lecture 3, Slide 46

Page 47: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

Mechanics Lecture 3, Slide 47

Page 48: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue

N

E

dockriverv ,

riverboatv ,

dockboatv ,

Dock Frame

θ

Mechanics Lecture 3, Slide 48

Page 49: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue-Dock Frame

jir

tvrtrjivv

jiv

jivv

dockchild

dockchilddockchilddockchild

dockriverdockchild

riverboat

childriverriverchild

ˆ6.0ˆ5.2

)(

ˆ)0(ˆ)1.3(

ˆ)sin*8.24(ˆ)cos*8.24(

ˆ0ˆ0

0

0

,

,,,

,,

,

,,

+−=

×+=

+==

+=

+==

θθ N

E

dockchildv ,

ij

boatchildv ,

Dock Frame0,dockchildr -2.5i,0.6j )(, meetdockchild ttr =

( )

( )jittr

tjijittr

tvrtvrtr

tjijitvrttr

jivvtv

meetboatchild

meetmeetboatchild

boatchilddockchildboatchildboatchildboatchild

meetmeetdockchilddockchildmeetdockchild

riverboatboatriverboatchild

ˆ0ˆ0)(

ˆ)sin*8.24(ˆ)cos*8.24(ˆ6.0ˆ5.2)(

)(

ˆ)0(ˆ)1.3(ˆ6.0ˆ5.2)(

ˆ)sin*8.24(ˆ)cos*8.24()(

,

,

,,,,,

,,,

,,,

00

0

+==

×−+−++−==

×+=×+=

×+++−=×+==

−+−=−==

θθ

θθ

Mechanics Lecture 3, Slide 49

Page 50: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue-Dock Frame

( ) ( ) hrttt

tt

tt

meetmeetmeet

meetmeet

meetmeet

1037.06.05.28.24

118.24

6.08.24

5.2

8.246.0sin0sin*8.246.0

8.245.2cos0cos*8.245.2

2222

=+−=⇒=

×

+

×

×=⇒=×−

×−

=⇒=×−−

θθ

θθ

N

E

dockchildv ,

ij

boatchildv ,

Dock Frame0,dockchildr -2.5i,0.6j )(, meetdockchild ttr =

Mechanics Lecture 3, Slide 50

Page 51: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue-Dock Frame

( )( )

( ) ( )

( ) ( ) kmd

tttrd

jitttr

tjijittr

tvrttrhrt

meetmeetdockchild

meetmeetdockchild

meetmeetdockchild

meetdockchilddockchildmeetdockchild

meet

26.26.01037.01.35.2

6.01.35.2)(

ˆ6.0ˆ1.35.2)(

ˆ)0(ˆ)1.3(ˆ6.0ˆ5.2)(

)(1037.0

22

22,

,

,

,,, 0

=+×+−=

+×+−===

+×+−==

×+++−==

×+===

N

E

dockchildv ,

ij

boatchildv ,

Dock Frame0,dockchildr -2.5i,0.6j )(, meetdockchild ttr =

)(, meetdockchild ttrd ==

deg4.166

2333.01037.08.24

6.08.24

6.0sin

9721.01037.08.245.2

8.245.2cos

=

=

−=×−

−=

θ

θ

θ

meet

meet

t

t

jiv riverboatˆ)786.5(ˆ108.24, +−=

Mechanics Lecture 3, Slide 51

Page 52: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue-child frame

jir

tvrtrjivtv

jivv

jivv

jiv

jivv

childdock

childdockchilddockchilddock

riverboatboatchild

dockchildchilddock

dockriverdockchild

riverboat

childriverriverchild

ˆ6.0ˆ5.2

)(

ˆ)sin*8.24(ˆ)cos*8.24()(

ˆ)0(ˆ)1.3(

ˆ)0(ˆ)1.3(

ˆ)sin*8.24(ˆ)cos*8.24(

ˆ0ˆ0

0

0

,

,,,

,,

,,

,,

,

,,

−=

×+=

−+−=−=

+−=−=

+==

+=

+==

θθ

θθ

N

Echilddockv , i

j

childboatv ,

Child Frame

0,childdockr 2.5i,-0.6j

)(, meetchilddock ttr =

θ

Mechanics Lecture 3, Slide 52

Page 53: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue-child frame( )

( )

( ) ( ) hrttt

tt

tt

jittr

tjijittr

tvrtvrtr

tjijitvrttr

meetmeetmeet

meetmeet

meetmeet

meetboatchild

meetmeetchildboat

riverboatchilddockchildboatchildboatchildboat

meetmeetchilddockchilddockmeetchilddock

1037.06.05.28.24

118.24

6.08.24

5.2

8.246.0sin0sin*8.246.0

8.245.2cos0cos*8.245.2

ˆ0ˆ0)(

ˆ)sin*8.24(ˆ)cos*8.24(ˆ6.0ˆ5.2)(

)(

ˆ)0(ˆ)1.3(ˆ6.0ˆ5.2)(

2222

,

,

,,,,,

,,,

00

0

=+−=⇒=

×

+

×

×=⇒=×+−

×−

=⇒=×+

+==

×++−==

×+=×+=

×+−+−=×+==

θθ

θθ

θθ

N

Echilddockv , i

j

childboatv ,

Child Frame

0,childdockr 2.5i,-0.6j

)(, meetchilddock ttr =

θ

Mechanics Lecture 3, Slide 53

Page 54: Relative and Circular Motion - AstronomyRelative and Circular Motion a) Relative motion b) Centripetal acceleration Mechanics Lecture 3, Slide 1. Mechanics Lecture 3, Slide 2. Time

River Rescue( )

( )

( ) ( )

( ) ( ) kmd

tttrd

jitttr

hrt

tjijitvrttr

meetmeetchilddock

meetmeetchilddock

meet

meetmeetchilddockchilddockmeetchilddock

26.26.01037.01.35.2

6.01.35.2)(

ˆ6.0ˆ1.35.2)(

1037.0

ˆ)0(ˆ)1.3(ˆ6.0ˆ5.2)(

22

22,

,

,,, 0

=−+×−=

−+×−===

−×−==

=

×+−+−=×+==

deg4.166

2333.01037.08.24

6.08.24

6.0sin

9721.01037.08.245.2

8.245.2cos

=

=

−=×−

−=

θ

θ

θ

meet

meet

t

t

Mechanics Lecture 3, Slide 54