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Physics 111: Lecture 3, Pg 1 Physics 111: Lecture 3 Today’s Agenda Reference frames and relative motion Uniform Circular Motion
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Physics 111: Lecture 3 Today’s Agenda

Feb 23, 2016

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Physics 111: Lecture 3 Today’s Agenda. Reference frames and relative motion Uniform Circular Motion. Inertial Reference Frames:. Cart on track on track. A Reference Frame is the place you measure from. It’s where you nail down your (x,y,z) axes! - PowerPoint PPT Presentation
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Page 1: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 1

Physics 111: Lecture 3

Today’s Agenda

Reference frames and relative motion

Uniform Circular Motion

Page 2: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 2

Inertial Reference Frames:

A Reference Frame is the place you measure from. It’s where you nail down your (x,y,z) axes!

An Inertial Reference Frame (IRF) is one that is not accelerating. We will consider only IRFs in this course.

Valid IRFs can have fixed velocities with respect to each other. More about this later when we discuss forces. For now, just remember that we can make measurements

from different vantage points.

Cart ontrack on

track

Page 3: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 3

Relative Motion Consider a problem with two distinct IRFs:

An airplane flying on a windy day.

A pilot wants to fly from Champaign to Chicago. Having asked a friendly physics student, she knows that Chicago is 120 miles due north of Urbana. She takes off from Willard Airport at noon. Her plane has a compass and an air-speed indicator to help her navigate.

The compass allows her to keep the nose of the plane pointing north.

The air-speed indicator tells her that she is traveling at 120 miles per hour with respect to the air.

Page 4: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 4

Relative Motion...

The plane is moving north in the IRF attached to the air: Vp, a is the velocity of the plane w.r.t. the air.

Air

Vp,a

Page 5: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 5

Relative Motion... But suppose the air is moving east in the IRF attached to

the ground. Va,g is the velocity of the air w.r.t. the ground (i.e. wind).

Va,g

Air

Vp,a

Page 6: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 6

Relative Motion...

What is the velocity of the plane in an IRF attached to the ground? Vp,g is the velocity of the plane w.r.t. the ground.

Vp,g

Page 7: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 7

Relative Motion...

Vp,g = Vp,a + Va,g Is a vector equation relating the airplane’s velocity in different reference frames.

Vp,g

Va,g

Vp,a

Tractor

Page 8: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 8

Lecture 3, Act 1Relative Motion

You are swimming across a 50m wide river in which the current moves at 1 m/s with respect to the shore. Your swimming speed is 2 m/s with respect to the water. You swim across in such a way that your path is a straight perpendicular line across the river.How many seconds does it take you to get across ?

(a)

(b)

(c)

50 3 29

2 m/s

1 m/s50 m

35250

50150

Page 9: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 9

Lecture 3, Act 1solution

The time taken to swim straight across is (distance across) / (vy )

Choose x axis along riverbank and y axis across rivery

x

Since you swim straight across, you must be tilted in the water so thatyour x component of velocity with respect to the water exactly cancels the velocity of the water in the x direction:

2 m/s 1m/sy

x

1 m/s

2 13

2 2

m/s

Page 10: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 10

Lecture 3, Act 1solution

So the y component of your velocity with respect to the water is

So the time to get across is

y

x

3m/s

503

29mm s

s

50 m

3m/s

Page 11: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 11

Uniform Circular Motion

What does it mean?

How do we describe it?

What can we learn about it?

Page 12: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 12

What is UCM?

Motion in a circle with: Constant Radius R

Constant Speed v = |v|

R

v

x

y

(x,y)

Puck on ice

Page 13: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 13

How can we describe UCM?

In general, one coordinate system is as good as any other: Cartesian:

» (x,y) [position]» (vx ,vy) [velocity]

Polar:» (R,) [position]» (vR ,) [velocity]

In UCM: R is constant (hence vR = 0). (angular velocity) is constant. Polar coordinates are a natural way to describe UCM!

R

v

x

y

(x,y)

Page 14: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 14

Polar Coordinates: The arc length s (distance along the circumference) is

related to the angle in a simple way: s = R, where is the angular displacement. units of are called radians.

For one complete revolution:2R = Rc

c = 2

has period 2.

1 revolution = 2radians

R

v

x

y

(x,y)s

Page 15: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 15

Polar Coordinates...

x = R cos y = R sin

/2 3/2 2

-1

1

0

sincos

R

x

y

(x,y)

Page 16: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 16

Polar Coordinates...

In Cartesian coordinates, we say velocity dx/dt = v. x = vt

In polar coordinates, angular velocity d/dt = . = t has units of radians/second.

Displacement s = vt. but s = R = Rt, so: R

v

x

y

st

v = R

Tetherball

Page 17: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 17

Period and Frequency

Recall that 1 revolution = 2 radiansfrequency (f) = revolutions / second (a)angular velocity () = radians / second (b)

By combining (a) and (b) = 2 f

Realize that:period (T) = seconds / revolutionSo T = 1 / f = 2/

R

v

s

= 2 / T = 2f

Page 18: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 18

Recap:

R

v

st

(x,y)

x = R cos()= R cos(t)y = R sin()= R sin(t) = arctan (y/x)

= ts = v ts = R = Rt

v = R

Page 19: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 19

Aside: Polar Unit Vectors

We are familiar with the Cartesian unit vectors: i j k

Now introduce“polar unit-vectors” r and :r points in radial direction points in tangential direction

R

x

y

i

j

r̂ ̂

^ ^^^

(counter clockwise)

Page 20: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 20

Acceleration in UCM:

Even though the speed is constant, velocity is not constant since the direction is changing: must be some acceleration! Consider average acceleration in time t aav = v / t

v2

tv1

v1v2

v

R

Page 21: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 21

Acceleration in UCM:

seems like v (hence v/t )points at the origin!

R

Even though the speed is constant, velocity is not constant since the direction is changing. Consider average acceleration in time t aav = v / t

v

Page 22: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 22

Acceleration in UCM:

Even though the speed is constant, velocity is not constant since the direction is changing. As we shrink t, v / t dv / dt = a

a = dv / dt

We see that a points in the - R direction.

R

Page 23: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 23

Acceleration in UCM:

This is called Centripetal Acceleration. Now let’s calculate the magnitude:

v2

v1

v1v2

v

RR

vv

RR

Similar triangles:

But R = vt for small t

So: vt

vR

2 v

vv tR

a vR

2

Page 24: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 24

Centripetal Acceleration

UCM results in acceleration:Magnitude: a = v2 / RDirection: - r (toward center of circle)

Ra

^

Page 25: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 25

Derivation:

RRa

2

We know that and v = R

Substituting for v we find that:

a vR

2

a = 2R

Page 26: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 26

Lecture 3, Act 2Uniform Circular Motion

A fighter pilot flying in a circular turn will pass out if the centripetal acceleration he experiences is more than about 9 times the acceleration of gravity g. If his F18 is moving with a speed of 300 m/s, what is the approximate diameter of the tightest turn this pilot can make and survive to tell about it ?

(a) 500 m(b) 1000 m(c) 2000 m

Page 27: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 27

Lecture 3, Act 2Solution

a vR

g 2

9

2

2

2

2

sm8199

sm90000

g9vR

.

m1000m819

10000R .

D R m 2 2000

2km

Page 28: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 28

Example: Propeller Tip

The propeller on a stunt plane spins with frequency f = 3500 rpm. The length of each propeller blade is L = 80cm. What centripetal acceleration does a point at the tip of a propeller blade feel?

f

L

what is a here?

Page 29: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 29

Example:

First calculate the angular velocity of the propeller:

so 3500 rpm means = 367 s-1

Now calculate the acceleration. a = 2R = (367s-1)2 x (0.8m) = 1.1 x 105 m/s2

= 11,000 g

direction of a points at the propeller hub (-r ).

1 1 160

2 0105 0105 rpm s-1 rot x

sx rad

rotradsmin

min . .

^

Page 30: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 30

Example: Newton & the Moon

What is the acceleration of the Moon due to its motion around the Earth?

What we know (Newton knew this also):T = 27.3 days = 2.36 x 106 s (period ~ 1 month)R = 3.84 x 108 m (distance to

moon)RE = 6.35 x 106 m (radius of

earth)

R RE

Page 31: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 31

Moon...

Calculate angular velocity:

So = 2.66 x 10-6 s-1.

Now calculate the acceleration. a = 2R = 0.00272 m/s2 = 0.000278 gdirection of a points at the center of the Earth (-r ).

127 3

186400

2 2 66 10 6.

.rotday

x days

x radrot

x s-1

^

Page 32: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 32

Moon... So we find that amoon / g = 0.000278 Newton noticed that RE

2 / R2 = 0.000273

This inspired him to propose that FMm 1 / R2

(more on gravity later)

R RE

amoon g

Page 33: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 33

Lecture 3, Act 3Centripetal Acceleration

The Space Shuttle is in Low Earth Orbit (LEO) about 300 km above the surface. The period of the orbit is about 91 min. What is the acceleration of an astronaut in the Shuttle in the reference frame of the Earth? (The radius of the Earth is 6.4 x 106 m.)

(a) 0 m/s2

(b) 8.9 m/s2

(c) 9.8 m/s2

Page 34: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 34

First calculate the angular frequency :

Realize that:

Lecture 3, Act 3Centripetal Acceleration

RO

300 kmRO = RE + 300 km = 6.4 x 106 m + 0.3 x 106 m = 6.7 x 106 m

RE

1-s 00115.0 rotrad2 x

s601 xrot

911 min

min

Page 35: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 35

Now calculate the acceleration:

Lecture 3, Act 3Centripetal Acceleration

a = 2R

a = (0.00115 s-1)2 x 6.7 x 106 m

a = 8.9 m/s2

Page 36: Physics 111: Lecture 3 Today’s Agenda

Physics 111: Lecture 3, Pg 36

Recap for today:

Reference frames and relative motion. (Text: 2-1, 3-3, & 4-1)

Uniform Circular Motion (Text: 5-2, also 9-1)

Look at Textbook problems Chapter 3: # 47, 49, 97, 105