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MS101: Physics Chapter 5 Dr. Ahmed Amin Hussein [email protected] 2013-2014 Wednesday, August 17, 2022 Prepared By: Dr. Ahmed Amin 1

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Page 1: 05Physics_lecture_29 Mar 2014

MS101: Physics

Chapter 5Dr. Ahmed Amin Hussein

[email protected]

May 3, 2023 Prepared By: Dr. Ahmed Amin 1

Page 2: 05Physics_lecture_29 Mar 2014

Chapter 5: Circular Motion

May 3, 2023 2Prepared By: Dr. Ahmed Amin

Uniform Circular Motion Radial Acceleration Banked and Unbanked Curves Circular Orbits Non-uniform Circular Motion Tangential and Angular

Acceleration Artificial Gravity

Page 3: 05Physics_lecture_29 Mar 2014

§5.1 Uniform Circular Motion

May 3, 2023 3Prepared By: Dr. Ahmed Amin

is the angular position.

Angular displacement:

if

Note: angles measured CW are negative and angles measured CCW are positive. is measured in radians.

2 radians = 360 = 1 revolution

x

y

i

f

Page 4: 05Physics_lecture_29 Mar 2014

May 3, 2023 4Prepared By: Dr. Ahmed Amin

The average and instantaneous angular velocities are:

tt t

0av lim and

is measured in rads/sec.

Page 5: 05Physics_lecture_29 Mar 2014

May 3, 2023 5Prepared By: Dr. Ahmed Amin

x

y

i

f

r

arclength = s = r

rs

is a ratio of two lengths; it is a dimensionless ratio!

Page 6: 05Physics_lecture_29 Mar 2014

May 3, 2023 6Prepared By: Dr. Ahmed Amin

An object moves along a circular path of radius r; what is its average speed?

avav timetotaldistance total r

tr

trv

Also, rv (instantaneous values).

x

y

i

f

r

Page 7: 05Physics_lecture_29 Mar 2014

May 3, 2023 7Prepared By: Dr. Ahmed Amin

The time it takes to go one time around a closed path is called the period (T).

Trv 2

timetotaldistance total

av

Comparing to v = r: fT

22

f is called the frequency, the number of revolutions (or cycles) per second.

Page 8: 05Physics_lecture_29 Mar 2014

§5.4 Circular Orbits

May 3, 2023 8Prepared By: Dr. Ahmed Amin

rvmam

rMGmFF srs

esg

2

2

Consider an object of mass m in a circular orbit about the Earth.

Earth

r

The only force on the satellite is the force of gravity:

rGMv

rvm

rMGm

e

ses

2

2Solve for the speed of the satellite:

Page 9: 05Physics_lecture_29 Mar 2014

May 3, 2023 9Prepared By: Dr. Ahmed Amin

How high above the surface of the Earth does a satellite need to be so that it has an orbit period of 24 hours?

rGMv eFrom previous slide: Also need,

Trv 2

Combine these expressions and solve for r:3

12

24

TGMr e

m 10225.4

s 864004

kg 1098.5/kgNm1067.6

7

31

22

242211

r

km 000,35 ee RrhhRr

Example

Page 10: 05Physics_lecture_29 Mar 2014

May 3, 2023 10Prepared By: Dr. Ahmed Amin

31

224

TGMr e

is Kepler’s Third Law.

It can be generalized to:3

1

224

TGMr

Where M is the mass of the central body. For example, it would be Msun if speaking of the planets in the solar system.

Page 11: 05Physics_lecture_29 Mar 2014

TMA Exercises

May 3, 2023 11Prepared By: Dr. Ahmed Amin

Problems :

Questions # # 5, 9, 13,

Additional questions

Questions # 31, 33, 35