Loading in 5 sec....

PHY 113 C General Physics I 11 AM – 12:15 PM TR Olin 101 Plan for Lecture 17: Review of Chapters 9-13, 15-16 Comment on exam and advice for preparationPowerPoint Presentation

PHY 113 C General Physics I 11 AM – 12:15 PM TR Olin 101 Plan for Lecture 17: Review of Chapters 9-13, 15-16 Comment on exam and advice for preparation

Download Presentation

PHY 113 C General Physics I 11 AM – 12:15 PM TR Olin 101 Plan for Lecture 17: Review of Chapters 9-13, 15-16 Comment on exam and advice for preparation

Loading in 2 Seconds...

- 472 Views
- Uploaded on
- Presentation posted in: General

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.

- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -

PHY 113 C General Physics I

11 AM – 12:15 PM TR Olin 101

Plan for Lecture 17:

Review of Chapters 9-13, 15-16

Comment on exam and advice for preparation

Review

Example problems

PHY 113 C Fall 2013 -- Lecture 17

PHY 113 C Fall 2013 -- Lecture 17

Webassign questions – Assignment #15

Consider the sinusoidal wave of the figure below with the wave function y = 0.150 cos(15.7x − 50.3t)

where x and y are in meters and t is in seconds. At a certain instant, let point A be at the origin and point B be the closest point to A along the x axis where the wave is 43.0° out of phase with A. What is the coordinate of B?

PHY 113 C Fall 2013 -- Lecture 17

Webassign questions – Assignment #15

A transverse wave on a string is described by the following wave function. y = 0.115 sin ((π/9)x+ 5πt)

where x and y are in meters and t is in seconds.

Determine the transverse speed at t = 0.150 s for an element of the string located at x = 1.50 m.

(b) Determine the transverse acceleration at t = 0.150 s for an element of the string located at x = 1.50 m.

PHY 113 C Fall 2013 -- Lecture 17

Webassign questions – Assignment #15

A sinusoidal wave in a rope is described by the wave function

y= 0.20 sin (0.69πx + 20πt)

where x and y are in meters and t is in seconds. The rope has a linear mass density of 0.230 kg/m. The tension in the rope is provided by an arrangement like the one illustrated in the figure below. What is the mass of the suspended object?

T

mg

PHY 113 C Fall 2013 -- Lecture 17

Comment about exam on Tuesday 10/29/2013

PHY 113 C Fall 2013 -- Lecture 17

- iclicker question
- What is the purpose of exams?
- Pure pain and suffering for all involved.
- To measure what has been learned.
- To help students learn the material.
- Other.

PHY 113 C Fall 2013 -- Lecture 17

- Advice on how to prepare for the exam
- Review lecture notes and text chapters 9-13,15-16
- Prepare equation sheet
- Work practice problems

- Topics covered
- Linear momentum
- Rotational motion and angular momentum
- Gravitational force and circular orbits
- Static equilibrium
- Simple harmonic motion
- Wave motion

PHY 113 C Fall 2013 -- Lecture 17

- What to bring to exam:
- Clear head
- Calculator
- Equation sheet
- Pencil or pen

PHY 113 C Fall 2013 -- Lecture 17

iclicker question:

Have you looked at last year’s exams?

A. Yes B. No

PHY 113 C Fall 2013 -- Lecture 17

- Linear momentum
- What is it?
- When is it “conserved”?
- Conservation of momentum in analysis of collisions
- Notion of center of mass

PHY 113 C Fall 2013 -- Lecture 17

Linear momentum -- continued

Physics of composite systems

PHY 113 C Fall 2013 -- Lecture 17

Example – completely inelastic collision; balls moving in one dimension on a frictionless surface

PHY 113 C Fall 2013 -- Lecture 17

Examples of two-dimensional collision; balls moving on a frictionless surface

PHY 113 C Fall 2013 -- Lecture 17

The notion of the center of mass and the physics of composite systems

PHY 113 C Fall 2013 -- Lecture 17

Finding the center of mass

PHY 113 C Fall 2013 -- Lecture 17

- Rotational motion and angular momentum
- Angular variables
- Newton’s law for angular motion
- Rotational energy
- Moment of inertia
- Angular momentum

q

PHY 113 C Fall 2013 -- Lecture 17

Review of rotational energy associated with a rigid body

PHY 113 C Fall 2013 -- Lecture 17

Moment of inertia:

PHY 113 C Fall 2013 -- Lecture 17

CM

CM

PHY 113 C Fall 2013 -- Lecture 17

iclicker exercise:

Three round balls, each having a mass M and radius R, start from rest at the top of the incline. After they are released, they roll without slipping down the incline. Which ball will reach the bottom first?

C

B

A

PHY 113 C Fall 2013 -- Lecture 17

q

How can you make objects rotate?

Define torque:

t = r x F

t = rF sin q

r

F sin q

q

F

PHY 113 C Fall 2013 -- Lecture 17

Example form Webassign #11

- iclicker exercise
- When the pivot point is O, which torque is zero?
- A. t1?
- B. t2?
- C. t3?

t3

X

t2

t1

PHY 113 C Fall 2013 -- Lecture 17

Vector cross product; right hand rule

PHY 113 C Fall 2013 -- Lecture 17

From Newton’s second law – continued – conservation of angular momentum:

PHY 113 C Fall 2013 -- Lecture 17

Example of conservation of angular momentum

PHY 113 C Fall 2013 -- Lecture 17

Summary – conservation laws we have studied so far

PHY 113 C Fall 2013 -- Lecture 17

- Fundamental gravitational force law and planetary motion
- Newton’s gravitational force law
- Gravity at Earth’s surface
- Circular orbits of gravitational bodies
- Energy associated with gravitation and orbital motion

PHY 113 C Fall 2013 -- Lecture 17

Universal law of gravitation

Newton (with help from Galileo, Kepler, etc.) 1687

PHY 113 C Fall 2013 -- Lecture 17

Gravitational force of the Earth

RE

m

Note: Earth’s gravity acts as a point mass located at the Earth’s center.

PHY 113 C Fall 2013 -- Lecture 17

REM

F

Stable circular orbit of two gravitationally attracted objects (such as the moon and the Earth)

v

a

PHY 113 C Fall 2013 -- Lecture 17

m2

R2

R1

m1

Circular orbital motion about center of mass

v2

CM

v1

PHY 113 C Fall 2013 -- Lecture 17

m2

R2

R1

m1

v2

L1=m1v1R1

L2=m2v2R2

L = L1 + L2

v1

Note: More generally, stable orbits can be elliptical.

PHY 113 C Fall 2013 -- Lecture 17

Gravitational potential energy

Example:

PHY 113 C Fall 2013 -- Lecture 17

Analysis of static equilibrium

Meanwhile – back on the surface of the Earth:

Conditions for stable equilibrium

PHY 113 C Fall 2013 -- Lecture 17

PHY 113 C Fall 2013 -- Lecture 17

X

**

T

Mg

mg

PHY 113 C Fall 2013 -- Lecture 17

Some practice problems

PHY 113 C Fall 2013 -- Lecture 17

PHY 113 C Fall 2013 -- Lecture 17

From webassign:

A 100-kg merry-go-round in the shape of a uniform, solid, horizontal disk of radius 1.50 m is set in motion by wrapping a rope about the rim of the disk and pulling on the rope. What constant force would have to be exerted on the rope to bring the merry-go-round from rest to an angular speed of 0.800 rev/s in 2.00 s? (State the magnitude of the force.)

view from top:

F

R

PHY 113 C Fall 2013 -- Lecture 17

From webassign:

A 10.3-kg monkey climbs a uniform ladder with weight w = 1.24 102 N and length L = 3.35 m as shown in the figure below. The ladder rests against the wall and makes an angle of θ = 60.0° with the ground. The upper and lower ends of the ladder rest on frictionless surfaces. The lower end is connected to the wall by a horizontal rope that is frayed and can support a maximum tension of only 80.0 N.

PHY 113 C Fall 2013 -- Lecture 17