Physics 8 Wednesday, November 9, 2011

Similar documents
Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

Copyright 2010 Pearson Education, Inc. GRAVITY. Chapter 12

Chapter 13. Gravitation. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow

Preview. Circular Motion and Gravitation Section 1. Section 1 Circular Motion. Section 2 Newton s Law of Universal Gravitation

Rotation Quiz II, review part A

PHYSICS. Chapter 13 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT Pearson Education, Inc.

Practice Problems from Chapters 11-13, for Midterm 2. Physics 11a Fall 2010

Physics 8 Friday, November 4, 2011

PSI AP Physics 1 Gravitation

Preview. Circular Motion and Gravitation Section 1. Section 1 Circular Motion. Section 2 Newton s Law of Universal Gravitation

Lecture 16. Gravitation

Outline for Today: Newton s Law of Universal Gravitation The Gravitational Field Orbital Motion Gravitational Potential Energy. Hello!

Gravitation and Newton s Synthesis

PHYSICS 12 NAME: Gravitation

Comments about HW #1 Sunset observations: Pick a convenient spot (your dorm?) Try to get 1 data point per week Keep a lab notebook with date, time,

Chapter 8, Rotational Equilibrium and Rotational Dynamics. 3. If a net torque is applied to an object, that object will experience:

Copyright 2008 Pearson Education, Inc., publishing as Pearson Addison-Wesley.

Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

PHYSICS 221 SPRING EXAM 2: March 30, 2017; 8:15pm 10:15pm

Physics 8 Wednesday, October 14, 2015

More examples: Summary of previous lecture

CIRCULAR MOTION AND UNIVERSAL GRAVITATION

Downloaded from

Chapter: The Laws of Motion

AP practice ch 7-8 Multiple Choice

The Moon does not fall to Earth because

= v = 2πr. = mv2 r. = v2 r. F g. a c. F c. Text: Chapter 12 Chapter 13. Chapter 13. Think and Explain: Think and Solve:

End-of-Chapter Exercises

Planetary Mechanics:

Outline for Today: Newton s Law of Universal Gravitation The Gravitational Field Orbital Motion Gravitational Potential Energy

FIFTH MIDTERM -- REVIEW PROBLEMS

The Force of Gravity exists between any two masses! Always attractive do you feel the attraction? Slide 6-35

Please turn on your clickers

PH201 Chapter 6 Solutions

Unit 2: Forces Chapter 6: Systems in Motion

Physics 111. Tuesday, November 9, Universal Law Potential Energy Kepler s Laws. density hydrostatic equilibrium Pascal s Principle

Gravitation & Kepler s Laws

Circular Motion & Gravitation MC Question Database

UNIVERSITY OF MANITOBA. All questions are of equal value. No marks are subtracted for wrong answers.

Chapter 4. Forces and Newton s Laws of Motion. continued

General Physics I Spring Applying Newton s Laws

Lecture Outline. Chapter 13 Gravity Pearson Education, Inc. Slide 13-1

Algebra Based Physics Newton's Law of Universal Gravitation

Review PHYS114 Chapters 4-7

Honors Assignment - Circular and Periodic Motion

Conceptual Physics Fundamentals

Ph1a: Solution to the Final Exam Alejandro Jenkins, Fall 2004

Advanced Higher Physics. Rotational motion

Exam 3 PREP Chapters 6, 7, 8

Gravitation and Newton s Synthesis

Assignment - Periodic Motion. Reading: Giancoli, Chapter 5 Holt, Chapter 7. Objectives/HW:

Episode 403: Orbital motion

PH 2213 : Chapter 06 Homework Solutions. Problem 6.08 :

Circular Motion and Gravitation. Centripetal Acceleration

CH 8. Universal Gravitation Planetary and Satellite Motion

Central Force Particle Model

Physics 53 Exam 3 November 3, 2010 Dr. Alward

Physics 8 Wednesday, October 11, 2017

AP Physics II Summer Packet

Chapter 2. Force and Newton s Laws

Chapter 3 Celestial Sphere Movie

Physics 8, Fall 2011, Homework #12. Due in 1W12 DRL by 5pm, Friday, December 9, 2011

Physics General Physics. Lecture 8 Planetary Motion. Fall 2016 Semester Prof. Matthew Jones

1 The displacement, s in metres, of an object after a time, t in seconds, is given by s = 90t 4 t 2

PHY2020 Practice Problems Fall 2015

Chapter 5 Part 2. Newton s Law of Universal Gravitation, Satellites, and Weightlessness

Chapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Orbits. Objectives. Orbits and unbalanced forces. Equations 4/7/14

UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics

CH 10: PRESSURE, GRAVITY AND MOMENTS

Newton s Third Law of Motion Newton s Law of Gravitation Buoyancy Momentum. 3-2 Section 3.4

P - f = m a x. Now, if the box is already moving, for the frictional force, we use

PHYS 1303 Final Exam Example Questions

Circular Motion and Gravitation. Centripetal Acceleration

Key Points: Learn the relationship between gravitational attractive force, mass and distance. Understand that gravity can act as a centripetal force.

Gravity and Orbits. Objectives. Clarify a number of basic concepts. Gravity

GRAVITATIONAL FORCE NEAR EARTH

Angular Motion Unit Exam Practice

INTRODUCTION: Ptolemy geo-centric theory Nicolas Copernicus Helio-centric theory TychoBrahe Johannes Kepler

ASTRONAUT PUSHES SPACECRAFT

Chapter 13: universal gravitation

CIRCULAR MOTION AND SHM : Higher Level Long Questions.

Chapter 7. Preview. Objectives Tangential Speed Centripetal Acceleration Centripetal Force Describing a Rotating System. Section 1 Circular Motion

Force Test Review. 1. Give two ways to increase acceleration. You can increase acceleration by decreasing mass or increasing force.

3. A bicycle tire of radius 0.33 m and a mass 1.5 kg is rotating at 98.7 rad/s. What torque is necessary to stop the tire in 2.0 s?

Kepler s first law (law of elliptical orbit):- A planet moves round the sun in an elliptical orbit with sun situated at one of its foci.

PC 1141 : AY 2012 /13

Midterm 3 Thursday April 13th

Physics Exam 1 Formulas

Energy and Angular Momentum

Chapter 13 Gravity Pearson Education, Inc. Slide 13-1

Physics. Student Materials Advanced Higher. Tutorial Problems Mechanics HIGHER STILL. Spring 2000

ΣF=ma SECOND LAW. Make a freebody diagram for EVERY problem!

Honors Physics Final Exam Review. Symbol Units Units (if applicable)

Circular Motion and Gravitation Practice Test Provincial Questions

Hint 1. The direction of acceleration can be determined from Newton's second law

Name: Date: 5. A 5.0-kg ball and a 10.0-kg ball approach each other with equal speeds of 20 m/s. If

Multiple Choice Portion

PHYSICS 221 Fall 2016 EXAM 2: November 02, :15pm 10:15pm. Name (printed): Recitation Instructor: Section #:

In this chapter, you will consider the force of gravity:

Transcription:

Physics 8 Wednesday, November 9, 2011 For HW8 problems to sketch out in class, I got 5 requests for # 9 3 requests for # 3 2 requests for # 14 1 request each for # 2, 7, 10, 11, 15, 19 I will be in DRL 3W2 at 7pm both Wed and Thu this week. Next week Zoey will do both days.

People also asked about rolling motion in ch12 A 215 g can of soup is 10.8 cm tall and has a radius of 3.19 cm. (a) Calculate its theoretical rotational inertia, assuming it to be a solid cylinder. (b) When it is released from rest at the top of a ramp that is 3.00 m long and makes an angle of 25 with the horizontal, it reaches the bottom in 1.40 s. What is the experimental rotational inertia? (c) Compare the experimental and theoretical rotational inertias and suggest possible sources of the difference.

People also asked about rolling motion in ch12 A 215 g can of soup is 10.8 cm tall and has a radius of 3.19 cm. (a) Calculate its theoretical rotational inertia, assuming it to be a solid cylinder. (b) When it is released from rest at the top of a ramp that is 3.00 m long and makes an angle of 25 with the horizontal, it reaches the bottom in 1.40 s. What is the experimental rotational inertia? (c) Compare the experimental and theoretical rotational inertias and suggest possible sources of the difference. One constant-acceleration trick that you may not have seen: if you solve x f = 1 2 at2 for a and then plug a = 2x f into v 2 t 2 f = 2ax f, you get (for v i = 0, x i = 0, a = constant): ( ) vf 2 2xf = 2 t 2 x f = 4x f 2 t 2 Now use energy conservation to relate I to v 2 f...

9. Archimedes screw, one of the first mechanical devices for lifting water, consists of a very large screw surrounded by a hollow, tight-fitting shaft (shown below). The bottom end of the device is placed in a pool of water. As the screw is turned, water is carried up along its ridges and comes out the top of the shaft and into a storage tank. As the handle is turned, work done by the torque exerted on the handle is converted to gravitational potential energy of the water-earth system. Let s say you want to take a shower using this device. You figure your shower will consume 44 liters of water, and so you have to raise this amount to the storage tank 2.5 m above the pool, so it can fall down on you. When you turn the handle, you apply a torque of 12 N m. How many times must you turn the handle?

Problem 3. A 35 kg child stands on the edge of a 400 kg playground merry-go-round that is turning at the rate of 1 rev every 2.2 s. She then walks to the center of the platform. If the radius of the platform is 1.5 m, what is its rotational speed once the child arrives at the center?

I got two requests for #14 A square clock of inertia M = 5.0 kg is hung on a nail driven in a wall, as shown at right. The length of each side of the square is l = 20 cm, the thickness is w = 10 cm, and the clock is a distance d = 0.1 cm from the wall at the top, where it hangs on the nail. Assume that the surface of the wall is very smooth and that the center of mass of the clock corresponds to its geometric center. What is the magnitude of the normal force exerted by the wall on the clock? Make simplifying approximations any answer within 10% of the correct answer gets full credit.

Chapter 13 gravity If the density of all the planets were the same, how would the surface acceleration of gravity on each planet depend on its radius? (A) (B) a = GM R 2 so the acceleration would be proportional to 1/R 2 a = G(4 3 πr3 ρ) R 2 so the acceleration would be proportional to R

g = (4π/3)(density)G R The surface gravity of a planet or with a given mass will be approximately inversely proportional to the square of its radius, and the surface gravity of a planet or star with a given average density will be approximately proportional to its radius. Acceleration due to gravity is shown through the equation g = GM/R 2. On different scales the mass is proportional to its radius cubed. When this is plugged back into the first equation, g R. Surface acceleration of gravity and the planet s radius are directly related (for constant density). Given that volume is proportional to the radius cubed, which implies that mass is proportional to the radius cubed if the density is uniform, then the acceleration of gravity will be given by g R directly proportional to the radius of the planet.

Chapter 13 gravity An astronaut on the international space station gently releases a satellite that has a gravitational mass much less than that of the station. Describe the behavior of the satellite after release. (A) The satellite goes into orbit around the space station (B) The satellite will float along with the astronaut and everything else in the space station (C) The satellite is pulled back toward the station s center of mass by the small force of gravity between the station and the satellite (D) There would be a small gravitational pull between the station and the satellite, but this pull is so small that even if the astronaut is pretty careful, the relative speed of the satellite and station will still exceed the escape velocity, and the satellite will slowly drift away.

Chapter 13 gravity The satellite is only subject to the force of Earth s gravity, so it experiences weightlessness and just floats. It would tend to follow in the same trajectory of the space station and continue to orbit. The satellite will float along with the astronaut and everything else in the space station. The object is essentially in free fall, experiencing weightlessness. If the satellite with much less gravitational mass is released outside of the international space station, I believe it would begin to orbit the planet it was near, if any. Because every piece of matter attracts another piece of matter according to Newton s law of gravity, the satellite would have to interact with the gravitational pulls of the nearest planet. The satellite will orbit around the space station in an elliptical manner. The space station will be at one of the foci of this ellipse.

Chapter 13 gravity The International Space Station is in low-earth orbit, about 400 km above the earth s surface. Earth s radius is about 6400 km. The gravitational acceleration toward the center of the earth at this altitude is G M earth (6800 km) 2 = (6.67 10 11 N m2 )(6.0 10 24 kg) kg 2 (6.8 10 6 m) 2 = 8.7 m s 2 By comparison, gravitational acceleration toward (500,000 kg) ISS of a nearby satellite (say 10 m away) is (6.67 10 11 N m2 kg 2 )(5 10 5 kg) (10 m) 2 = 3 10 7 m s 2 So attraction between satellite and ISS is more than 10 million times smaller than attraction between satellite and earth.

Plugging in numbers, it looks as if satellite would take about 2 hours to fall 10 m back to ISS, or if released at the right relative velocity, it could orbit the ISS with a period of about 10 hours. So on a time scale of minutes, the satellite would just sit there next to the space station. On a time scale of hours, it looks as if it could be very slowly accelerated toward the space station s center of mass. (I wouldn t have guessed this.) If you gave it precisely the right push w.r.t. the space station, it may be conceivable that the satellite would very slowly orbit the space station, going around a couple of times a day. But I think in reality it would be very difficult not to give the satellite some nonzero initial velocity w.r.t. the space station, e.g. at least 0.001 m/s, so it would drift out of reach of the space station s gravity.

Note that the time that it takes both the space station and the satellite (in an orbit 400 km above earth s surface) to go around the earth is only about R 2π = 1.5 hours a

What is the acceleration due to gravity at a distance of one earth radius above earth s surface? (A) g/4 (B) g/2 (C) g (D) 2g (E) 4g where g is our old friend 9.8 m/s 2.

What is the acceleration due to gravity at a distance of one earth radius above earth s surface? a = GM earth (2R earth ) 2 = (6.67 10 11 N m2 kg 2 )(6.0 10 24 kg) (2 6.4 10 6 m) 2 = 2.44 m s 2 or more simply a = g/4 = 2.45 m/s 2