Two satellites A and B of the same mass are going around Earth in concentric orbits. The distance of satellite B from Earth’s center is twice that of satellite.

Slides:



Advertisements
Similar presentations
THERMAL PHYSICS. Temperature and the zeroth Law of Thermodynamics 2 objects are in thermal contact if energy can be exchange between them 2 objects are.
Advertisements

Chapter 9 Thermal Energy
Physics for Scientists and Engineers, 6e
10. ConcepTest 5.8a Earth and Moon I
Force, Mass and Acceleration Newton’s Laws
Universal Gravitation
ConcepTest Clicker Questions
Physics: Principles with Applications, 6th edition
Answer each of these with your first instinct to the answer. You will have limited time to submit an answer. There will be a bit of discussion after most.
Explain why the Earth precesses and the consequences
Ch12-1 Newton’s Law of Universal Gravitation Chapter 12: Gravity F g = Gm 1 m 2 /r 2 G = 6.67 x Nm 2 /kg 2.
SMDEP Physics Gravity, Simple Harmonic Motion. Vote only on required HW problems Other problems will be worked out in TA sessions.
SMDEP Physics Gravity: Orbits, energy. Ch 6, #27 (b) only: mass of stars? 1.9x10 28 kg 2.9x10 26 kg 3.5x10 26 kg 4.5x10 24 kg 5.Other 6.Didn’t finish.
6. Centripetal force F = ma 1. Example: A stone of mass m sits at the bottom of a bucket. A string is attached to the bucket and the whole thing is made.
Two satellites A and B of the same mass are going around Earth in concentric orbits. The distance of satellite B from Earth’s center is twice that of satellite.
Newton’s Second Law of Motion Page Force and Acceleration Force is a push or a pull. Acceleration is when the motion of an object changes. Examples:
Isaac Newton’s 3rd Law and the Universal Law of Gravitation
Physical Science and You Chapter One: Studying Physics and Chemistry Chapter Two: Experiments and Variables Chapter Three: Key Concepts in Physical Science.
Energy, Heat and Heat Transfer
Earth and Moon I 1) the Earth pulls harder on the Moon
Motion and Force Chapter Twelve: Distance, Time, and Speed Chapter Thirteen: Forces Chapter Fourteen: Force and Motion.
Part 4 Newton’s Second Law of Motion Newton’s Second Law Acceleration is the rate at which your velocity (speed with direction) changes.
Universal Gravitation
Universal Gravitation Sir Isaac Newton: The Universal Law of Gravitation.
Thursday, October 11 Journal: Define gravity and inertia. Schedule: Gravity Notes Gravity Video Homework: None.
Gravity ISCI More Free Fall Free Fall Vertical and Horizontal Components of Free Fall.
©1997 by Eric Mazur Published by Pearson Prentice Hall Upper Saddle River, NJ ISBN No portion of the file may be distributed, transmitted.
Kepler’s first law of planetary motion says that the paths of the planets are A. Parabolas B. Hyperbolas C. Ellipses D. Circles Ans: C.
© 2012 Pearson Education, Inc. The mass of the Moon is 1/81 of the mass of the Earth. Compared to the gravitational force that the Earth exerts on the.
Kinetic Molecular Theory of Matter
Planetary Dynamics § 13.4–13.8. Closed Orbits U g + K tr = constant < 0 The closer the satellite is to the main body, the faster it moves Objects do not.
Unit 06 “ Circular Motion, Gravitation and Black Holes” Gravity in our Solar System.
Laws of Motion and Energy Chapter Seven: Gravity and Space 7.1 Gravity 7.2 The Solar System 7.3 The Sun and the Stars.
Centripetal Force and Acceleration
Isaac Newton and the Universal Law of Gravitation.
Review Question What are Kepler’s laws?. Review Question What are Newton’s laws?
Law of Universal Gravitation Chapter 12 November 9/10.
Chapter 10 Thermal Physics 1. Temperature and the zeroth Law of Thermodynamics 2. Thermometers and Temperature Scales 3. Thermal Expansion.
Physics 101 THursday 10/27/11 Class 19 Chapter 12.2 – 12.3 Gravitational attraction of spherical bodies Keplers laws.
Chapter 7 Rotational Motion and the Law of Gravity
NOTES-Chapter 12 Thermal Energy. Heat is defined and expressed by the Kinetic Molecular Theory of heat.
The Nature of Force.
Unit 6 : Part 2 Temperature and Kinetic Theory. Outline Temperature and Heat The Celsius and Fahrenheit Temperature Scales Gas Laws, Absolute Temperature,
 This version has no answers.. Which is stronger, Earth’s pull on the Moon, or the Moon’s pull on Earth? 1) the Earth pulls harder on the Moon 2) the.
Thermodynamics. Temperature What is temperature? Temperature is what we measure with a thermometer. What is a thermometer? A thermometer is any devise.
EQ: Why does an object in circular motion have a constant velocity yet an acceleration and unbalanced force that is directed toward the center of the circle?
Copyright © 2012 Pearson Education Inc. Gravitation Physics 7C lecture 17 Tuesday December 3, 8:00 AM – 9:20 AM Engineering Hall 1200.
What is Heat?. Why did you put a jacket on this morning? What is cold? What is hot? Why are faucets labeled “H” and “C”? When you first turn on the “hot”
T072: Q19: A spaceship is going from the Earth (mass = M e ) to the Moon (mass = M m ) along the line joining their centers. At what distance from the.
@earthscience92. What is Energy? Energy – Is the ability to cause change – Many forms of energy – Two general forms of energy are Kinetic energy Potential.
Newton’s Second Law Pages Describe your acceleration if you are in a circular motion. What is the net force of your motion? You are constantly.
GRAVITY Gravity Gravity is a force that for us is always directed downwards. But to say that gravity acts downwards is not correct. Gravity acts down,
Chapter 3. Force, Mass, and Acceleration Newton’s first law of motion states that the motion of an object changes only if an unbalanced force acts on.
PHY 151: Lecture 6A 6.1 Newton’s Law of Universal Gravity 6.2 Gravitational Formula 6.3 Extending Particle in Uniform Circular Motion Model.
Gravitational Forces. What is Gravity? Gravity is the tendency of all objects (with mass) to attract one another. We often refer to this as a gravitational.
Which is stronger, Earth’s pull on the Moon, or the Moon’s pull on Earth? 1) the Earth pulls harder on the Moon 2) the Moon pulls harder on the Earth 3)
A satellite orbits the earth with constant speed at height above the surface equal to the earth’s radius. The magnitude of the satellite’s acceleration.
Basic Mechanics. Units Velocity and Acceleration Speed: Time rate of change of position. Velocity: Speed in a specific direction. Velocity is specified.
Gravity and Motion. Standards P.8.B.1 Students know the effects of balanced and unbalanced forces on an object’s motion. E/S P.8.B.3 Students know every.
Satellite Motion.
College Physics, 7th Edition
3.1 Motion in a Circle Gravity and Motion
Gravity.
A rigid object is rotating with an angular speed w > 0
Thermal 3.
Chapter 11 Section 2.
Unit 2 Force & Motion Ch 6 Sec 4 Gravity.
Gravitational Fields.
ConcepTest Clicker Questions Chapter 6
Rotational Motion and the Law of Gravity
Presentation transcript:

Two satellites A and B of the same mass are going around Earth in concentric orbits. The distance of satellite B from Earth’s center is twice that of satellite A. What is the ratio of the centripetal force acting on B to that acting on A? 1. 1/8 2. 1/4 3. 1/2 4. √1⁄2 5. 1 Answer: 2.The centripetal force on each satellite is provided by the gravitational force between the satellite and Earth.

Two satellites A and B of the same mass are going around Earth in concentric orbits. The distance of satellite B from Earth’s center is twice that of satellite A. What is the ratio of the tangential speed of B to that of A? 1. 1⁄2 2. √1⁄2 3. 1 4. √2 5. 2 Answer: 2. For each satellite, the centripetal force is equal to the gravitational force between the satellite and Earth, and is proportional to the square of the tangential velocity and the inverse of the distance.

1. be much less than g (because the ball doesn’t fall to the ground). Suppose Earth had no atmosphere and a ball were fired from the top of Mt. Everest in a direction tangent to the ground. If the initial speed were high enough to cause the ball to travel in a circular trajectory around Earth, the ball’s acceleration would 1. be much less than g (because the ball doesn’t fall to the ground). 2. be approximately g. 3. depend on the ball’s speed. Answer: 2.The ball’s acceleration is caused by the only force exerted on the ball: gravitation. Near the surface of Earth, the value of this acceleration is g (perhaps a little less because of the altitude of Mt. Everest).

The Moon does not fall to Earth because 1. It is in Earth’s gravitational field. 2. The net force on it is zero. 3. It is beyond the main pull of Earth’s gravity. 4. It is being pulled by the Sun and planets as well as by Earth. 5. all of the above 6. none of the above Answer: 6.The Moon is accelerating toward Earth because of the gravitational attraction between the two.This attraction supplies the centripetal force necessary to keep the Moon in orbit.

Thermodynamics

CH 17: Temperature

What is temperature? Temperature describes the relative hotness or coldness between two objects. If you use your hand to compare the temperature of two objects you can only tell that one is warmer than the other. Temperature is a means of comparing the “hotness” between two objects. We define a standard “hotness” and compare all objects with this standard. What is the most commonly used standard for comparing the temperatures of different objects? The typical choice for a reference is the freezing point of water. All relative temperatures are compared to this standard. The numerical value for this standard is arbitrary. When two objects are placed in contact and internal energy can be transferred from one object to the other we say these two objects are in Thermal Contact. When two objects at different temperatures are placed in contact with each other they transfer internal energy from the object with more internal energy to the object with less internal energy. This will continue until both objects reach the same temperature. Two objects that are at the same temperature are said to be in Thermal Equilibrium. This fundamental idea is the basis for the zeroth law of thermodynamics. 0th Law of Thermodynamics – If object A and object B are separately in thermal equilibrium with a third object C, then A and B are in thermal equilibrium with each other. This law essential describes how a thermometer works.

Temperature Scales There are two temperature scales based on the 0th law of thermodynamics. These two scales are called relative scales. They are both arbitrarily based on the properties of water. Celsius Define two points 0oC and 100oC, which correspond to two distinct point where a phase change (temperature remains constant) occurs for water. All temperatures are measured relative to these specified values. Fahrenheit Define two points 32oF and 212oF, which correspond to two distinct point where a phase change (temperature remains constant) occurs for water. All temperatures are measured relative to these specified values. Both of these scales operate under the same principle, but they use a different mathematical relation to define the smallest change in the scale. These are relative scales, therefore zero has no meaning for the scale, it is just a reference point. Zero Celsius (32oF) is just the temperature at which water freezes. We can convert between the Fahrenheit and Celsius scales in the following way: There is approximately a 2o change in Fahrenheit for every 1o change in Celsius.