© 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.

Slides:



Advertisements
Similar presentations
UNIT 6 (end of mechanics) Universal Gravitation & SHM
Advertisements

Chapter 13 Gravitation PhysicsI 2048.
TEST QUESTION 3-1 Kepler’s second law (law of equal areas) refers to
Physics for Scientists and Engineers, 6e
Q12.1 The mass of the Moon is 1/81 of the mass of the Earth.
Review Chap. 12 Gravitation
Chapter 12 Gravity DEHS Physics 1.
© 2010 Pearson Education, Inc. Newton’s third law of motion: For every force, there is always an equal and opposite reaction force.
© 2004 Pearson Education Inc., publishing as Addison-Wesley 5.1 Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration.
PHYS16 – Lecture 27 Gravitation November 10, 2010.
Uniform Circular Motion and Gravity
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.
Physics 151: Lecture 28 Today’s Agenda
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.
2006: Assoc. Prof. R. J. Reeves Gravitation 3.1 P113 Gravitation: Lecture 3 Escape speed from orbit Planets and satellites: Keplers Laws Orbital energy.
Chapter 13 Gravitation.
Chapter 12.
Satellites What keeps them in orbit?. Satellites A satellite is any projectile given a large enough velocity so its path follows the curvature of the.
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.
Dynamics Questions Chris Parkes. Motion s-t graph I drop a ball out of the window of my office (4 th floor) – which graph best represents the distance.
-Energy Considerations in Satellite and Planetary Motion -Escape Velocity -Black Holes AP Physics C Mrs. Coyle.
What keeps them in orbit?
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.
Gravity Review.
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.
Circular Motion.
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.
Review Question What are Kepler’s laws?. Review Question What are Newton’s laws?
Orbits Read Your Textbook: Foundations of Astronomy –Chapter 5 Homework Problems –Review Questions: 3, 4, 5, 9, 10 –Review Problems: 1, 3, 4 –Web Inquiries:
Physics 221 Chapter 13 Is there gravity on Mars? Newton's Law of Universal Gravitation F = GmM/r 2 Compare with F = mg so g = GM/r 2 g depends inversely.
Kepler ’ s Breakthrough Kepler used Brahe ’ s data to develop three laws that could be used to describe planetary motion. All of the laws are based upon.
Gravitation. Gravitational Force and Field Newton proposed that a force of attraction exists between any two masses. This force law applies to point masses.
GRAVITY What goes up, must come down??. Gravity Is it possible for some basketball players to “hang” in the air during a dunk? Give your opinion
Chapter 12 Universal Law of Gravity
Kepler’s Laws 1. The orbits of the planets are ellipses, with the sun at one focus of the ellipse. 2. The line joining the planet to the sun sweeps out.
Chapter 7 Rotational Motion and the Law of Gravity
Physics.
Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration. What is the acceleration of gravity? How does the acceleration.
Motions of the Earth ….it ’ s what moves us. Two motions of the Earth Rotation - Circular movement of an object around an axis Revolution -The movement.
 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.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 12 Physics, 4 th Edition James S. Walker.
PHY 2048C General Physics I with lab Spring 2011 CRNs 11154, & Dr. Derrick Boucher Assoc. Prof. of Physics Session 18, Chapter 13.
Copyright © 2012 Pearson Education Inc. Gravitation Physics 7C lecture 17 Tuesday December 3, 8:00 AM – 9:20 AM Engineering Hall 1200.
Created by: John Black Our planet Jupiter is very cold! In fact it is NEGATIVE 160 degrees (-234 F) Our planet has 67 moons! But only 18 moons are named!
Newton’s Law of Universal Gravitation
Q12.1 The mass of the Moon is 1/81 of the mass of the Earth.
Kepler’s Laws of Planetary Motion - 3 Laws -. Elliptical Orbits Planets travel in elliptical orbits with the sun at one focus. Furthest point = Aphelion.
Gravitation and the Waltz of the Planets Chapter 4.
A100 Movie Special Tuesday, March 23 Swain West 119 7:00 pm (153 minutes) Winner of several awards 20 activity points! BYOP (Bring Your Own Popcorn)
8-4.7 :: Explain the effects of gravity on tides and planetary orbits.
Kepler’s Three Laws of Planetary Motion. YMXtohttp:// YMXto.
Geometry of Earth’s Orbit Kepler’s Laws of Planetary Motion.
Newton’s Law of Universal Gravitation. Law of Universal Gravitation.
Unit 3 Lesson 2 Kepler’s Laws of Planetary Motion.
Laws of Planetary Motion KEPLER & NEWTON. Kepler’s 3 Laws  1 st Law- Law of Ellipses  2 nd Law- Law of Equal Areas  3 rd Law- Law of Periods.
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.
Kepler’s Three Laws of Planetary Motion
Gravitation Created by Craig Smiley (Harrison HS, West Lafayette, IN)
A rigid object is rotating with an angular speed w > 0
Chapter 12 Section 2 Gravity and Motion.
Chapter 2 Astronomy.
When an unbalanced force acts on an object, the force: a
Laws of Motion and Energy
Kepler’s Laws Ms. Jeffrey- Physics.
Mechanical Energy in circular orbits
Kepler’s Three Laws of Planetary Motion
Label it as completely as possible.
Presentation transcript:

© 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 Moon, the gravitational force that the Moon exerts on the Earth is A = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great. Q13.1

© 2012 Pearson Education, Inc. The planet Saturn has 100 times the mass of the Earth and is 10 times more distant from the Sun than the Earth is. Compared to the Earth ’ s acceleration as it orbits the Sun, the acceleration of Saturn as it orbits the Sun is A. 100 times greater. B. 10 times greater. C. the same. D. 1/10 as great. E. 1/100 as great. Q13.2

© 2012 Pearson Education, Inc. Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the Earth ’ s surface gravity, the surface gravity on Planet X is Q13.3 A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as much.

© 2012 Pearson Education, Inc. Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the amount of energy required to move an object from the Earth ’ s surface to infinity, the amount of energy required to move that same object from Planet X ’ s surface to infinity is A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as much. Q13.4

© 2012 Pearson Education, Inc. A satellite is moving around the Earth in a circular orbit. Over the course of an orbit, the Earth ’ s gravitational force A. does positive work on the satellite. B. does negative work on the satellite. C. does positive work on the satellite during part of the orbit and negative work on the satellite during the other part. D. does zero work on the satellite at all points in the orbit. Q13.5

© 2012 Pearson Education, Inc. A planet (P) is moving around the Sun (S) in an elliptical orbit. As the planet moves from aphelion to perihelion, the Sun ’ s gravitational force A. does positive work on the planet. B. does negative work on the planet. C. does positive work on the planet during part of the motion and negative work during the other part. D. does zero work on the planet at all points between aphelion and perihelion. Q13.6

© 2012 Pearson Education, Inc. A. increases during part of the motion and decreases during the rest of the motion. B. increases at all times. C. decreases at all times. D. remains the same at all times. Q13.7 A planet (P) is moving around the Sun (S) in an elliptical orbit. As the planet moves from aphelion to perihelion, the planet ’ s angular momentum

© 2012 Pearson Education, Inc. Star X has twice the mass of the Sun. One of Star X ’ s planets has the same mass as the Earth and orbits Star X at the same distance at which the Earth orbits the Sun. The orbital speed of this planet of Star X is A. faster than the Earth ’ s orbital speed. B. the same as the Earth ’ s orbital speed. C. slower than the Earth ’ s orbital speed. D. not enough information given to decide Q13.8

© 2012 Pearson Education, Inc. Suppose the Sun were to shrink to half of its present radius while maintaining the same mass. What effect would this have on the Earth ’ s orbit? A. The size of the orbit would decrease and the orbital period would decrease. B. The size of the orbit would increase and the orbital period would increase. C. The size of the orbit and the orbital period would remain unchanged. D. none of these Q13.9

© 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 Moon, the gravitational force that the Moon exerts on the Earth is A = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great. A13.1

© 2012 Pearson Education, Inc. The planet Saturn has 100 times the mass of the Earth and is 10 times more distant from the Sun than the Earth is. Compared to the Earth ’ s acceleration as it orbits the Sun, the acceleration of Saturn as it orbits the Sun is A. 100 times greater. B. 10 times greater. C. the same. D. 1/10 as great. E. 1/100 as great. A13.2

© 2012 Pearson Education, Inc. Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the Earth ’ s surface gravity, the surface gravity on Planet X is A13.3 A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as much.

© 2012 Pearson Education, Inc. Compared to the Earth, Planet X has twice the mass and twice the radius. This means that compared to the amount of energy required to move an object from the Earth ’ s surface to infinity, the amount of energy required to move that same object from Planet X ’ s surface to infinity is A. 4 times as much. B. twice as much. C. the same. D. 1/2 as much. E. 1/4 as much. A13.4

© 2012 Pearson Education, Inc. A satellite is moving around the Earth in a circular orbit. Over the course of an orbit, the Earth ’ s gravitational force A. does positive work on the satellite. B. does negative work on the satellite. C. does positive work on the satellite during part of the orbit and negative work on the satellite during the other part. D. does zero work on the satellite at all points in the orbit. A13.5

© 2012 Pearson Education, Inc. A planet (P) is moving around the Sun (S) in an elliptical orbit. As the planet moves from aphelion to perihelion, the Sun ’ s gravitational force A. does positive work on the planet. B. does negative work on the planet. C. does positive work on the planet during part of the motion and negative work during the other part. D. does zero work on the planet at all points between aphelion and perihelion. A13.6

© 2012 Pearson Education, Inc. A13.7 A. increases during part of the motion and decreases during the rest of the motion. B. increases at all times. C. decreases at all times. D. remains the same at all times. A planet (P) is moving around the Sun (S) in an elliptical orbit. As the planet moves from aphelion to perihelion, the planet ’ s angular momentum

© 2012 Pearson Education, Inc. Star X has twice the mass of the Sun. One of Star X ’ s planets has the same mass as the Earth and orbits Star X at the same distance at which the Earth orbits the Sun. The orbital speed of this planet of Star X is A. faster than the Earth ’ s orbital speed. B. the same as the Earth ’ s orbital speed. C. slower than the Earth ’ s orbital speed. D. not enough information given to decide A13.8

© 2012 Pearson Education, Inc. Suppose the Sun were to shrink to half of its present radius while maintaining the same mass. What effect would this have on the Earth ’ s orbit? A. The size of the orbit would decrease and the orbital period would decrease. B. The size of the orbit would increase and the orbital period would increase. C. The size of the orbit and the orbital period would remain unchanged. D. none of these A13.9