Acceleration Due to Gravity Gravity accelerates all objects in the same manner Any differences in freefall are due to air resistance Hammer and feather.

Slides:



Advertisements
Similar presentations
Lecture Outline Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity © 2015 Pearson Education, Inc.
Advertisements

Lecture Outline Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity © 2015 Pearson Education, Inc.
© 2005 Pearson Education Inc., publishing as Addison- Wesley The Planets Prof. Geoff Marcy The Law of Gravity Velocity and Acceleration Newton’s Laws:
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Law of Universal Gravitation Sir Isaac Newton (1642–1727) gave us.
Taking cube roots on a simple “scientific” calculator y x or using shift x  y 27 y x = or 27 shift x  y 3 = 3.
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.
Newton’s 2 nd Law Of Motion By Mr. Yum. Newton’s 2 nd Law Newton’s 2 nd Law is defined as: Newton’s 2 nd Law is defined as: F = m x a Where, F = force,
Physics 151: Lecture 28 Today’s Agenda
Kepler’s Laws of Planetary Motion Newton’s Laws of Gravity
Conservation of Momentum
Physics 151: Lecture 27, Pg 1 Physics 151: Lecture 27 Today’s Agenda l Today’s Topic çGravity çPlanetary motion.
Kepler’s Laws and Motion Astronomy 311 Professor Lee Carkner Lecture 5.
Planets Along the Ecliptic. Retrograde Motion Retrograde Motion Explained.
Feb. 2, 2011 NEWS: Exoplanets from Kepler.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Newton’s Laws of Motion and Planetary Orbits Gravity makes the solar system go round.
Newton and Gravity. State of Physics By now the world knew: Bodies of different weights fall at the same speed Bodies in motion did not necessarily come.
Sir Isaac Newton English physicist & mathematician …he developed the 3 laws of motion Motion is any change in position! p. 45 Click here.
Physical Science Gravity. Objectives Explain that gravitational force becomes stronger as the masses increase and rapidly become weaker as the distance.
Universal Gravitation
Chapter 10 Study Guide Tuesday, March 23, Section 1 Know Newton’s 1st Law of Motion. –Be able to explain and cite examples. Distinguish between.
Gravity. Law of Universal Gravitation The force of gravity applies to everything in the universe The force of gravity applies to everything in the universe.
Newton’s Law of Universal Gravitation
Lecture 5: Gravity and Motion
Universal Laws of Motion “ If I have seen farther than others, it is because I have stood on the shoulders of giants.” Sir Isaac Newton (1642 – 1727) Physicist.
Copyright © 2009 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Planets move through the sky with More complicated paths than Stars do. We begin with Kepler’s Laws in Order to find out how.
Lecture 4: Gravity and Motion Describing Motion Speed (miles/hr; km/s) Velocity (speed and direction) Acceleration (change in velocity) Units: m/s 2.
Kepler’s three laws Kepler’s three laws explain how planets orbit around the sun. These laws are common to any body orbiting around a massive body.
Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
AST 101 Lecture 7 Newton’s Laws and the Nature of Matter.
Gravity The force of attraction between objects that is due to their masses.
Universal Gravitation - Isaac Newton Combine Kepler’s Laws with Newton’s three laws of motion to get: “Between any two objects there exist an attractive.
17-1 Physics I Class 17 Newton’s Theory of Gravitation.
Kepler’s Laws What they tell us, and where they come from.
Kepler’s Laws of planetary motion Newton’s law of universal gravitation Free fall acceleration on surface of a planet Satellite motion Lecture 13: Universal.
PHYS 2010 Nathalie Hoffmann University of Utah
Very Large Telescope Finds Largest Star - Feb
Newton’s Law of Universal Gravitation && Kepler’s Laws of Planetary Motion.
Forces & Motion
Chapter 1 The Copernican Revolution. The planets’ motions Wanderers among the stars Retrograde motion.
Laws of Motion Classical Mechanics A brief overview.
 Mass- the amount of atoms inside an object ◦ Mass does not change!  Weight- the pull of gravity on the mass of an object ◦ Weight changes depending.
Gravity and Motion. Isaac Newton Isaac Newton was the first person to hypothesize that the force that pulls an apple to the ground also pulls the moon.
4.2 Gravity and Kepler’s Solar System p Falling Objects The Moon in Free Fall Newton understood that the Moon was in free-fall around the Earth.
Force Unit Part 2: Gravity. Objectives  Explain the law of universal gravitation and how applies to objects on Earth both still and falling and in space.
Introductory Physics. How we describe motion Speed – how fast something is moving Velocity – speed and direction Acceleration – change in velocity Acceleration.
The Contributions of Sir Isaac Newton Compare effects of gravitational force on Earth, on the moon and within space. Identify contributions of Newton to.
Friction Definition The resistance that one surface or object encounters when moving over another. Picture Word List: Motion Average Speed Velocity Acceleration.
Kepler’s Laws What are the shapes and important properties of the planetary orbits? How does the speed of a planet vary as it orbits the sun? How does.
Welcome to Who Wants to be a Millionaire
The Drag Force and Terminal Speed
Essential Questions: 1. How do forces affect the motion of an object?
Chapter 12 Section 2 Gravity Objectives
Newton, Einstein and Gravity
GRAVITY The force of gravity is an attractive force between all objects in the universe. The amount of GRAVITATIONAL FORCE between objects depends upon.
Chapter 1 Orion.
Newton’s Law of Universal Gravitation
Newton’s Laws of Motion
Forces Affecting Motion
Chapter 2: Forces and Motion
Test Review.
Orbits…the celestial paths of planets
Physics of the Solar System
Chapter 13 Gravitation In this chapter we will explore the following topics: -Newton’s law of gravitation that describes the attractive.
Chapter 13 Gravitation In this chapter we will explore the following topics: -Newton’s law of gravitation, which describes the attractive force between.
Chapter 20 Section 4 Planetary Motion Bellringer
Newton’s Law of Universal Gravitation
Gravitational Fields, Circular Orbits and Kepler’s Laws
Newton’s Law of Universal Gravitation
Presentation transcript:

Acceleration Due to Gravity Gravity accelerates all objects in the same manner Any differences in freefall are due to air resistance Hammer and feather fall at the same rate on Moon… no atmospshere

Acceleration

Sir Isaac Newton

Newton’s Law of Gravitation

Newton’s Insight

Planetary Motion from Gravity

Kepler’s Laws Explained All three of Kepler’s law can be explained by Newton’s gravity Ellipses are special cases: bound orbits 2 nd law follows from central force and conservation of angular momentum Newton’s form of Kepler’s 3 rd law: p 2 = 4  2 a 3 G(M 1 +M 2 )