By; Jarrick Serdar, Michael Broberg, Trevor Grey, Cameron Kearl, Claire DeCoste, and Kristian Fors

Similar documents
GRAVITY. You can t blame gravity for falling in love. Albert Einstein

Gravity and the Orbits of Planets

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

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields

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

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Planetary Mechanics:

Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

7.4 Universal Gravitation

7 Study Guide. Gravitation Vocabulary Review

Gravitation and the Motion of the Planets

Copyright 2010 Pearson Education, Inc. GRAVITY. Chapter 12

Kepler, Newton, and laws of motion


January 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

Astronomy- The Original Science

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

Newton s Gravitational Law

Announcements. Topics To Be Covered in this Lecture

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

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

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Introduction To Modern Astronomy I

Chapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Universal Gravitation

Contents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic

Occam s Razor: William of Occam, 1340(!)

Unit 5 Gravitation. Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion

PHYS 155 Introductory Astronomy

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

Gravitation and the Waltz of the Planets

Gravitation and the Waltz of the Planets. Chapter Four

Gravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force.

Circular Motion and Gravitation. Centripetal Acceleration

Astronomy Lesson 8.1 Astronomy s Movers and Shakers

Physics 12. Unit 5 Circular Motion and Gravitation Part 2

1. Which of the following correctly lists our cosmic address from small to large?

Universal gravitation

Intro to Astronomy. Looking at Our Space Neighborhood

Welcome back to Physics 211. Physics 211 Spring 2014 Lecture Gravity

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

6. Summarize Newton s Law of gravity and the inverse square concept. Write out the equation

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion

Standard units of mass, length and 7me. Kilograms (kg) Meters (m) Seconds (s)

Cosmology is the study of the universe. What is it s structure? How did it originate? How is it evolving? What is its eventual fate?

AP Physics-B Universal Gravitation Introduction: Kepler s Laws of Planetary Motion: Newton s Law of Universal Gravitation: Performance Objectives:

4π 2 G(M1+M2 ) p2 = Newton s 3 Laws of Motion AST 105. Introduction to Astronomy: The Solar System. Newton's Version of Kepler's Third Law

Physics Test 7: Circular Motion page 1

Early Models of the Universe. How we explained those big shiny lights in the sky

Chapter 14 Satellite Motion

CIRCULAR MOTION AND UNIVERSAL GRAVITATION

Lesson 2 - The Copernican Revolution

Welcome back to Physics 215

Circular Motion and Gravitation. Centripetal Acceleration

Welcome back to Physics 215

The History of Astronomy

Today. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics

What is the solar system?

AST 105. Introduction to Astronomy: The Solar System. Announcement: First Midterm this Thursday 02/25

Chapter. Origin of Modern Astronomy

The Acceleration of Gravity (g)

How Astronomers Learnt that The Heavens Are Not Perfect

Chapter 13: universal gravitation

l Register your iclicker on LON-CAPA l First exam: Feb 6 in Life Sciences A133 >95% of you have

Observational Astronomy - Lecture 4 Orbits, Motions, Kepler s and Newton s Laws

2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity

What is a Satellite? A satellite is an object that orbits another object. Ex. Radio satellite, moons, planets

History of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period

Chapter 13. Universal Gravitation

towards the modern view

Ch. 22 Origin of Modern Astronomy Pretest

Astronomy 1 Fall 2016

CH 8. Universal Gravitation Planetary and Satellite Motion

Origins of the Universe

LESSON 1. Solar System

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:

AP Physics Multiple Choice Practice Gravitation

Circular Motion and Gravitation Notes 1 Centripetal Acceleration and Force

Chapter 8 - Gravity Tuesday, March 24 th

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

How big is the Universe and where are we in it?

Planetary Orbits: Kepler s Laws 1/18/07

Chapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios

14.1 Earth Satellites. The path of an Earth satellite follows the curvature of the Earth.

History of Astronomy. Historical People and Theories

,.~ Readlng ~ What,~,~~ is a geocentric system? Chapter3 J 73

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

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1

Chapter 2 The Science of Life in the Universe

Motion in the Heavens

Copernican Revolution. ~1500 to ~1700

Gravity. The Universal Force

Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points)

The following notes roughly correspond to Section 2.4 and Chapter 3 of the text by Bennett. This note focuses on the details of the transition for a

ASTR 150. Planetarium Shows begin Sept 9th. Register your iclicker! Last time: The Night Sky Today: Motion and Gravity. Info on course website

1 Astronomy: The Original Science

Gravitation. Luis Anchordoqui

5. Universal Laws of Motion

Test 1 Review Chapter 1 Our place in the universe

Transcription:

By; Jarrick Serdar, Michael Broberg, Trevor Grey, Cameron Kearl, Claire DeCoste, and Kristian Fors

What is gravity? Gravity is defined as the force of attraction by which terrestrial bodies tend to fall toward the center of the earth. Means by which all things with mass are attracted to each other, including planets, stars, and galaxies. Fg=Gm₁m₂ r^2 G = 6.67 10^-11 Nm2/kg2 The Gravitational constant is always the same no matter where you are in the Universe.

The force of gravity between two objects depends on 3 quantities: 1. Distance between the two objects: r 2. How big the first object is: m₁ 3. How big the second object is: m₂

Gravitational Potential Energy PEg = -Gm1m2 r WHY it s negative? Because a negative amount of work is done to bring an object closer to the Earth. The gravitational potential is the energy that an object has, based on where it is in a gravitational field The gravitational acceleration on the surface of the earth is 9.8 m/s^2

Orbital Velocity Objects that already have velocity come into the gravity field of an object begin to fall into their orbit ex.) When a satellite is put into space, it maintains a current speed while it travels in earths orbit, just as the moon does The equation for Orbital Velocity relies on the mass of the object, the gravitational pull, and the radius of the planet

Escape Velocity Escape Velocity is the lowest velocity that a body must have in order to escape the gravitational attraction of a particular planet or other object. ex.)in order for NASA to put satellites into space, they must first find the escape velocity of the satellite so they can overcome earth's gravity The equation of escape velocity depends on the gravitational pull of the planet, the mass of the planet and the radius of the planet Vesc = (2GM/R)

Kepler s 3 Laws of Planetary Motion 1. The orbit of a planet is an ellipse with the sun at one of the two focus points. 2. A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time. 3. The square of the orbital period of a planet is proportional to the cube of its average distance from the Sun. T^2 = 4π^2r^3 r = the average distance from the Sun GM

Major Contributions Eratosthenes was the first to measure the circumference of Earth. Ptolemy created the idea of a Geocentric Universe. Nicolaus Copernicus was the father of the Heliocentric Theory, and often thought to spark the Scientific Revolution. Tycho Brahe discovered that our universe is dynamic and ever changing. Galileo Galilei discovered that in the absence of air resistance, all objects accelerate toward the Earth at the same rate, regardless of mass. Albert Einstein proposed that gravity is the universal attraction between all mass, and, since E = mc2, all forms of energy Gravity is the curvature of spacetime the four dimensional fabric of the universe Edwin Hubble believed that the Universe goes beyond the Milky Way, and that is was expanding ever so rapidly.

Newton s Theory of Gravity Explained the motion of falling objects In 1821, Alexis Bouvard observed disturbances in the orbit of Uranus Newton s theory of gravity predicted these disturbances were due to the presence of an unknown gravitational source and eventually led to the discovery of Neptune

Common Misconceptions - - - The shape of an orbit is an ellipse, not a circle Weight changes, mass is constant. Make sure to convert to the appropriate units before making any calculations. Gravitational potential energy is negative Doesn't have constant velocity, has constant speed In acceleration due to gravity, all objects fall in free fall, this means that no matter what the mass is, in a vacuum they would fall at the same velocity, the only reason some objects fall faster is due to air resistance. Remember when calculation how strong the force of gravity is to measure the distance from the CORE not from the surface of the Earth i.e. If an apple tree is doubled in height Isaac Newton did not discover gravity because of an apple tree Earth is not a perfect sphere and that s why Eratosthenes messed up when calculating the circumference of the Earth

Multiple Choice Review

Question 1 What is the force of gravity between Jupiter and it s moon that are 670, 000 kilometers apart? The mass of Jupiter is 1.9 x 10^27 kg, and the mass of moon is 4.8 x 10^22 kg. A. 1.36 x 10^22 C. 9.0 x 10^30 B. 9.1 x 10^22 D. 1.36 x 10^30

Question 1 Answer Answer: A. 1.36 x 10^22 N

Question 2) Question 2) Kepler's 1st law The orbit of a planet is an with the sun at one of the two focus points. A. Sphere B. circle C. Ellipse D. Oval

Question 2 Answer Answer: C. Ellipse

Question 3 The sun weighs 1.989 10^30 kg. If it takes 365 days to orbit the sun, on average how far is the earth from the sun? a) 1.62 x 10^11 b) 1.49 x 10^11 c) d) 1.28 x 10^11 1.45 x 10^11

Question 3 Answer Answer: b) 1.49 x 10^11

Question 4 How is your mass on Earth compared to your mass on the moon? A. 2x greater B. Same C. 2x smaller D. 4x greater

Question 4 Answer B. Same

Question 5 Calculate the escape velocity of Planet B, which has a mass of 1.38 x 10^25 kg, and a radius of 6.32 x 10^7 m. a) 6453.2 m/s c) 5397.1 m/s b) 4312.1 m/s d) 5285.1 m/s

Question 5 Answer Answer: c) 5397.1 m/s