Universal Law of Gravitation

Slides:



Advertisements
Similar presentations
Week.  Student will:  Study the effects of forces on objects though  Newton’s First Law of Motion  Law of Inertia  Newton’s Second Law  Newton’s.
Advertisements

Chapter 2 Preview Objectives Changes in Velocity
Week.  Student will: centripetal accelerationcentripetal force  Solve problems involving centripetal acceleration and centripetal force.
Solving Systems of three equations with three variables Using substitution or elimination.
Science 30 Physics: Field Theory
Objectives WARM UP Identify forces of motion
Aim: How can we explain Newton’s Universal Law of Gravitation? Do Now: Why does the moon orbit the Earth? You will know by the end of the lesson.
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Section 2 Gravity Objectives Explain that gravitational force becomes.
Newton’s Law of Gravitation. Newton concluded that gravity was a force that acts through even great distances Newton did calculations on the a r of the.
Newton’s Law of Universal Gravitation
Week.  Student will: laws of conservation of energy  Demonstrate and apply the laws of conservation of energy in terms of  KineticPotential Energy.
Week.  Student will:  Incorporate Force of Friction into calculation  Static Friction  Kinetic Friction.
Mechanical Energy Pt. 2 Week.
Newton didn’t discover gravity; he discovered that gravity is universal. Everything pulls on everything else in a simple way that involves only mass and.
Newton believed that every object ___attracts_____ every other object. The force of the attraction depends on the __mass___ and _distance__ of the two.
Gravitation. Universal Law of Gravitation Every mass attracts every mass in universe - F g. F g directly proportional to mass. –Doubling the mass of one.
Projectile Motion Pt. 1 Week.
Week.  Student will: scalars vectors  Distinguish between scalars and vectors  Add subtract vectors  Add and subtract vectors.
Law of Universal Gravitation. Universal Gravitation gravity is a force of attraction between any two masses gravity is a UNIVERSAL force –universal meaning.
The Law of Universal Gravitation
Week.  Student will: Impulse and Momentum  Study Impulse and Momentum in one dimension.
Unit 06 “ Circular Motion, Gravitation and Black Holes” Gravitation Problem Solving.
Forces Chapter 6.1. What You Already Learned Velocity is the ratio of the change in position of an object over a period of time. Acceleration describes.
Week.  Student will: Magnetic Fields and Forces  Demonstrate Magnetic Fields and Forces.
 Newton’s Second Law can be expressed with an equation:  Which can be re-arranged to isolate Force like this:
MS. MORGAN Force. What is a Force? Something that changes the state of rest or the state of motion of an object. Can be a…. push or a pull Unit of measurement:
What is the centripetal force acting on a 2000 kilogram airplane if it turns with a radius of 1000 meters while moving at 300 meters per second? a c =
If it is known that A is directly proportional to B, how would A change if B is increased by a factor of 2? 1. Increase by a factor of 2 2. Increase by.
SOLVING SYSTEMS OF EQUATIONS BY SUBSTITUTION. #1. SOLVE one equation for the easiest variable a. Isolated variable b. Leading Coefficient of One #2. SUBSTITUTE.
Notes 6.5, Date__________ (Substitution). To solve using Substitution: 1.Solve one equation for one variable (choose the variable with a coefficient of.
Universal Gravitation Part 2. What holds galaxies together? Newton’s Law of Universal Gravitation says:
Here, we’ll show you how to calculate the area of a force being applied when we are given the force and the pressure.
Law of Gravitation. Law of Gravity  Gravitational Force  All objects have mass and therefore will attract all other objects.  The size of the gravitational.
Law of Universal Gravitation Law of Universal Gravitation: gravity is a force of attraction that exists between any two objects that have mass. Force of.
Newton’s Fourth Law Universal Gravitation UniversalUniversal Universal Gravitation.
Newton’s “4 th law”. Law of Universal Gravitation 1.Gravity is universal: ALL objects attract each other. 2.The force of gravity is directly proportional.
Newton’s Law of Universal Gravitation
Newton’s Universal Law of Gravity Every object attracts every other object with a force that is directly proportional to the masses of the objects and.
Forces Chapter 6.1. What You Already Learned Velocity is the ratio of the change in position of an object over a period of time. Acceleration describes.
The Solar System The Moon The Earth The Sun How do they move? Why doesn’t the Earth fly away? Photos by NASA.
The Force of Gravity. It is a centripetal force and it is provided by the gravitational force between the Earth & the Moon. What Type of force is this.
Forces Chapter 6.1. What You Already Learned Velocity is the ratio of the change in position of an object over a period of time. Acceleration describes.
Universal Gravitation Honors Physics First! Mr. Fowler.
Universal Gravitation Problems Universal Gravitation Problems
The Newtonian Synthesis Nicolaus Copernicus 1473 – 1543 Frame of Reference Tycho Brahe Accurate Data Johannes Kepler Emperical Laws.
Week.  Student will:  Incorporate Force of Friction into calculation  Static Friction  Kinetic Friction Cornell Notes Needed – Section 5.2.
What holds us together? Gravity. Gravity is a force Force: a push or pull exerted on an object Gravity: the attractive force between objects; force that.
“Every object in the universe attracts every other object in the universe”
FgFg agag mg g W Do you know the difference?? Newton’s Law of Universal Gravitation Every body in the universe attracts every other body with a force.
Gravitation Examples Answers 1. Two balls have their centers 3.0 m apart. One ball has a mass of 10.0 kg, while the other ball has a mass of 15.0 kg. Calculate.
Section 1 Displacement and Velocity Chapter 2 One Dimensional Motion To simplify the concept of motion, we will first consider motion that takes place.
Universal Law of Gravitations, Statics, Coulomb’s Law
Universal Gravitation
The Force of Gravity.
Mrs. Bryant 6th Grade Science
Warm-Up Hints: Proportional Reasoning
Law of Universal Gravitation
2-2-2 Universal Gravitation
Gravitation.
Section 3: Newton’s Third Law
Baseline (flightpath E): Know that the weight of an object can be calculated using the equation: W=mg and know the SI units of weight and mass. Further.
Solving equations Mrs. Hall.
Warm Up: 12/19/16 Pull out your pink lab sheet from Friday. Make sure that is finished up. Make sure you have a calculator today and tomorrow.
Solution... Click for answers.
Universal Gravitation
Universal Gravitation
Bell Work: Torque Review
Physics Final Review 2019.
Universal Gravitation
Do Now: What did Newton discover about gravity?.
Presentation transcript:

Universal Law of Gravitation Week

Student will: Objective Describe and calculate how the magnitude of the gravitational force between two objects

Force (N) = G∙mass 1 kg ∙mass 2 (kg) distance (m) 2 Cornell Notes (1/3) Questions Do all things have their own gravity? Law of Universal Gravitation: Every mass attracts every other mass through a force called gravity F g = G∙ m 1 ∙ m 2 r 2 Force (N) = G∙mass 1 kg ∙mass 2 (kg) distance (m) 2 Gravitational Constant = 6.67 x 10-11 N (m/kg)2

Cornell Notes (2/3) What happens to the force when you cut the distance in half? Cut the distance in half, and the force is 4 time greater. Double the distance, and the force is 1/4th what it was. What happens to the force when you double the distance?

Cornell Notes (1/5) Example: Gravitational Force Mr. Fantastic (82 kg) and Dr. Doom (102 kg), are standing 10 meters apart. Calculate the gravitational force between them.

Cornell Notes (2/5) Steps Define Given: m1 = 82 kg m2 = 102 kg r = 10 m G = 6.673 x 10-11 N∙m2/kg2 Unknown: Fg = ? Mr. Fantastic (82 kg) and Dr. Doom (102 kg), are standing 10 meters apart. Calculate the gravitational force between them.

Cornell Notes (3/5) F g =G m 1 m 2 r 2 F g =G m 1 m 2 r 2 Plan Choose an equation or situation: Rearrange the equation to isolate the unknown: F g =G m 1 m 2 r 2 F g =G m 1 m 2 r 2

Cornell Notes (4/5) F g =G m 1 m 2 r 2 Calculate Substitute the values into the equation and solve F g =G m 1 m 2 r 2 F g =6.67× 10 −11 ∙ (82)(102) 10 2 F g =5.578788× 10 −9 F g =5.579× 10 −9 N

Cornell Notes (5/5) Evaluate So, Mr. Fantastic pulls on Dr. Doom and Dr. Doom pulls on Mr. Fantastic with 5.579 x 10-9 N.