Chapter 4 Making Sense of the Universe “If I have seen farther than others, it is because I have stood on the shoulders of giants.” — Sir Isaac Newton.

Slides:



Advertisements
Similar presentations
How do we describe motion?
Advertisements

5. Universal Laws of Motion
Chapter 4: Making Sense of The Universe: Matter, Energy & Gravity
How to Study the Universe
The Beginning of Modern Astronomy
ASTR100 (Spring 2008) Introduction to Astronomy Newton’s Laws of Motion Prof. D.C. Richardson Sections
© 2010 Pearson Education, Inc. Newton’s third law of motion: For every force, there is always an equal and opposite reaction force.
Chapter 5 Gravity. Describing motion Speed: Rate at which object moves example: 10 m/s Velocity: Speed and direction example: 10 m/s, due east Acceleration:
© 2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Newton’s Laws of Motion Newton’s 1st Law Newton’s 2nd Law and Friction Newton’s 3rd Law and Law of Universal Gravitation.
(a) nearest the axis. (b) nearest the rim.
Chapter 4 Making Sense of the Universe Understanding Motion, Energy, and Gravity.
Lecture Outline Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity © 2015 Pearson Education, Inc.
Making Sense of the Universe Understanding Motion, Energy, and Gravity.
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:
Gravity. Review Question What are Kepler’s laws of planetary motion?
Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Fix Astronomy Chapter 5.
Chapter 4 Making Sense of the Universe Understanding Motion, Energy, and Gravity.
© 2004 Pearson Education Inc., publishing as Addison-Wesley 5.1 Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration.
© 2005 Pearson Education Inc., publishing as Addison-Wesley
Today’s Lectures: The Laws of Gravity Speed, velocity, acceleration, force Mass, momentum and inertia Newton’s three laws of motion The Force of Gravity.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Gravity, Projectiles, and Satellites Physics Click HERE if the web page above does not open. In this lesson, we will discuss the following: Newton’s Law.
Surface Gravity Objects on the Moon weigh less than objects on Earth This is because surface gravity is less –The Moon has less mass than the Earth, so.
Newton’s Third Law of Motion
Forces Chapter 3. Newton’s 2 nd law 2 nd – an object accelerates in the direction of the net force acting upon it A= net force/Mass a= Fnet/m A force.
What are Forces? A force is a push or a pull on an object.
Chapter 4: Newton and Universal Motion
Uniform Circular Motion. How does a roller coaster do a loop without falling off the track? How is water removed from a clothes washer?
Chapter 4d Making Sense of the Universe: Understanding Motion, Energy, and Gravity “ If I have seen farther than others, it is because I have stood on.
© 2005 Pearson Education Inc., publishing as Addison- Wesley The Planets Prof. Geoff Marcy The Law of Gravity Velocity and Acceleration Newton’s Laws:
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
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.
© 2005 Pearson Education Inc., publishing as Addison-Wesley Correction in Exam 1 Date: Thursday Feb. 10 Updated Syllabus in website has the corrected date.
Copyright © 2009 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Homework #2  Due today at 6PM  Covers Chapters 1, 2, and 3  Estimated time to complete: 1 hour 10 minutes (so don’t wait until the last minute!)  Read.
Lecture 4: Gravity and Motion Describing Motion Speed (miles/hr; km/s) Velocity (speed and direction) Acceleration (change in velocity) Units: m/s 2.
Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Sir Isaac Newton Newton, as he appeared on the last day of his life, in 1727.
Chapter 4b Making Sense of the Universe: Understanding Motion, Energy, and Gravity “ If I have seen farther than others, it is because I have stood on.
What is motion? what do scientists define as motion ? Why do the planets move the way they do?
Chapter 12 Universal Law of Gravity
Lecture 6: Gravity and Motion Review from Last Lecture… Newton’s Universal Law of Gravitation Kepler’s Laws are special cases of Newton’s Laws bound.
Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration. What is the acceleration of gravity? How does the acceleration.
NATS From the Cosmos to Earth Billiard Balls.
© 2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity “ If I have seen farther than others, it is because I have stood on.
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)
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)
Making Sense of the Universe Understanding Motion, Energy, and Gravity.
Chapter 4c Making Sense of the Universe: Understanding Motion, Energy, and Gravity “ If I have seen farther than others, it is because I have stood on.
Chapter 5 Gravity and Motion. Essential Question How are forces related to motion.
Review Question What is retrograde motion?. Review Question Explain why the phases of Venus proved to Galileo that Venus must orbit the Sun when the Moon.
© 2005 Pearson Education Inc., publishing as Addison-Wesley Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity “ If I have.
4.3 Energy and Conservation Laws. Kinetic energy is the energy associated with motion. KE = ½ mv 2 m = mass, v = velocity Types of Energy – Kinetic Energy.
Introductory Physics. How we describe motion Speed – how fast something is moving Velocity – speed and direction Acceleration – change in velocity Acceleration.
Motion and Energy. Motion What is Motion? Position is the location of an object. Motion is a change in position over time. Motion has two parts: distance.
Forces and Motion CHAPTER 6. Gravity and Motion Aristotle (round 400 BC) believed that heavier objects fell to the earth faster than lighter objects.
Today: Go over Review Packet from last time Reviews 3 and 4 Homework: Review Packet.
© 2014 Pearson Education, Inc. Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Chapter 4: Making Sense of the Universe Understanding Motion, Energy, and Gravity © 2015 Pearson Education, Inc.
4.1 Describing Motion: Examples from Everyday Life
Chapter 4: Making Sense of the Universe: Understanding Motion, Energy, and Gravity © 2017 Pearson Education, Inc.
Making Sense of the Universe Understanding Motion, Energy, and Gravity
5.1 Describing Motion: Examples from Daily Life
Chapter 4 Making Sense of the Universe:
Making Sense of the Universe Understanding Gravity and Motion
Presentation transcript:

Chapter 4 Making Sense of the Universe “If I have seen farther than others, it is because I have stood on the shoulders of giants.” — Sir Isaac Newton (1642 – 1727)

Sir Isaac Newton Much of what we learned from Newton was published in a text he wrote which is known today as “Principia”. Newton’s picture will indicate one of his contributions presented in this lecture that was first published in the Principia

Before we go into what Newton taught us. How do we describe motion? Speed : Rate at which object moves example: speed of 10 m/s Velocity : Speed and direction example: 10 m/s, due east Force An influence on motion e.g. pushing, pulling, friction, gravity, etc.

Newton’s first law of motion: Law of Inertia An object moves at constant velocity unless a net force acts to change its speed or direction. or “A body remains at rest or moves in a straight line at a constant speed unless acted upon by a force.”

More definitions Acceleration – Change in Velocity What are three examples of acceleration? – Speeding up – Slowing Down – Turning Mass- the amount of matter in an object. Also a measure of the resistance of an object to undergo an acceleration Or as Newton first defined it The quantity of matter is that which arises conjointly from its density and magnitude. A body twice as dense in double the space is quadruple in quantity. This quantity I designate by the name of body or of mass.

Newton’s Second Law Net Force = mass acceleration F = m a “The amount of acceleration that a force produces depends on the mass of the object being accelerated.” If more than one force is acting on an object the sum of the forces is called the net force…. Examples

Forces We earlier gave examples of forces as – pushing, pulling, friction, gravity, etc Newton was the first to identify and mathematically define the force of gravity. End of Aristotle’s separation of Heaven and Earth

Newton’s The Law of Gravity Every mass exerts a force of attraction on every other mass. The math… G = 6.67  N·m 2 /kg 2

Gravity Questions If the distance between two objects in space is doubled, then what happens to the gravitational force between them? What if the distance is tripled? …quadrupled?

If we drop a rock The only force acting on the falling object is gravity. Thus the net force is the force of gravity. Write F=ma and solve for a

Acceleration due to gravity The acceleration due to gravity on the earths surface is g=9.81m/s 2 and always points towards the center of the earth for all objects regardless of their mass. This was first demonstrated by Galileo dropping objects from the leaning tower of Pisa Apollo 15 demonstration

Mass of the Earth Since we can experimentally measure the acceleration due to gravity we could use Newton’s Universal Gravitation to calculate the mass of the earth. Density

Weight Weight is the force of gravity acting on an object. Weight = (mass acceleration due to gravity) W=mg

Thought Question On the Moon: A.My weight is the same, my mass is less. B.My weight is less, my mass is the same. C.My weight is more, my mass is the same. D.My weight is more, my mass is less.

Thought Question On the Moon: A.My weight is the same, my mass is less. B.My weight is less, my mass is the same. C.My weight is more, my mass is the same. D.My weight is more, my mass is less.

How does gravity cause tides? Moon’s gravity pulls harder on near side of Earth than on far side Difference in Moon’s gravitational pull stretches Earth

Tides and Phases Size of tides depends on phase of Moon

Newton’s Third Law Action-Reaction Whenever one body exerts a force on a second body, the second body exerts an equal and opposite force on the first body.”

Thought Question: When you jump out of a plane, is the force the Earth exerts on you larger, smaller, or the same as the force you exert on it? A.Earth exerts a larger force on you. B.I exert a larger force on Earth. C.Earth and I exert equal and opposite forces on each other.

Thought Question: A compact car and a Mack truck have a head-on collision. Are the following true or false? 1.The force of the car on the truck is equal and opposite to the force of the truck on the car. 2.The change of velocity of the car is the same as the change of velocity of the truck.

Thought Question: A compact car and a Mack truck have a head-on collision. Are the following true or false? 1.The force of the car on the truck is equal and opposite to the force of the truck on the car. T 2.The change of velocity of the car is the same as the change of velocity of the truck. F

Apparent Weight What a scale would read. You appear weightless in free-fall

Weightless To have a weight equal to zero you would have to be an infinite distance from all mass. Weightless instead implies your apparent weight would be zero. This is the case in the elevator accelerating down with a=g This is the case for astronauts in orbit

There is gravity in space Weightlessness is due to a constant state of free-fall Why are astronauts weightless in space?

Kepler’s laws revisited Newton was able to show that Kepler’s laws hold for all gravitationally bound orbits, not just planets around the sun. – Moon orbiting earth, comets, etc. Newton also showed orbits can be any conic section not just ellipses. – Parabolic and hyperbolic orbits are “unbound” meaning they do not close on themselves

Kepler’s 3 rd law revisited Newton was also able to generalize Kepler’s 3 rd law. G is the G from Universal gravitation, M 1 and M 2 are the masses of the system With this we can calculate the mass of each member of the solar system. – We know the mass of the earth – Use earth to get the sun…

Geosynchronous orbits All are at an altitude of 3.58 x 10 7 m or ~ 22,300 miles above the Earth. The period is one day

Conservation Laws in Physics It can be shown (by magic, hand waving, or miracle) that certain quantities in physics are constant under certain circumstances. Thus we say these quantities are conserved. Conserved quantities – Momentum – Angular momentum – Energy

Conservation of Momentum The total momentum of interacting objects cannot change unless an external force is acting on them Interacting objects exchange momentum through equal and opposite forces

Conservation of Angular Momentum The angular momentum of an object cannot change unless an external twisting force (torque) is acting on it Earth experiences no twisting force as it orbits the Sun, so its rotation and orbit will continue indefinitely This is the reason for precession of the earths axis angular momentum = mass x velocity x radius

Conservation of angular momentum is hat keeps a planet rotating and orbiting the Sun?

Angular momentum conservation also explains why objects rotate faster as they shrink in radius:

Energy Energy is the mover of matter, it cannot be created or destroyed, only changed from one type to another Types of energy KineticPotential Radiative (Radiation/light)Thermal Mass-energyAnd others...

Kinetic Energy Kinetic Energy is the energy of motion. Kinetic Energy = ½ mass  speed 2

Braking Example A car traveling 60 mph will skid 4 times farther than a car traveling 30 mph.

Cosmic Connections In 1994 a comet collided with Jupiter. The more massive fragments imparted more energy into the atmosphere of Jupiter.

150 ft. meteor impact in Arizona. 1 mi in diameter

June 30, 1908, 7:17 a.m. local time, Tungus natives and Russian settlers in the hills observed a column of bluish light, nearly as bright as the Sun, moving across the sky. About 10 minutes later, there was a flash and a sound similar to artillery fire. The sounds were accompanied by a shock wave that knocked people off their feet and broke windows hundreds of miles away. The majority of eyewitnesses reported only the sounds and the tremors, and not the sighting of the explosion. The explosion registered on seismic stations. Kulik's party reached the site in 1927.

Tunguska Event ~ 100 m (330 ft.) meteor exploded above ground.

Thermal Energy: the collective kinetic energy of many particles (for example, in a rock, in air, in water) Thermal energy is related to temperature but it is NOT the same. Temperature is the average kinetic energy of the many particles in a substance.

Thermal Energy Cool Hot

Temperature Scales

Mass-Energy Mass itself is a form of potential energy E = mc 2 A small amount of mass can release a great deal of energy Concentrated energy can spontaneously turn into particles (for example, in particle accelerators)

Potential Energy The energy that is stored is called potential energy. Examples: – Rubber bands – Springs – Bows – Batteries – Gravity – Chemical

Gravitational Potential Energy On Earth, depends on: – object’s mass (m) – strength of gravity (g) – distance object could potentially fall

Gravitational Potential Energy In space, an object or gas cloud has more gravitational energy when it is spread out than when it contracts.  A contracting cloud converts gravitational potential energy to thermal energy.

How do gravity and energy together allow us to understand orbits? Total orbital energy (gravitational + kinetic) stays constant if there is no external force Orbits cannot change spontaneously. More gravitational energy; Less kinetic energy Less gravitational energy; More kinetic energy Total orbital energy stays constant

 So what can make an object gain or lose orbital energy? Friction or atmospheric drag A gravitational encounter. Changing an Orbit

Orbital velocity It can be shown the speed of an object in orbit at a given radius R is given by Note it is only dependent on the mass of the object being orbited. V =

If an object gains enough orbital energy, it may escape (change from a bound to unbound orbit) Escape velocity from Earth ≈ 11 km/s from sea level (about 40,000 km/hr) Escape Velocity

V e = Escape Velocity