Newton and the Spring 2007 His 3464. Did Newton discover gravity? What, then did he do? And what did the have do do with it?

Slides:



Advertisements
Similar presentations
Sir Isaac Newton Law of Gravitation.
Advertisements

Progetto “Physics in English”
Universal Gravitation Everything Pulls on Everything Else!
Chapter 9 Gravity.
The Beginning of Modern Astronomy
Quiz Suppose that a planet was found to orbit the Sun, and that its path was an ellipse with eccentricity of 0.5. If the planet always moved at.
Famous Astronomers. Ptolemy Thought the Earth was at the center of the universe and that the other planets revolved around it (GEOcentric model) Thought.
© 2004 Pearson Education Inc., publishing as Addison-Wesley 5.1 Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration.
Physics 151: Lecture 27, Pg 1 Physics 151: Lecture 27 Today’s Agenda l Today’s Topic çGravity çPlanetary motion.
Gravitation Learn the nature of gravitational force. Solve problems using Newton’s law of gravitation. Learn about the two kinds of mass. Chapter 7 In.
Newton’s Law of Universal Gravitation By: Heather Britton.
Chapter 7 Review.
Gravity and Motion and Time on the Earth Upward Bound.
Do Now Significantly decreased gravity gives astronauts the sensation of being weightless and forces astronauts to make many adjustments in their activities.
Newton’s Third Law of Motion
Day 4.  Discussion on Yesterday’s Probes  Work on Today’s Probes.
Gravity Sucks! The acceleration due to gravity on the International space station is 8.7 m/s 2. If an 50 kg astronaut stood on a scale what would it.
Ch. 8 Universal Gravitation
Universal Gravitation
Chapter 19.1 Part 2.
Total of ALL forces acting on an object
Universal Gravitation
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.
Planets move through the sky with More complicated paths than Stars do. We begin with Kepler’s Laws in Order to find out how.
Measuring motion Two fundamental components: Change in position Change in time Three important combinations of length and time: 1.Speed 2.Velocity 3.Acceleration.
How we know what we know An introduction into orbital mechanics Matt Hamill.
Review Question What are Kepler’s laws?. Review Question What are Newton’s laws?
Sir Isaac Newton Newton, as he appeared on the last day of his life, in 1727.
Law of Universal Gravitation Chapter 12 November 9/10.
Universal Gravitation Applied Science Mr. Kuffer.
Apples and Planets PTYS Feb List of Symbols F, force a, acceleration (not semi-major axis in this lecture) v, velocity M, mass of Sun m,
AST 101 Lecture 7 Newton’s Laws and the Nature of Matter.
Universal Gravitation Gravity is the way in which masses communicate with each other.
Gravitation AP Physics 1. Newton’s Law of Gravitation What causes YOU to be pulled down? THE EARTH….or more specifically…the EARTH’S MASS. Anything that.
Gravity. The famous legend: The English scientist Sir Isaac Newton ( ) developed the theory of gravity when an apple fell from a tree and hit.
Unit 06 “Circular Motion, Gravitation and Black Holes” Gravity And Centripetal Force.
What if….. I know you are probably familiar with the movie “Gravity.” A lot of that was scientifically accurate. I find it interesting, however, that.
Describing Motion: Examples from Daily Life Distinguish between speed, velocity, and acceleration. What is the acceleration of gravity? How does the acceleration.
Universal Law of Gravitation and Planetary orbits.
Explaining the Universe. Pioneer and Voyager missions Pioneer 10 and 11 Voyager 1 and 2 Portrait of Solar System.
Newton’s Universal Law of Gravitation
Circular Motion Centripetal Force Apparent Weight Newtons’ Universal Gravitation Law.
Universal Gravitation. Gravity… Makes things such as leaves and rain fall It made the Earth round Builds up the pressures that kindle every star to shine.
Newton’s Universal Law of Gravitation Chapter 8. Gravity What is it? The force of attraction between any two masses in the universe. It decreases with.
The Apple & the Moon Isaac Newton realized that the motion of a falling apple and the motion of the Moon were both actually the same motion, caused by.
Gravity: A Force of Attraction
Gravity F Why would air make a difference? If you drop a ball and a feather from the same height at the same time, the ball would hit the ground.
Gravity: A Force of Attraction Chapter 19 Matter in Motion Section 4.
Gravity Newton realized that a force acts to pull objects straight down toward the center of Earth. He called this force gravity. Gravity is the force.
Bell Work What are Kepler’s three laws about planetary motion?
Universal Gravitation Chapter 12. The Falling Apple The idea that gravity extends through the universe is attributed to Sir Issac Newton He knew that.
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.
Chapter 9: Gravity & Planetary Motion
PHY 151: Lecture 6A 6.1 Newton’s Law of Universal Gravity 6.2 Gravitational Formula 6.3 Extending Particle in Uniform Circular Motion Model.
Gravity is a force that pulls objects toward each other. Legend says that Isaac Newton discovered gravity when he saw an apple fall from a tree Sir Isaac.
The Contributions of Sir Isaac Newton Compare effects of gravitational force on Earth, on the moon and within space. Identify contributions of Newton to.
Newton and the 20 October 2015 PHY 1033C. ? Why does the moon orbit the earth? So what was the problem The moon presented? ? ? ? ?
Basic Mechanics. Units Velocity and Acceleration Speed: Time rate of change of position. Velocity: Speed in a specific direction. Velocity is specified.
Everything pulls on everything else.
Newton at 46.
Universal Gravitation
The development of ideas regarding the Solar System
Gravity.
Unit 7 Lesson 2. Gravity: A Force of Attraction A
Classical Astronomy Introduction
Early Ideas.
The Effects of Gravity on Matter
GRAVITY & Tides.
PLANETARY MOTION.
Newton’s Laws.
Presentation transcript:

Newton and the Spring 2007 His 3464

Did Newton discover gravity? What, then did he do? And what did the have do do with it?

Newton at 83 Portrait by Enoch Seeman

Sir James Thronhill’s portrait of Newton at 67

Newton in 1701 (at 59)

Newton at 46

? Why does the moon orbit the earth? The Problem: ? ? ? ?

Complicating the Problem Galileo’s explanation: inertial motion circular

cosmic string

"After dinner, the weather being warm, we went into the garden and drank tea, under the shade of some apple trees, only he and myself. Amidst other discourse, he told me he was in the same situation as when formerly the notion of gravitation came into his mind. It was occasioned by the fall of an apple as he sat in a contemplative mood." William Stuckley, 1726 The legend of the apple

“As he sat alone in a garden, he fell into a speculation on the power of gravity: that as this power is not found sensibly diminished at the remotest distance from the center of the earth to which we can rise, neither at the tops of the loftiest buildings, nor even on the summits of the highest mountains, it appeared to him reasonable to conclude that this power must extend much farther than was usually thought. Why not as high as the moon, said he to himself? And if so, her motion must be influenced by it; perhaps she is retained in her orbit thereby....

The structure of Newton’s argument is p = The same force that affects apples also affects the moon q = The moon falls 16 feet in one minute Given the following statements: A. If p then q B. q C. Therefore p So he must prove both A and B

Gravity likely weakens, but by how much? Newton figures this out by combining his own insights with those of his predecessors

What he already knew a = 32 ft/sec 2 (by measuring it) d = 1/2 a t 2 (from Galileo) Inertial motion (his own “corrected” version) f of tension in a string The relation between a planet’s period and its distance from the sun

r1r1 r2r2 r If r is the average distance of a planet from the sun And T is the time it takes the planet to circle the sun Then Kepler’s 3rd Law says: T2T2  r3r3

cosmic string To find the tension in the cosmic string Newton examined the case of a rock on a string

f  mv2v2 /r

f  mv 2 /r v = d/t = f  m(2 B r/T) 2 /r = m4 B 2 r 2 T2T2 x 1 r m4 B 2 r T2T2 = 2 B r/T m(4 B 2 r 2 /T 2 ) x 1/r Now Newton applies this result to the moon case:

m4 B 2 r T2T2 But, from Kepler’s Third Law T 2  r 3 m4 B 2 r T2T2 = r3r3 = m4 B 2 r2r2 So f  k Thus f " 2 r2r2

f is  1 r2r2 At 1 earth radius: At 2 earth radii: F  1 (2r) 2 r2 r2 1 = some amount F 1 X F 1 = 1 2 F 1 r 2r

Newton’s next move: To show that the moon (like apples) falling body can be considered a

From Newton’s Principia Mathematica

Two cases of projectile fall Thrown slowlyThrown hard

d = 89.4 mi 1 mi (4001) Throw at 4.92 mi/sec for sec (4001) 2 + (89.4) 2 = 4002 C B CB = D = CD = 5280 ft So CD =4002 mi - 1 mi =4001 mi (89.4) CB - BD BD = ½ x 32 ft/sec 2 x (18.166) 2

Since f  a, a  f f is also  1 r2r2 Therefore a is  1 r2r2 At 1 earth radius: At 2 earth radii: a= 32 ft/sec 2 a= 1/2 2 x 32 = 8 ft/sec 2

The moon is 60 earth radii away Therefore at the distance of the moon x32 or ft/sec 2 a =

In one minute (60 sec) the moon will “fall” d = 1/2 a t 2 = 1/2x x = 16 feet He has thus proven A (if p then q)

To prove B (q: the moon “falls” 16 in 1 min) Newton drew the following construction A F C. E D B AEDADF

A F C. E D B His task is to find BD, the distance the moon “falls” in a given amount of time.

A F C. E D B To find BD Newton thinks like an engineer

A F C. E D B AED ADF AE AD = AF SO AD 2 = AE X AF THUS AF= AD 2 AE

A D represents 1 minute. Therefore arc length AD is 1 min minutes in a month xmoon’s orbit We now know AD Arc AD Earth The whole circleis 1 month

A F C. E D B AF= AD 2 AE Since and since AE is known Newton calculated AF to be ?

Recall the structure of Newton’s argument : If p then q, q: therefore p If the “apple force” is affecting the moon, then the moon “falls” 16 feet in 1 minute. The moon does fall 16 feet in one minute. Therefore the apple force affects the moon.

But, look at the following argument: p: If you have enough money, you go to the movies q: You go to the movies. Therefore you have enough money.

Nature was more complicated than Newton ever dreamed.

"The most beautiful experience we can have is the mysterious. It is the fundamental emotion that stands at the cradle of true art and true science. Whoever does not know it and can no longer wonder, no longer marvel, is as good as dead.”