Isaac Newton - Late 17th Century

Slides:



Advertisements
Similar presentations
How do we describe motion?
Advertisements

Chapter 9 & 10 Gravity Pythagoras (550 BC) n Claimed that natural phenomena could be described by mathematics.
Chapter 4 Making Sense of the Universe Understanding Motion, Energy, and Gravity.
LESSON 10: Gravity and Orbits Modified from 05.ppt#295,6,Isaac Newton ( )
From Aristotle to Newton
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity.
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.
Introduction to Gravity and Orbits. Isaac Newton Born in England in 1642 Invented calculus in early twenties Finally published work in gravity in 1687.
Please pick up problem set #1. Median score = 63 (B-). Recitation session: Every Monday before a problem set is due. 4:30 – 5:30 pm McPherson (“The.
Chapter 4: Newton and Universal Motion
Ch. 8 Universal Gravitation
Circular Motion; Gravitation
Gravity, Orbits & Tides.
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.
Lecture 5: Gravity and Motion
Gravity How come the astronauts float around when they are inside the space shuttle? A) The shuttle’s rockets compensate for gravity B) The shuttle is.
Gravity. Geocentric vs. Heliocentric Model The Geocentric Model Arguments For: Parallax not seen Almagest says so Fits with “heavenly” perfection Arguments.
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.
Review Question What are Kepler’s laws?. Review Question What are Newton’s laws?
17-1 Physics I Class 17 Newton’s Theory of Gravitation.
1 Tycho Brahe ( ) best observer of his day Made most accurate measurements of his time.
Daily Science Pg.30 Write a formula for finding eccentricity. Assign each measurement a variable letter. If two focus points are 450 km away from one another.
A New Era of Science Mathematics as a tool for understanding physics.
PHYS 2010 Nathalie Hoffmann University of Utah
Stable Orbits Kepler’s Laws Newton’s Gravity. I. Stable Orbits A. A satellite with no horizontal velocity will __________________. B. A satellite with.
Unit 11, problem 3, 16 Unit 12, problem 5, 8, 10, 11, 12 Unit 14, problem 13, 14 Unit 15 problem 10, 13.
Gravitation and the Waltz of the Planets Chapter 4.
Nicholas Copurnicus Chapter 3 Survey of Astronomy astro1010-lee.com.
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.
Newton’s Laws. Newton’s First Law: The Law of Inertia An object at rest will stay at rest unless acted upon by a force, and an object in motion will stay.
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.
Newton’s Law of Universal Gravitation by Daniel Silver AP Physics C
Universal Gravitation and Kepler’s Laws
History of Astronomy - Part II
Newton’s Laws.
From Aristotle to Newton
Chapter 10: Projectile and Satellite Motion
Gravity.
Chapter 3: “Orbits & Gravity"”
Newton’s Universal Law of Gravitation
Chapter 9: Gravity Gravity is the force most familiar to us, and yet, is the least understood of all the fundamental forces of nature.
5.1 Describing Motion: Examples from Daily Life
Astronomy-Part 7 Notes Gravity and its Role in the Solar System
Newton’s Law of Universal Gravitation
Newton’s Laws of Motion
What is gravity? Galileo and Newton gave the name
Astronomy-Part 7 Notes Gravity and its Role in the Solar System
Unit 2 Review Questions.
4.2 Newton’s Laws of Motion
Kepler’s Laws.
Orbits and Kepler’s Laws
Making Sense of the Universe Understanding Gravity and Motion
Pages Gravity.
Gravity and Motion.
Gravity and Orbits – Not Free Fall
Orbits Round and round we go!.
Gravitational Fields, Circular Orbits and Kepler
Gravity and Motion.
Forces.
Kepler’s Laws Ms. Jeffrey- Physics.
Newton’s Law of Universal Gravitation
Kepler’s laws And Orbital Velocity.
Gravitational Fields, Circular Orbits and Kepler’s Laws
History of Astronomy - Part II
PLANETARY MOTION.
Kepler’s Laws.
Kepler’s laws And Orbital Velocity.
Physics I Class 17 Newton’s Theory of Gravitation.
Presentation transcript:

Isaac Newton - Late 17th Century Discovered Three Laws of Motion Discovered Universal Laws of Gravitation Modified Kepler’s Laws Invented calculus Invented new telescope Studied Light’s spectrum Etc. Newton

Newton’s Three Laws of Motion Objects go in straight lines at constant velocity unless you push on them When a force acts on an object, it changes speed (accelerates) according to When one object pushes on another, the other pushes back with exactly the same force F = ma

Newton’s First Law

Newton’s Third Law Q. 7: Understanding Newton’s Laws

m M r Newton’s Law of Universal Gravitation All objects have mass which tells us how much stuff they have in them Any two objects will be attracted to each other depending on their separation Force is proportional to product of their masses and inversely proportional to the square of their separation. m M r Q. 8: Newton’s Law of Gravity and Forces

Kepler’s Laws – Newton’s Version Planets move on ellipses with one focus at the Sun , parabolas, or hyperbolas

Kepler’s Laws – Newton’s Version 2. A line joining the Sun and the planet sweeps out equal area in equal time Unchanged by Newton 3. The square of the period (in years) equals the cube of the semi-major axis (in AU). times the mass of the combined objects (in solar masses) (M + m) P2 = a3 Far away move slower Massive moves faster

Solar Masses – a New Unit For describing stars, kilograms are too small (M + m)P2 = a3 This symbol means Sun Planets are much lighter than the Sun Q. 9: Using Newton’s Version of Kepler’s Third Law

Gravity and Orbits – Not Free Fall What happens when something holds you up. Gravity pulls you down Floor pushes you up Forces balance - you don’t go anywhere. You know which way is up because that is the way the floor is pushing you

Gravity and Orbits – Free Fall Cut the cable The elevator starts falling The floor no longer holds you up You fall too You float around – no gravity Because you and elevator are falling at the same rate, feels like weightlessness Free fall can be up, down, or sideways Help!

Gravity and Orbits - Circular Orbits “The knack [to flying] lies in learning how to throw yourself at the ground and miss” - The Hitchhiker’s Guide to the Galaxy trilogy, in Life, the Universe, and Everything

Q. 10: Why Is There “No Gravity” in Space? Gravity and Orbits Q. 10: Why Is There “No Gravity” in Space?

Non-Circular Orbits If velocity is more or less than this, you get an ellipse If velocity is big enough, it leaves on a parabola – escape velocity If velocity is bigger, it leaves on a hyperbola