17-1 Physics I Class 17 Newton’s Theory of Gravitation.

Slides:



Advertisements
Similar presentations
17-1 Physics I Class 17 Newton’s Theory of Gravitation.
Advertisements

14 The Law of Gravity.
Kepler’s Laws. 2.5 The Laws of Planetary Motion Law 2. Imaginary line connecting Sun and planet sweeps out equal areas in equal times.
Gravity.
18-1 Physics I Class 18 Newton’s Theory of Gravitation.
Gravitation Newton’s Law of Gravitation; Kepler’s Laws of Planetary Motion. Lecture 14 Monday: 1 March 2004.
Chapter 13: Gravitation. Newton’s Law of Gravitation A uniform spherical shell shell of matter attracts a particles that is outside the shell as if all.
Physics 111: Elementary Mechanics – Lecture 12 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
CH 12: Gravitation. We have used the gravitational acceleration of an object to determine the weight of that object relative to the Earth. Where does.
Physics 111: Mechanics Lecture 13
GRAVITATION 10th Grade – Physics 10th - Physics.
Planetary Dynamics § 13.4–13.8. Closed Orbits U g + K tr = constant < 0 The closer the satellite is to the main body, the faster it moves Objects do not.
Physics 201: Lecture 24, Pg 1 Chapter 13 The beautiful rings of Saturn consist of countless centimeter-sized ice crystals, all orbiting the planet under.
The law of orbits:  All planets move in elliptical orbits, with the sun at one focus.
In 1543 Copernicus published On the Revolutions of the Heavenly Spheres in which he proposed that Earth and the other planets orbit the sun in perfect.
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.
Physics 221 Chapter 13 Is there gravity on Mars? Newton's Law of Universal Gravitation F = GmM/r 2 Compare with F = mg so g = GM/r 2 g depends inversely.
Gravitation. Gravitational Force and Field Newton proposed that a force of attraction exists between any two masses. This force law applies to point masses.
Newton’s Law of Universal Gravitation
Solving for Keplers 3 laws January 10,2012. Using your Orbit of Mercury you need to apply Kepler’s 3 laws of planetary motion…and write up in.
UNIVERSAL GRAVITATIONAL LAW of
Gravity and Orbits   Newton’s Law of Gravitation   The attractive force of gravity between two particles   G = 6.67 x Nm 2 /kg 2 Why is this.
Chapter 6 - Gravitation Newton’s Law of Gravitation (1687)
Universal Gravitation E M Ah, the same force that pulls the apple to the ground pulls moon out of its inertial path into circular motion around the earth!
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.
PLANETARY ORBITS Chapter 2. CONIC SECTIONS PLANETARY GEOMETRY l Definition of a Circle äA Circle is a figure for which all points on it are the same.
Kepler’s Laws of planetary motion Newton’s law of universal gravitation Free fall acceleration on surface of a planet Satellite motion Lecture 13: Universal.
Kepler’s Laws of Planetary Motion © David Hoult 2009.
Gravitation. Flat Earth This is true for a flat earth assumption. Is the earth flat? What evidence is there that it is not? Up to now we have parameterized.
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.
Kepler’s Laws of Planetary Motion - 3 Laws -. Elliptical Orbits Planets travel in elliptical orbits with the sun at one focus. Furthest point = Aphelion.
Gravitation and the Waltz of the Planets Chapter 4.
Kepler’s Law Eric Angat teacher. Orbit Eccentricity The eccentricity of an ellipse can be defined.
Newton’s Law of Universal Gravitation && Kepler’s Laws of Planetary Motion.
Kepler’s Three Laws of Planetary Motion. YMXtohttp:// YMXto.
Section Orbital Motion of Satellites and Kepler’s Laws
Universal Gravitation and Kepler’s Laws
Universal Gravitation Newton’s 4 th law. Universal Gravitation Kepler’s Laws Newton’s Law of Universal Gravity Applying Newton’s Law of Universal Gravity.
Unit 3 Lesson 2 Kepler’s Laws of Planetary Motion.
Copernicus’s Model  Many scientists believed our Earth was the center of the solar system, this theory is called geocentric  Copernicus first proposed.
Chapter 13 Gravitation & 13.3 Newton and the Law of Universal Gravitation Newton was an English Scientist He wanted to explain why Kepler’s Laws.
Satellite Motion Satellite – a projectile moving fast enough to fall continually around the Earth rather than into it - the Earth surface drops a vertical.
Satellite Physics & Planetary Motion Illustration from Isaac Newton, Philosophiae Naturalis Principia Mathematica, Book III Isaac Newton was the first.
Chapter 7 Gravitation. Newton’s Law of Universal Gravitation If two particles with masses m 1 and m 2 are separated by a distance r, then a gravitational.
Physics 141Mechanics Lecture 18 Kepler's Laws of Planetary Motion Yongli Gao The motion of stars and planets has drawn people's imagination since the.
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.
Kepler’s Three Laws of Planetary Motion
Chapter 11 – Gravity Lecture 1 April 6, 2010
Chapter 9: Gravity Gravity is the force most familiar to us, and yet, is the least understood of all the fundamental forces of nature.
Newton’s Law of Universal Gravitation
Newton’s Laws of Motion
Physics I Class 18 Newton’s Theory of Gravitation.
Kepler’s Laws: Physics not optional!
Chapter 12: Gravitation Newton’s Law of Gravitation.
Do Now We will be starting with a Kepler’s Law Review today
A Solar System is Born.
Kepler’s Laws 1. Planets have an elliptical orbit
Universal Gravitation
Kepler’s Laws of Planetary Motion
Gravitational Fields, Circular Orbits and Kepler
After Tycho Brahe’s death, Johannes Kepler (pictured here with Tycho in the background) used Tycho’s observations to deduce the three laws of planetary.
Chapter Contents Newton's Law of Universal Gravity
Gravitation See video on extreme sports --- defying gravity
Kepler’s Laws.
Gravitational Fields, Circular Orbits and Kepler’s Laws
Kepler’s Three Laws of Planetary Motion
THE EARTH, THE MOON & THE SUN
Kepler’s Laws of Planetary Motion
Physics I Class 17 Newton’s Theory of Gravitation.
Presentation transcript:

17-1 Physics I Class 17 Newton’s Theory of Gravitation

17-2 Forces Known to Physics

17-3 Newton’s Theory of Gravitation

17-4 Newton’s Law of Universal Gravitation

17-5 Properties of Gravity

17-6 If Gravity Varies As 1/r 2, Where Does g = 9.8 m/s 2 Fit In?

17-7 Gravity is a Conservative Force

17-8 Class #17 Problems of the Day

17-9 Kepler’s Three Laws of Planetary Motion 1. The Law of Orbits: All planets move in elliptical orbits having the Sun at one focus. 2. The Law of Areas: A line joining any planet to the Sun sweeps out equal areas in equal times. 3. The Law of Periods: The square of the period of any planet about the Sun is proportional to the cube of the semi-major axis of its orbit.

17-10 Kepler’s Three Laws of Planetary Motion

The Law of Areas

The Law of Periods

ENERGY IN CIRCULAR ORBITS