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Circular Motion
Circular Motion

Newton*s Laws of Motion
Newton*s Laws of Motion

College Physics
College Physics

Free Body Diagrams
Free Body Diagrams

Tuesday, Sept. 30, 2014
Tuesday, Sept. 30, 2014

... observations for a long time. The data people collected, however, have not been explained until Newton has discovered the law of gravitation. Every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional ...
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Forces in 1D Phet Lab

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2001 AL Physics MC Suggested Solution 1. E. Any three forces

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... Final Challenge 7. Try to arrange things so that the golf ball and the Ping-Pong ball end up with about the same acceleration. How will you have to alter the unbalanced force applied by the ruler to accomplish this? ...
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Solutions to the sample problems

... cosine are easy numbers to work with. sinθ = 3/5 and cosθ = 4/5. The angle is not 30˚, 45˚, or 60˚. Defining the positive x-direction as up the slope, apply Newton’s Second Law in the x-direction: -mg sinθ = ma, so a = - g sinθ = -10*(3/5) = -6.0 m/s2. To determine the distance traveled use: v 2 = v ...
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... Whoooaaa, so thats why Calc III was useful. Often times, we are given the derivation of several formulas. Will it be necessary to know or understand the derivation or can we just simply apply the formulas? We should have cookies in lecture one day You were right at the beginning, this was very diffi ...
1. A particle of mass m is projected vertically upward at z=O, with an
1. A particle of mass m is projected vertically upward at z=O, with an

Physics Notes – Types of Forces
Physics Notes – Types of Forces

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Chapter 4 - Santiago Canyon College

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Chapter 3 Reading Guide

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From last time… - High Energy Physics

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The Force Be With You

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... she falls faster and faster through the air, does her acceleration increase, decrease, or remain the same? A: Acceleration decreases because the net force acting on her decreases. Net force is equal to her weight minus her air drag, and being that air drag, increases with speed, net force and hence ...
Intro to Physics - hrsbstaff.ednet.ns.ca
Intro to Physics - hrsbstaff.ednet.ns.ca

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... mass to decelerate until it reaches zero velocity. Find the deceleration using Newton’s second law and the force of friction. We are on a flat surface so the normal force is equal to the gravity. Once you have the value of deceleration, you can use kinematics equations with initial and final velocit ...
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Physics PAP Syllabus Outline 2013-2014 Instructor: Claire Sauder

... • Words often have one meaning in everyday language and another, more specific meaning, in science. • The slope and shape of a graph have meaning. • All objects in free fall experience the same acceleration. • Velocity is motion, and acceleration is how motion changes. • Free fall motion is symmetri ...
PHYSICS 231 INTRODUCTORY PHYSICS I Lecture 11
PHYSICS 231 INTRODUCTORY PHYSICS I Lecture 11

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Chapter 4

... The First Law describes the natural state of motion of a body on which no forces are acting. The other two laws describe the behavior of a body under the influence of forces. ...
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... • Used Brahe’s data to find mathematical description of planetary motion • Isaac Newton (1642-1727) • Used his laws of motion and gravitation to derive Kepler’s laws ...
South Pasadena · AP Chemistry
South Pasadena · AP Chemistry

... air resistance of 250 Newtons. What is the acceleration of the skydiver? Weight of skydiver = mg = 85 kg x 9.8 m/s2 = 833 Newtons. Net Force = 833 N + - 250 N = 583 Newtons. acceleration = Fnet / mass = 583 N / 85 kg = 6.9 m/s2 4. Another skydiver of mass 70 kg, is moving through the air with an acc ...
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Gravity

Gravity or gravitation is a natural phenomenon by which all things with mass are brought towards (or 'gravitate' towards) one another including stars, planets, galaxies and even light and sub-atomic particles. Gravity is responsible for the complexity in the universe, by creating spheres of hydrogen, igniting them under pressure to form stars and grouping them into galaxies. Without gravity, the universe would be an uncomplicated one, existing without thermal energy and composed only of equally spaced particles. On Earth, gravity gives weight to physical objects and causes the tides. Gravity has an infinite range, and it cannot be absorbed, transformed, or shielded against.Gravity is most accurately described by the general theory of relativity (proposed by Albert Einstein in 1915) which describes gravity, not as a force, but as a consequence of the curvature of spacetime caused by the uneven distribution of mass/energy; and resulting in time dilation, where time lapses more slowly in strong gravitation. However, for most applications, gravity is well approximated by Newton's law of universal gravitation, which postulates that gravity is a force where two bodies of mass are directly drawn (or 'attracted') to each other according to a mathematical relationship, where the attractive force is proportional to the product of their masses and inversely proportional to the square of the distance between them. This is considered to occur over an infinite range, such that all bodies (with mass) in the universe are drawn to each other no matter how far they are apart.Gravity is the weakest of the four fundamental interactions of nature. The gravitational attraction is approximately 10−38 times the strength of the strong force (i.e. gravity is 38 orders of magnitude weaker), 10−36 times the strength of the electromagnetic force, and 10−29 times the strength of the weak force. As a consequence, gravity has a negligible influence on the behavior of sub-atomic particles, and plays no role in determining the internal properties of everyday matter (but see quantum gravity). On the other hand, gravity is the dominant force at the macroscopic scale, that is the cause of the formation, shape, and trajectory (orbit) of astronomical bodies, including those of asteroids, comets, planets, stars, and galaxies. It is responsible for causing the Earth and the other planets to orbit the Sun; for causing the Moon to orbit the Earth; for the formation of tides; for natural convection, by which fluid flow occurs under the influence of a density gradient and gravity; for heating the interiors of forming stars and planets to very high temperatures; for solar system, galaxy, stellar formation and evolution; and for various other phenomena observed on Earth and throughout the universe.In pursuit of a theory of everything, the merging of general relativity and quantum mechanics (or quantum field theory) into a more general theory of quantum gravity has become an area of research.
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