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chapter 11
chapter 11

... proportional to the volume stress (change in pressure). The corresponding constant ratio of stress to strain is called the bulk modulus, denoted by B. When the pressure on an object changes by a small amount Δp, from p0 to p0 + Δp, and the resulting volume strain is ΔV/V, Hooke’s law takes the form ...
IPC Review - Humble ISD
IPC Review - Humble ISD

... of 20.0 meters per second. Which statement best describes the time required for the spheres to reach the ground and the horizontal distance they travel? (1) Both spheres hit the ground at the same time and at the same distance from the base of the tower. (2) Both spheres hit the ground at the same t ...
12.2 Forces and Motion Keywords Acceleration
12.2 Forces and Motion Keywords Acceleration

4.01B Michelle was learning about forces today in her science class
4.01B Michelle was learning about forces today in her science class

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2. Forces

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THIS MS Word file
THIS MS Word file

... Work = force X displacement, but only if both force and displacement (WHICH ARE BOTH VECTORS!!!) are parallel or lie along the same line. If the previous statement is not true then the answer for work is zero. A vertical force cannot do work on an object that has horizontal displacement. For example ...
Chap4-Conceptual Modules
Chap4-Conceptual Modules

... 6. ConcepTest 4.2b Cart on Track II We just decided that the cart continues with constant velocity. What would have to be done in order to have the cart continue with constant ...
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TPC - Blue Valley Schools

... The following sections of TPC [The Physics Classroom] have been assigned during Unit 2. 1. Circle the letter of each page over which you took notes. 2. Circle the title if you have evidence of answering / working the CYU questions for that page. ...
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... – Acceleration – A measure of the change in velocity over change in time. – Force – A push or pull that is equal to the mass of the object multiplied by its acceleration (F = ma). ...
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... Question: An object is being pushed along at constant velocity by a force of 5 N [left]. What is the force of friction acting on the object? If the velocity is constant, there is no net force, so the force of friction must be equal in magnitude and opposite in direction to the applied force: ...
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net force - University of Iowa Physics
net force - University of Iowa Physics

Chapters Two and Three
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... Newton’s Third Law of Motion  “Whenever two objects interact, the force exerted on one object is equal in size and opposite in direction to the force exerted on the other object”  Example: Standing on the Floor  FAB = FBA ...
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Chapter 4 - Senior Physics

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June 2016 - Maths Genie

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Modeling with Integrals as Net Change

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Laws of Motion - SCHOOLinSITES

... curved path an object follows when thrown, launched, or otherwise projected near surface of Earth. ...
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Newton`s Laws of Motion

... Don’t let this be you. Wear seat belts. Because of inertia, objects (including you) resist changes in their motion. When the car going 80 km/hour is stopped by the brick wall, your body keeps moving at 80 m/hour. ...
circular motion ppt pdf
circular motion ppt pdf

... 1. The paths of planets around the sun are elliptical with the sun at one focus 2. The planets sweep out equal areas in equal times. That is, they move faster when closer to the sun and slower when further from the sun 3. The square of the period of a planet is proportional to the cube of the distan ...
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Unit 6: Motion and Forces

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Badger Chapter 28 - Forces and Motion

... motion, whether at rest or at a constant speed in a straight line. To change the motion of an object, there must be an overall force acting: a resultant or net force. It is the forces acting on an object that determine its motion. ...
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Classical central-force problem



In classical mechanics, the central-force problem is to determine the motion of a particle under the influence of a single central force. A central force is a force that points from the particle directly towards (or directly away from) a fixed point in space, the center, and whose magnitude only depends on the distance of the object to the center. In many important cases, the problem can be solved analytically, i.e., in terms of well-studied functions such as trigonometric functions.The solution of this problem is important to classical physics, since many naturally occurring forces are central. Examples include gravity and electromagnetism as described by Newton's law of universal gravitation and Coulomb's law, respectively. The problem is also important because some more complicated problems in classical physics (such as the two-body problem with forces along the line connecting the two bodies) can be reduced to a central-force problem. Finally, the solution to the central-force problem often makes a good initial approximation of the true motion, as in calculating the motion of the planets in the Solar System.
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