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CPphysics review 2-10
CPphysics review 2-10

... d) both momentum and kinetic energy are conserved ...
Problem 1 (20 points)
Problem 1 (20 points)

p250t2f03
p250t2f03

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gravity and motion - carswellsciencetms

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Compared to the amount of energy required to accelerate a car from
Compared to the amount of energy required to accelerate a car from

... Concept Question: Consider two carts, of masses m and 2m, at rest on an air track. If you push first one cart for 3 s and then the other for the same length of time, exerting equal force on each, the kinetic energy of the light cart is 1. larger than 2. equal to 3. smaller than the kinetic energy of ...
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Document

6 - MIT
6 - MIT

... Concept Question: Consider two carts, of masses m and 2m, at rest on an air track. If you push first one cart for 3 s and then the other for the same length of time, exerting equal force on each, the kinetic energy of the light cart is 1. larger than 2. equal to 3. smaller than the kinetic energy of ...
Velocity - SFSU Physics & Astronomy
Velocity - SFSU Physics & Astronomy

... Note that the units cancel properly – this is the key to using the conversion factor correctly! ...
Text 1 (1.1 What is physics?) Children have an insatiable curiosity
Text 1 (1.1 What is physics?) Children have an insatiable curiosity

P2a Forces and Their Effects
P2a Forces and Their Effects

... Car safety: The force on a passenger will be large if there is a large change in momentum in a short time. The key to safety is to extend the time of impact to reduce the force. This is done by: seat belts stretch a little, crumple zones at the front and rear, air bags to cushion the impact. ...
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P2a Forces and Their Effects

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Momentum Jeopardy Review Game

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... starting, stopping, or changing directions inertia must be overcome in order to change the motion of the object. This is why inertia is newton’s first law of motion. Newton’s 2nd Law of Motion: Force = Mass x Acceleration Example: It takes more force to move a bus than a smart car, because the bus h ...
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2.1 Forces change Motion

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PowerPoint Presentation - Newton’s Laws of Motion
PowerPoint Presentation - Newton’s Laws of Motion

... philosophy) in 1687. Today these laws are known as Newton’s Laws of Motion and describe the motion of all objects on the scale we experience in our everyday lives. ...
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forces

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Work and Energy
Work and Energy

... both kinetic and gravitational potential energy. ET = KE + PE When an object is in motion, the total mechanical energy remains constant all along the path between the initial and final points. This law holds true if the net work done by external nonconservative forces is zero. In situations where he ...
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24 Slides

... will stay at rest…unless a force acts on them. The ball will stay at rest (not move) unless the dog moves it. ...
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Newton's Second Law of Motion
Newton's Second Law of Motion

... to toss a softball into the air and to toss a bowling ball into the air. Which one will accelerate more? The one with the smaller mass accelerates more. This is essentially Newton’s Second Law. Newton’s Second Law of Motion says the acceleration of an object is equal to the net force divided by the ...
Force and Motion Study Guide 1. What is motion? What do we use to
Force and Motion Study Guide 1. What is motion? What do we use to

Newton_s Laws Reviewx
Newton_s Laws Reviewx

... (D) The net work done by air resistance on the ball during its flight is zero. (E) The net work done by gravity on the ball during its flight is greater than zero. ...
Newton Review
Newton Review

... Use Chapters 1 & 2 in your book to help you find the answers to the questions below. 1. Write Newton’s first law. Law of Inertia: objects remain in motion, or at rest, until a force acts upon them. 2. Give an example of Newton’s first law using a tiny pebble and a boulder in your example. The tiny p ...
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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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