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20150126075555
20150126075555

Physics Year Long Plan
Physics Year Long Plan

... describe the direction of velocity of, acceleration of, and force acting on an object in UCM calculate the velocity of, acceleration of, and force acting on and object in UCM determine the force providing the centripetal force describe the relationship between speed, radius, and force or acceleratio ...
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11. Rotation Translational Motion
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Simple Harmonic Motion

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Newton`s Laws - Galileo and Einstein
Newton`s Laws - Galileo and Einstein

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... 7. A car, initially at rest , travels 20 m in 4 s along a straight line with constant acceleration. The acceleration of the car (in m/s2) is: 8. An object is thrown straight up from ground level with a speed of 50 m/s. If g = 10 m/s 2 its distance above ground level 1.0 sec later is: 9 - 12 A ball i ...
Force
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... Weakest universal force at close distances, but most effective over great distances  …an attractive force that act between any two masses  Newton’s Law of Universal Gravitation states that every object in the universe attracts every other object ...
Physics 102 Introduction to Physics
Physics 102 Introduction to Physics

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Phy 211: General Physics I
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... Suppose an object was moving in a straight line with some velocity, v. According to Newton’s 1st Law of Motion, “An object in motion continues that motion unless a net external force acts on it”. If you want the object to move in a circle, some force must push or pull it towards the center of the c ...
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4.) A running football player has a momentum of 500 kg·m/s and a

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Science 2 - School helper
Science 2 - School helper

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Force – Acceleration and Velocity

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Physics unit 06 REVIEW Name___C. ANSWERS__________
Physics unit 06 REVIEW Name___C. ANSWERS__________

... 18. Why is centripetal force known as a net force? Give three different examples of objects in circular motion and the force(s) providing the centripetal force. Centripetal force must be unbalanced by other forces. If it would be balanced by another force, the net force would be 0, and an object wou ...
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File force and motion notes 2010

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Newton's theorem of revolving orbits



In classical mechanics, Newton's theorem of revolving orbits identifies the type of central force needed to multiply the angular speed of a particle by a factor k without affecting its radial motion (Figures 1 and 2). Newton applied his theorem to understanding the overall rotation of orbits (apsidal precession, Figure 3) that is observed for the Moon and planets. The term ""radial motion"" signifies the motion towards or away from the center of force, whereas the angular motion is perpendicular to the radial motion.Isaac Newton derived this theorem in Propositions 43–45 of Book I of his Philosophiæ Naturalis Principia Mathematica, first published in 1687. In Proposition 43, he showed that the added force must be a central force, one whose magnitude depends only upon the distance r between the particle and a point fixed in space (the center). In Proposition 44, he derived a formula for the force, showing that it was an inverse-cube force, one that varies as the inverse cube of r. In Proposition 45 Newton extended his theorem to arbitrary central forces by assuming that the particle moved in nearly circular orbit.As noted by astrophysicist Subrahmanyan Chandrasekhar in his 1995 commentary on Newton's Principia, this theorem remained largely unknown and undeveloped for over three centuries. Since 1997, the theorem has been studied by Donald Lynden-Bell and collaborators. Its first exact extension came in 2000 with the work of Mahomed and Vawda.
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