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Chapter 4
Chapter 4

... where Utangent is the tangential velocity of the surface. In the 19th century, during the period of the original formulation of the Navier Stokes equations, the validity of this condition was in doubt. Experimental verification was uncertain and Stokes himself, who felt the no slip condition was the ...
Physics Curriculum Map - Norwell High School SUBJECT: Physics
Physics Curriculum Map - Norwell High School SUBJECT: Physics

...   Interpret and apply Newton’s three laws of motion.   Use a free-body force diagram to show forces acting on a system consisting of a  unbalanced forces? pair of interacting objects. For a diagram with only co-linear forces, determine the     net force acting on a system and between the objects. Ho ...
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... Simple harmonic motion is a type of periodic motion where the restoring force on a mass is directly proportional to the displacement. The displacement of the mass has a sinusoidal dependence on the elapsed time, i.e. depends on time through a sine or cosine function. ...
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... IDENTIFY: The mechanical energy of the roller coaster is conserved since there is no friction with the track. We must also apply Newton’s second law for the circular motion. SET UP: For part (a), apply conservation of energy to the motion from point A to point B: K B  Ugrav,B  K A  Ugrav,A with ...
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... divided by the elapsed time Δt equals the constant net force Fnet acting on the object If a constant force acts on a object. The impulse I delivered to the object over a time interval Δt is given by: I = F Δt SI unit: kg m/s (ex 6.2/163) ...
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... The body of a 1275 kg car is Supported on a frame by four springs Each of which has a constant of 2 X 104 . 2 people riding in the car Have a combined mass of 153 kg. Find the period of Vibration of the car when it is Driven over a pothole on the road? T = 0.84s ...
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... Ground Displacement and Acceleration Consider the situation in which the system vibrates because of motion introduced at the base of the system, not by a force applied to the mass. The system is shown at the right. The forces exerted by the spring and the dashpot on the mass are functions of the rel ...
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... The goal of this experiment is to investigate the relationship between force, mass and acceleration. You will be verifying a powerful physical law well known as Newton's second law. F = ma You will also be comparing the gravitational mass of an object with its inertial mass. Where: m=W/g (gravitati ...
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... 6. The difference between speed and velocity is that velocity indicates the ____________________ of motion and speed does not. 7. Freely falling objects accelerate at 9.8 m/s2 because the force of ____________________ acts on them. 8. Accelerated motion is represented by a(an) ____________________ l ...
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Special cases of the three body problem
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... small and moves in the same plane (approximated by the Sun-Earth-Moon system and many others). The restricted problem (both circular and elliptical) was worked on by many famous mathematicians and physicists. In the circular problem, with respect to a rotating reference frame, the two co-orbiting bo ...
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... 1. If a car travels 400m in 20 seconds, how fast is it going? 20 m/s 2. A plane travels 395,000 meters in 9000 seconds, what is it’s speed? 43.89 m/s 3. You arrive to my class 45 seconds after leaving math which is 90 meters away. How fast did you travel? 2 m/s 4. It takes Serina 0.25 hours to drive ...
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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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