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Lecture17-10
Lecture17-10

... The Moon does not crash into Earth because of its high speed. If it stopped moving, it would, of course, fall directly into Earth. With its high speed, the Moon would fly off into space if it weren’t for gravity providing the centripetal force. Follow-up: What happens to a satellite orbiting Earth a ...
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Newton`sLaws - Redwood High School

... That Professor Goddard…does not know the relation of action to reaction, and of the need to have something better than a vacuum against which to react - to say that would be absurd. Of course, he only seems to lack the knowledge ladled out daily in high schools. The New York Times, January 13, 1920 ...
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work power energy - White Plains Public Schools
work power energy - White Plains Public Schools

... shown above, a vertical distance h above the ground. It slides down an inclined track, around a circular loop of radius 0.5 m, then up another incline that forms an angle of 30o with the horizontal. The block slides off the track with a speed of 4 m/s at point C, which is a height of 0.5 m above the ...
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... The elastic potential energy is 1/2 kx2. So in the second case, ...
Review C: Work and Kinetic Energy
Review C: Work and Kinetic Energy

... effects of friction”. This means that from the outset we assume that the change in heat energy is zero. Energy is always conserved but sometimes we prefer to restrict our attention to a set of objects that we define to be our system. The rest of the universe acts as the surroundings. Our conservatio ...
1st Semester Physics Final Review
1st Semester Physics Final Review

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AS Unit G481: Mechanics

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Momentum - USU Physics

... P2 • Answer: The cue ball stops dead on impact and red ball moves forward with the same velocity (magnitude and direction) as that of the cue ball prior to impact! • Why?...Because both KE(= ½.m.v2) and momentum (m.v) are conserved on impact. • As the masses of both balls are the same the only solut ...
Energy Unit - WordPress.com
Energy Unit - WordPress.com

... The California Dept. of Education Standards I have come to understand are:  2.a. Students know how to calculate kinetic energy by using the formula E = (1/2)mv2.  2.b. Students know how to calculate changes in gravitational potential energy near Earth by using the formula (change in potential ener ...
Midway High School Science TAKS Review
Midway High School Science TAKS Review

... The Third Law. Try this at home without adult supervision. Have a friend, neighbor or total stranger hold a piece of paper vertically. Punch it with your fist as hard as you can. ...
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File - Miss Hinze`s Class

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File - Physical Science

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Review C: Work and Kinetic Energy

... Two critical points emerge. The first is that only change in energy has meaning. The initial or final energy is actually a meaningless concept. What we need to count is the change of energy and so we search for physical laws that determine how each form of energy changes. The second point is that we ...
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... T1 = m1a and T1R – T2R = − Iα We are using the minus sign with α because the pulley accelerates clockwise. Also, a = Rα. Thus, T1 = m1a and ...
Phys101 Final Code: 20 Term: 123 Monday, July 29, 2013 Page: 1
Phys101 Final Code: 20 Term: 123 Monday, July 29, 2013 Page: 1

... Figure 7 shows two particles of masses, m and 2m fixed in their positions. A particle of mass m is to be brought from an infinite distance to one of the three locations, a, b and c. Rank these three locations according to the magnitude of the net work done by the gravitational force on this particle ...
Unit 6 Work and Energy Student Notepack
Unit 6 Work and Energy Student Notepack

... We have seen in the previous notes how to find work… W = (F)(cosϴ)(d) But how will we find time, t ?... The most common way will be to use kinematics and the kinematic equations: (vi, vf, d, a, t)’s…. So keep those equations handy Finally… If we go back to the other uses of power like political or m ...
Center of Mass and Linear Momentum
Center of Mass and Linear Momentum

Newton`s Laws of Motion
Newton`s Laws of Motion

... scientist and mathematician famous for his discovery of the law of gravity also discovered the three laws of motion. He published them in his book Philosophiae Naturalis Principia Mathematica (mathematic principles of natural philosophy) in 1687. Today these laws are known as Newton’s Laws of Motion ...
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Relativistic mechanics

In physics, relativistic mechanics refers to mechanics compatible with special relativity (SR) and general relativity (GR). It provides a non-quantum mechanical description of a system of particles, or of a fluid, in cases where the velocities of moving objects are comparable to the speed of light c. As a result, classical mechanics is extended correctly to particles traveling at high velocities and energies, and provides a consistent inclusion of electromagnetism with the mechanics of particles. This was not possible in Galilean relativity, where it would be permitted for particles and light to travel at any speed, including faster than light. The foundations of relativistic mechanics are the postulates of special relativity and general relativity. The unification of SR with quantum mechanics is relativistic quantum mechanics, while attempts for that of GR is quantum gravity, an unsolved problem in physics.As with classical mechanics, the subject can be divided into ""kinematics""; the description of motion by specifying positions, velocities and accelerations, and ""dynamics""; a full description by considering energies, momenta, and angular momenta and their conservation laws, and forces acting on particles or exerted by particles. There is however a subtlety; what appears to be ""moving"" and what is ""at rest""—which is termed by ""statics"" in classical mechanics—depends on the relative motion of observers who measure in frames of reference.Although some definitions and concepts from classical mechanics do carry over to SR, such as force as the time derivative of momentum (Newton's second law), the work done by a particle as the line integral of force exerted on the particle along a path, and power as the time derivative of work done, there are a number of significant modifications to the remaining definitions and formulae. SR states that motion is relative and the laws of physics are the same for all experimenters irrespective of their inertial reference frames. In addition to modifying notions of space and time, SR forces one to reconsider the concepts of mass, momentum, and energy all of which are important constructs in Newtonian mechanics. SR shows that these concepts are all different aspects of the same physical quantity in much the same way that it shows space and time to be interrelated. Consequently, another modification is the concept of the center of mass of a system, which is straightforward to define in classical mechanics but much less obvious in relativity - see relativistic center of mass for details.The equations become more complicated in the more familiar three-dimensional vector calculus formalism, due to the nonlinearity in the Lorentz factor, which accurately accounts for relativistic velocity dependence and the speed limit of all particles and fields. However, they have a simpler and elegant form in four-dimensional spacetime, which includes flat Minkowski space (SR) and curved spacetime (GR), because three-dimensional vectors derived from space and scalars derived from time can be collected into four vectors, or four-dimensional tensors. However, the six component angular momentum tensor is sometimes called a bivector because in the 3D viewpoint it is two vectors (one of these, the conventional angular momentum, being an axial vector).
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