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5 Newton`s Third Law of Motion
5 Newton`s Third Law of Motion

... ♦ The third law: – Whenever one object exerts a force on a second object, the second object exerts an equal and opposite force on the first. – Forces come in pairs, one action and the other reaction, both of which comprise the interaction between one object and the other. – Action and reaction alway ...
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4 Newton`s Second Law of Motion

...  The third law: – Whenever one object exerts a force on a second object, the second object exerts an equal and opposite force on the first. – Forces come in pairs, one action and the other reaction, both of which comprise the interaction between one object and the other. – Action and reaction alway ...
Grade 11: Physical Sciences Outline
Grade 11: Physical Sciences Outline

...  Define static frictional force, fs, as the force that opposes the tendency of motion of a stationary object relative to a surface. The static frictional force can have a range of values from zero up to a maximum value, μsN.  Define kinetic frictional force, fk, as the force that opposes the motio ...
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Balanced/Unbalanced Review File

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Newton`s third law of motion

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... 5. What are the units of work? a. J c. kgm2/s2 b. Nm d. All of the above 6. Which of the following processes requires the most work? a. A 10 kg weight rests on a table. b. A person holds a 1 kg weight still with outstretched arms. c. A person lifts a 1 kg weight 1 m off the floor. d. A 10 kg ball ...
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... The solar system (and, hence, the Earth) is about 4.54 billion years old, and this is roughly the same as the half-life of 238 U (4.5 billion years). That means that there was approximately twice as much 238 U was present when the Earth formed. In another 4.5 billion years, we’d expect only a quarte ...
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The Conservation of Energy Space-Time Metric for Space Outside

... is distorting space-time, G is Newton’s universal gravitational constant and c is the speed of light. It is rather obvious that Equation (2) behaves badly at r = α and this is the source of the concept of black holes with an event horizon at radius r = α. Einstein’s gravitational field equations wer ...
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Chapter 12 Gravity

The NET Force - University of Iowa Physics
The NET Force - University of Iowa Physics

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Gravity

Gravity or gravitation is a natural phenomenon by which all things with mass are brought towards (or 'gravitate' towards) one another including stars, planets, galaxies and even light and sub-atomic particles. Gravity is responsible for the complexity in the universe, by creating spheres of hydrogen, igniting them under pressure to form stars and grouping them into galaxies. Without gravity, the universe would be an uncomplicated one, existing without thermal energy and composed only of equally spaced particles. On Earth, gravity gives weight to physical objects and causes the tides. Gravity has an infinite range, and it cannot be absorbed, transformed, or shielded against.Gravity is most accurately described by the general theory of relativity (proposed by Albert Einstein in 1915) which describes gravity, not as a force, but as a consequence of the curvature of spacetime caused by the uneven distribution of mass/energy; and resulting in time dilation, where time lapses more slowly in strong gravitation. However, for most applications, gravity is well approximated by Newton's law of universal gravitation, which postulates that gravity is a force where two bodies of mass are directly drawn (or 'attracted') to each other according to a mathematical relationship, where the attractive force is proportional to the product of their masses and inversely proportional to the square of the distance between them. This is considered to occur over an infinite range, such that all bodies (with mass) in the universe are drawn to each other no matter how far they are apart.Gravity is the weakest of the four fundamental interactions of nature. The gravitational attraction is approximately 10−38 times the strength of the strong force (i.e. gravity is 38 orders of magnitude weaker), 10−36 times the strength of the electromagnetic force, and 10−29 times the strength of the weak force. As a consequence, gravity has a negligible influence on the behavior of sub-atomic particles, and plays no role in determining the internal properties of everyday matter (but see quantum gravity). On the other hand, gravity is the dominant force at the macroscopic scale, that is the cause of the formation, shape, and trajectory (orbit) of astronomical bodies, including those of asteroids, comets, planets, stars, and galaxies. It is responsible for causing the Earth and the other planets to orbit the Sun; for causing the Moon to orbit the Earth; for the formation of tides; for natural convection, by which fluid flow occurs under the influence of a density gradient and gravity; for heating the interiors of forming stars and planets to very high temperatures; for solar system, galaxy, stellar formation and evolution; and for various other phenomena observed on Earth and throughout the universe.In pursuit of a theory of everything, the merging of general relativity and quantum mechanics (or quantum field theory) into a more general theory of quantum gravity has become an area of research.
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