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Jeopardy Force
Jeopardy Force

... Answer A 9.00-kg object is moving in a circle with a constant speed of 45.0 m/s. If the circular path has a radius of 20.0 m, what is the net force on the object? F = mv²/r = (9.00kg)*(45 m/s)²/(20.0m) = 911 N ...
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Newton`s Third Law

... Force and Changing Momentum By ___________________ these two relationships, Newton’s second law can be written in this way: _____________________________________________ In this equation __________ is the final momentum and ___________is the initial momentum • Law of Conservation of Momentum The mom ...
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Chapter4- Making Sense of the Universe-pptx

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The Age of Einstein

... Fitzgerald, Larmor, and other physicists at that time considered length contraction and time dilation to be “real” effects, associated with minute physical changes in the structure of rods and clocks when in motion. It was left to the young Einstein, working as a junior Patent Officer in Bern, and t ...
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Problem Set III Solutions
Problem Set III Solutions

... In this case, you can always make m big enough to have the total force be large enough to pull M up the hill. (Please note that in solving this problem I assumed that either the system was stationary or just beginning to move. This means that mg = T by the equation of motion for m. However, once the ...
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Circular Motion

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Chapter 8 Gravitational Attraction and Unification of Forces

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Secondary Robot

... law of motion, the acceleration of an object is a quantifiable concept. We are able to use this Law of Motion to make predictions about the acceleration of an object given the net force and mass. The implications here are four fold: 1) if the net force increases and the mass stays the same the accel ...
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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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