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The Nature of Force
The Nature of Force

Bell Work 2/23/10
Bell Work 2/23/10

... Newton’s first law of motion is sometimes called the law of inertia. Inertia is “want to,” when an object resists change because it “wants to” keep going in a straight line. Inertia depends on an object’s mass. The more mass an object has, the more inertia an object has. ...
Chapter 3 Review
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gravity ppt - District 196
gravity ppt - District 196

... Given: r = 2.1 x 105 m + 6.37 x 106 m = 6.58 x 106 m mearth = 5.98 x 1024 kg Unknown: Fg Equation: F = ma, now Fg = mg (We need g at that altitude.) Fg = Fg mg = G m1 m2 r2 g=Gm r2 = (6.67 x 10-11 N m2/kg2)(5.98 x 1024 kg) (6.58 x 106 m)2 = 9.21 m/s2 ...
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... 2. Do you see any relationship between the mass of the car and its velocity? (If mass increases, does velocity increase?) 3. If a semi-truck and a Honda Civic were to hit a block wall going at the same velocity, which would hit the wall with a greater force? Use Newton’s 2nd Law to answer this. 4. F ...
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... • Newton’s 1st Law of Motion – Objects in motion will stay in motion and objects at rest will stay at rest…unless a force acts on them. The ball will stay at rest (not move) unless the dog moves it. ...
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Section 1 Forces Newton`s Second Law
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PHYSICS SAE 4

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Newton`s Laws (powerpoint)

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Lecture 16: Centripetal Acceleration, ac = v 2/r

Newtons Laws and projectile motion
Newtons Laws and projectile motion

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ISCI 2002 Quiz Chapter 3 – Newton`s Laws of Motion

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9.2.3 Gravity in Space
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Newton`s Laws
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Today`s Powerpoint
Today`s Powerpoint

... Newton’s laws of motion explain how objects interact with the world and with each other. Newton’s first law: An object at rest will remain at rest, and an object will move in a straight line at constant speed if and only if the sum of forces that act on it are balanced. ...
Newton`s Law of Universal Gravitation
Newton`s Law of Universal Gravitation

... Newton’s Law of Universal Gravitation In 1666, some 45 years after Kepler did his work, 24-year-old Isaac Newton used mathematics to show that if the path of a planet were an ellipse, which was in agreement with Kepler’s first law of planetary motion, then the magnitude of the force, F, on the plan ...
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Modified Newtonian dynamics



In physics, modified Newtonian dynamics (MOND) is a theory that proposes a modification of Newton's laws to account for observed properties of galaxies. Created in 1983 by Israeli physicist Mordehai Milgrom, the theory's original motivation was to explain the fact that the velocities of stars in galaxies were observed to be larger than expected based on Newtonian mechanics. Milgrom noted that this discrepancy could be resolved if the gravitational force experienced by a star in the outer regions of a galaxy was proportional to the square of its centripetal acceleration (as opposed to the centripetal acceleration itself, as in Newton's Second Law), or alternatively if gravitational force came to vary inversely with radius (as opposed to the inverse square of the radius, as in Newton's Law of Gravity). In MOND, violation of Newton's Laws occurs at extremely small accelerations, characteristic of galaxies yet far below anything typically encountered in the Solar System or on Earth.MOND is an example of a class of theories known as modified gravity, and is an alternative to the hypothesis that the dynamics of galaxies are determined by massive, invisible dark matter halos. Since Milgrom's original proposal, MOND has successfully predicted a variety of galactic phenomena that are difficult to understand from a dark matter perspective. However, MOND and its generalisations do not adequately account for observed properties of galaxy clusters, and no satisfactory cosmological model has been constructed from the theory.
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