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Tutorial_03_Newton2 - UMD Physics
Tutorial_03_Newton2 - UMD Physics

... To rescue a child who has fallen down a well, rescue workers fasten him to a rope, the other end of which is then reeled in by a machine. The rope pulls the child straight upward at steady speed. The child weighs 250 newtons, which means gravity pulls him downward with 250 newtons of force. A. (Work ...
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- Review the Law of Interaction and balanced forces within bodies

... hooks (totalling 2 N.) Springs in the scales pulling upward (2 N. total) Also a pair of opposing forces between hands and the scale (not shown) ...
Circular Motion
Circular Motion

... At point B there are also two forces but both acting in opposite directions. Using the same coordinate system. vB 2 FR  maR  m r FR  FTB  mg vB 2 m  FTB  mg r vB 2 FTB  m(  g) r Now since we were given vB  6.56m / s, (6.56m / s) 2 FTB  0.150kg (  9.80m / s 2 ) 1.10m FTB  7.34 N ...
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File - Flipped Out Science with Mrs. Thomas!

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Newton`s Second Law of Motion

... 2. If you push harder, is the change in motion smaller or larger? 3. Do you think this is a direct or inverse relationship? 4. Assume that you have a bowling ball and a baseball, each suspended from a different rope. If you hit each of these balls with a full swing of a baseball bat, which ball will ...
Free Fall - Cobb Learning
Free Fall - Cobb Learning

... • Consider an apple falling from a tree. We know that it starts at rest and gains speed as it falls, or accelerates. • Gravity causes the apple to accelerate downward and is said to be in free fall. Free fall: when an object is only affected by gravity – SI unit: m/s2 ( for acceleration due to gravi ...
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... ● Move the “semimajor axis (AU)” slider to increase/decrease the overall size of the orbit. ● Move the “eccentricity” slider to adjust how much the orbit deviates from circular shape. ● Various views are available for selection in Visualization Options window: ○ “show solar system orbits” - shows al ...
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... 5. The speed and direction of a moving object. ___________________ 6. Everything gets pulled down toward the earth’s center because of this force. _______________ 7. This is the result of unbalanced forces making an object speed up. ________________________ 8. What you get when you multiply an objec ...
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Forces - Home - West Johnston High School

... • Centripetal Force: force that keeps objects moving in a circle. • Momentum: depends on the mass and velocity of an object ▫ A large truck is going to have more momentum (be more difficult to stop) than a small truck. ▫ Newton’s Cradle ...
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Newton`s Second Law

... happens to an object’s acceleration if the force applied to the object is increased but the object’s mass remains constant? Take time to answer the ‘What Do You Think?’ question(s) in the Lab Report section. Background Newton described the relationship between acceleration, force, and mass as follow ...
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Problem 1: Second Law and projectile motion

... come from? The normal component of the contact force exerted on her by the wall supplies that centripetal acceleration. You may wonder how the wall can exert a normal force on her if there is no other force acting to press her into the wall. Ordinarily we think of contact forces arising because some ...
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Unit: Forces in Motion

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Chapter 4 Forces and Newton’s Laws of Motion continued
Chapter 4 Forces and Newton’s Laws of Motion continued

... 3. On a frictionless surface, two boxes with the masses shown are pushed together by a force with magnitude F. What is the force that the larger mass block exerts on the smaller mass block? a) F / 3 b) F / 5 c) 2F / 3 d) 3F / 5 e) 3F / 2 ...
Answers - jpsaos
Answers - jpsaos

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4-3 - mrhsluniewskiscience

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PHYSICS Sc. (Main) B.

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Chapter 1

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Circular Motion

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Robert_Minchin_Galaxies_2011_REU
Robert_Minchin_Galaxies_2011_REU

... The Observed Rotation Curve • In the 1970s, interferometers such as the VLA and WSRT observed the rotation curves of spiral galaxies • They were able to trace the rotation curves out beyond the stellar disc. • The resulting curves were flat or slightly rising, not falling as predicted ...
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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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