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Newton`s Laws - Galileo and Einstein
Newton`s Laws - Galileo and Einstein

South Pasadena · AP Chemistry
South Pasadena · AP Chemistry

... describe the curved path of a projectile using the motion of an object in freefall for the vertical component and the motion of an object moving in a straight line for the ...
Balloon Racer Unit Overview Unit Title: Force and Motion Lesson
Balloon Racer Unit Overview Unit Title: Force and Motion Lesson

... find acceleration. The formula for acceleration is: a=υ/t. It is the velocity divided by the time. Acceleration is the speeding up or the slowing down of an object (pressing the accelerator in your car or pressing the brakes). Let’s see how much force was applied to your balloon. State the 2nd Law o ...
Chapter 4: Newton`s Second Law F = ma First Law
Chapter 4: Newton`s Second Law F = ma First Law

Impulse and Momentum
Impulse and Momentum

... 3. Each of the following situations describes the initial and final velocities of identical baseballs. Rank the magnitudes of the impulse for each case from greatest to smallest. A. Vi = 0 Vf = 20 m/s to the right B. Vi = 25 m/s to the right Vf = 40 m/s to the right C. Vi = 30 m/s to the left Vf = 1 ...
Laws of Motion Notes
Laws of Motion Notes

... For every action force there is an equal in magnitude but opposite in direction reaction force. - Force pairs, actions and reactions, come from interactions - Interaction: two surfaces come in contact with one another - For example: There is an interaction occurring right now between the chair and y ...
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... moving at 30 mph on a straight road. When the driver suddenly slams on the brakes, the bus comes to a stop. The passengers were all moving 30 mph. Newton’s first law says this motion can only be changed by applying a force. The brakes provide this force for the bus and anything attached to it. When ...
South Pasadena
South Pasadena

... d) What happens to her angular speed when she moves to the edge? ________________ ...
The Milky Way: Home to Star Clusters
The Milky Way: Home to Star Clusters

REVIEW: (Chapter 12) Newton`s Law of Gravity
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... level, to think of the Sun as a point mass in Newton’s Universal Gravity Law as a function of distance r away from the center of the Sun FG (r) = Gmp MS /r2 In fact even if the Sun’s radius were almost the orbital radius of the Earth, it is exactly correct to regard the Sun’s mass as all at its cent ...
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Hubble’s Law31 Oct 10/31/2011
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... • They move according to Hubble’s Law. • We will answer these questions by analyzing  the motion of 3 galaxies. – Was there a Big Bang? – Are we at the center of the Big Bang? – Why are galaxies moving? – How long ago did the big bang occur? ...
Jeopardy - Forces - Western Reserve Public Media
Jeopardy - Forces - Western Reserve Public Media

Classical mechanics: conservation laws and gravity
Classical mechanics: conservation laws and gravity

... A. The rocket exerts a force on the ground, and then the atmosphere, causing it to accelerate upward. B. The backward momentum of the rocket exhaust is canceled by the forward momentum of the rocket. C. The escaping rocket exhaust changes the mass of the rocket, giving it upward momentum. D. The bur ...
SCI 101 - Onondaga Community College
SCI 101 - Onondaga Community College

... 14) A cannonball is fired straight up at 50 m/s. Neglecting air resistance, when it returns to its starting point its speed A) is 50 m/s. C) is less than 50 m/s. B) is more than 50 m/s. D) depends on how long it is in the air. ...
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Why Aren`t All Galaxies Barred?

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Review for the Final Exam

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... Mass of the universe is dominated by invisible dark matter. The mass of lens’s constituent particles and their crosssection affect the distribution of dark matter in lens systems. Thus it is possible to determining how much dark matter they contain ...
Lab M14 – Pulleys
Lab M14 – Pulleys

... 5. Now suppose that you raise the hanging mass by 10 centimeters. Through how much distance must you exert the effort force ? On your prelab diagram, clearly label the effort and load distances for this situation, and write a short explanation of why those two distances are not equal. ...
CosmologyL1
CosmologyL1

... Galaxy, thus demonstrating that our Galaxy is not the Universe. • Resolution of the Baade demonstrated that MW is a typical galaxy. Contemporary LSS studies and CMB results: At large scales the Universe looks the same wherever you are. In 1917 Einstein invented the cosmological constant as a term in ...
Gravity Powerpoint
Gravity Powerpoint

... • How much do objects accelerate as they fall? • Near the surface of Earth, the acceleration due to gravity is 9.8 m/s2. • This means that for every second an object is falling, its velocity increases by 9.8 m/s. ...
NASA Explorer Schools - NSTA Learning Center
NASA Explorer Schools - NSTA Learning Center

... An object at rest will stay at rest, and an object in motion will stay in motion at constant velocity, unless acted upon by an unbalanced force. ...
1. Find the weight of a 2.3 kg bowling ball on Earth.
1. Find the weight of a 2.3 kg bowling ball on Earth.

... to verify experimentally?  ...
Diapositiva 1
Diapositiva 1

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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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