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PPT
PPT

... Good, the moment of inertia has the smallest value for rotation about the center of mass! Any other axis will give a larger moment of inertia. When we say “moment of inertia” we’re not finished. We always have to say — or think — “moment of inertia about some particular axis of rotation”. ...
Primordial Planet Formation - University of California San Diego
Primordial Planet Formation - University of California San Diego

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Goal: To understand the structure and makeup of our own Milky Way

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Newton`s Laws - Ccphysics.us
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Rotational Equilibrium and Dynamics - Faculty
Rotational Equilibrium and Dynamics - Faculty

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Teaching Forces and Motion with Confidence I.O.P day @ Rugby

Simple Pendulum Lab - northwoodschool.org
Simple Pendulum Lab - northwoodschool.org

... planets and lunar eclipses, and a host of other astronomical phenomena recur with a more or less complicated regularity. Early man was certainly aware of this recurrence, and it had a religious significance for him. Numerous temples, such as the impressive Stonehenge monument in England, were constr ...
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Chapter 5 – Newton`s Laws of Motion I

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Lecture 2c - Newton`s Laws & Applications
Lecture 2c - Newton`s Laws & Applications

... is zero, it will remain either at rest or moving in a straight line at constant speed. • Newton’s second law: • Newton’s third law: • Weight is the gravitational force on an object. • Free-body diagrams are essential for problemsolving. Do one object at a time, make sure you have all the forces, pic ...
Part III
Part III

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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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