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PPA6_Lecture_Ch_07
PPA6_Lecture_Ch_07

F - etsu
F - etsu

Inertia
Inertia

Lecture PowerPoints Chapter 7 Physics
Lecture PowerPoints Chapter 7 Physics

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... that Acceleration (of the same mass) is decreased, what must that mean about the force given? IT DECREASED. IN FACT- This relationship is Directly Proportional. This means that if you DOUBLE the force on a given mass (that must be constant), then the acceleration will DOUBLE Same goes for if you wer ...
Jeopardy
Jeopardy

Dynamics Powerpoint - HRSBSTAFF Home Page
Dynamics Powerpoint - HRSBSTAFF Home Page

... because of its inertia (until the back of the seat applies a forward force to make it move with the bus). From the point of view of someone on the bus, it appears that the package is moving backward; however, someone watching from outside the bus would see the bus move forward and the package trying ...
Chapter 8
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... Physics--Chapter 8: Rotational Equilibrium and Dynamics Practice Problems 5. The entrance of a science museum features a funnel into which marbles are rolled one at a time. The marbles circle around the wall of the funnel, eventually spiraling down into the neck of the funnel. The internal radius o ...
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... other galaxies: discovered in the LMC/SMC, M31, and another ~15 galaxies (all spirals) a handful of point X-ray sources (< 10) long-standing problems with low angular resolution and source confusion > XLF reliably constructed only for M31 and M101 > 'super-Eddington' sources were tentatively identif ...
California Physics Standard 1a Send comments to: layton@physics
California Physics Standard 1a Send comments to: layton@physics

... After establishing the ratio of the masses of the two objects you plan to drop (27 in the case above) discuss with your students if they think the larger object will fall “27” times faster than the smaller object. They probably will disagree but this was one of the arguments Galileo suggests in his ...
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... the harder you push on a cart, the faster it goes. However, according to Newton, the force merely changes the velocity. It is the acceleration, not the velocity, that is proportional to the force. Also, what does the mass of the cart have to do with how the motion changes? We know that it takes a mu ...
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2016-2017 Chapter 6 review

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... Galaxies like the Milky Way are believed to form by • the infall of gas which then turns gradually to stars (most of which form in the disk of the Galaxy, in open star clusters which quickly dissolve), and also by • the accretion of smaller galaxies which become absorbed in the larger system. A majo ...
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POP4e: Ch. 1 Problems

... The gravitational force exerted on an astronaut on Earth’s surface is 650 N down. When she is in the International Space Station, is the gravitational force on her (a) larger, (b) exactly the same, (c) smaller, (d) nearly but not exactly zero, or (e) exactly zero? According to Newton’s law of univer ...
2013 Physics I can statements
2013 Physics I can statements

... 3. I can use Newton’s Laws of Motion to describe how forces affect the motion of an object.   a. I can define and apply Newton’s First Law of Inertia.   i. Objects in motion will stay in motion and objects at rest will stay at rest unless acted upon by an outside force.   ii. I can define ine ...
Searching for stars in high-velocity clouds
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... does not rule out the scenario proposed by Braun & Burton (1999) and Blitz et al. (1999), but it does rule out HVCs being of the same class of object as the other known dwarf galaxies. If extragalactic then for some reason these H I clouds, unlike other dwarf galaxies, have not formed many (if any) ...
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... When in doubt, Newton • Your body’s inertia wants to keep going in a linear direction. Which is why you tend to tilt away from the center of axis on a curve. • This is often labeled as centrifugal force, but it is NOT a proper force. ...
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... The disk of the Milky Way measures The Milky Way is about 100,000 light-years in diameter. more than 100,000 light-years in diameter. The bulge of densely packed stars at the center is located about 26,000 light-years from the Sun. A large but very faint layer of stars surrounds the disk and bulge. ...
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Physics Benchmark Exam #1 2008-2009
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... 9. Equilibrium exists in a system where three forces are acting concurrently on an object. If the system includes a 5.0-newton force due north and a 2.0-newton force due south, the third force must be: A B C D ...
Lecture 13.1
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Dynamics Homework
Dynamics Homework

... 22. * Referring to the last question, when astronauts walked on the Moon they wore heavy spacesuits. What does the effect of mass and weight on the Moon mean about their physical activity on the Moon? 23. * (a) Can a normal force on an object be directed horizontally? If not, why not? If so, give an ...
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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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