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Copyright © 2010 Pearson Canada Inc., Toronto, Ontario. All rights
Copyright © 2010 Pearson Canada Inc., Toronto, Ontario. All rights

... All rights reserved. This publication (work) is protected by copyright. You are authorized to print one copy of this publication (work) for your personal, non-commercial use only. See Terms of Use for more information. Permission should be obtained from the publisher prior to any prohibited reproduc ...
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2gravity a new concept

... 4. Time dilation moving clocks are measured to tick more slowly than an observer's "stationary" clock. 5. Length contraction: Objects are measured to be shortened in the direction that they are moving with respect to the observer. 6. Mass – Energy equivalence: E = mc2, energy and mass are equivalent ...
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... When computer idle, screensaver does ‘real work’. American Physical Society (APS) will publicize as part of World Year of Physics (WYP) 2005 activities, and will help with web site & graphics. Use infrastructure/help from SETI@home developers for the distributed computing parts. Goal: pulsar searche ...
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... Initially, of course, α ≪ 1. But during the collapse, both R and M would decrease and Eq.(10) would show that, as z → ∞, α would increase dramatically, α → 1, at a sufficiently high z. At this stage the collapse would degenerate into a secular quasistatic contraction by the very definition of Led . ...
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Hands-On Universe/Modeling

... • What happened? Why did this occur? • What factors influence the strength of the gravitational force in a situation like this? • How would this event differ if we were to repeat it while standing on the surface of the moon? Why? Additional background discussion might focus on the concept of force ( ...
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PowerPoint Presentation - 5. Universal Laws of Motion

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... Lecture and reading material are both included. My goal is to test for understanding of the concepts we have discussed, and how they fit together. • Study tips. We have covered a lot of material in a short time, so here are some tips on how to approach your studies for the exam. – Topics covered in ...
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... Predict the bending of light passing in the vicinity of the massive objects First observed during the solar eclipse of 1919 by Sir Arthur Eddington, when the Sun was silhouetted against the Hyades star cluster Their measurements showed that the light from these stars was bent as it grazed the Sun, ...
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... Gravitation is a natural phenomenon by which physical bodies attract each other due to their masses. This force occurs whenever masses are present and the two bodies need not to be in contact with each other. It is however the weakest of the fundamental forces of nature. In 1687, Sir Isaac Newton co ...
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Equivalence principle

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