'Point mass' diaporamas de présentation

CONTINUOUS DYNAMICS & SECURITY

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DEC 1013 ENGINEERING SCIENCEs

DEC 1013 ENGINEERING SCIENCEs. 2. KINEMATICS AND KINETICS. NAZARIN B. NORDIN nazarin@icam.edu.my. What you will learn:. Distance and displacement Speed and velocity Acceleration Distance vs. time graph: interpret slope as speed

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Chapter 9

Chapter 9. Rotation of Rigid Bodies. Goals for Chapter 9. To describe rotation in terms of: angular coordinates ( q ) angular velocity ( w ) angular acceleration ( a ) To analyze rotation with constant angular acceleration

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An Efficient Brush Model for Physically-Based 3D Painting

An Efficient Brush Model for Physically-Based 3D Painting. Nelson S.-H. CHU (cpegnel@ust.hk) Chiew-Lan TAI (taicl@ust.hk) The Hong Kong University of Science and Technology October 9, 2002, Beijing, China. Input: Brush movements. Simulation of Brush & ink. Output: Realistic brushwork.

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Ontologies and Representations of Matter

Ontologies and Representations of Matter. Ernest Davis AAAI 2010 July 14, 2010. Gas in a piston. Figure 1-3 of The Feynmann Lectures on Physics. The gas is made of molecules. The piston is a continuous chunk of stuff.

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Ontologies and Representations of Matter

Ontologies and Representations of Matter. Ernest Davis AAAI 2010 July 14, 2010. Gas in a piston. Figure 1-3 of The Feynmann Lectures on Physics. The gas is made of molecules. The piston is a continuous chunk of stuff.

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Chapter 5 Review: Gases

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Pendulum

Pendulum. Simple Harmonic Motion. Pendulum. A simple pendulum is one which can be considered to be a point mass suspended from a string or rod of negligible mass. It is a resonant system with a single resonant frequency. Characteristics of a Pendulum. L = Length M = Mass T = Period

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Rotation and Inertia

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Rotation and Inertia

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Graphene NEMS at the Chalmers Condensed Matter Theory Group

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Analysis of Trans-Lunar Spiral Trajectory

February 12, 2009. Analysis of Trans-Lunar Spiral Trajectory. 1. Spiral Transfer. Equations of Motion (EOM)s :. r: distance from central body to spacecraft (s/c) ? : Gravitational parameter (G*M) ? : Angle of rotation T: Thrust from engine m: Mass of spacecraft. Assumes:

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How Well Can We Measure Neutron Star Radii?

How Well Can We Measure Neutron Star Radii?. Cole Miller University of Maryland. Collaborators: Romain Artigue , Didier Barret , Sudip Bhattacharyya, Stratos Boutloukos , Novarah Kazmi , Fred Lamb, Ka Ho Lo. Measuring stellar radii. Ordinary star, like the Sun

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Pendulums and Resonance

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Kinematics Point Mass Dynamics

Kinematics Point Mass Dynamics. Motion of a Point Mass. change in position d (this can be either x or y) change in speed dv (this can be either vx or vy). d = d + dv*dt + 0.5*da*dt*dt dv = dv + da*dt. Polar to Cartesian Coordinates. x = r * COS(rads) y = r * SIN(rads).

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Arnando Shastrini Minnesota State University Moorhead

Quantitative presentation example: Does a paper ball and scotch tape pendulum behave like an ideal pendulum?. Arnando Shastrini Minnesota State University Moorhead. Introduction. Laws of pendulum motion first developed by Galileo

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