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    MAE 241 - Statics

    Summer 2009

    Dr. Konstantinos A. Sierros

    Office Hours: M and W 10:30 11:30 (263 ESB new add)

    [email protected]

    Teaching Blog: http://wvumechanicsonline.blogspot.com

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    Textbook

    R. C. Hibbeler, STATICS, 12th Edition, Pearson Prentice Hall, NewJersey USA, 2004, ISBN 0-13-607790-0

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    Schedule

    Week Day Lecture/Class Topic Assignments/Problems

    M General introduction, Units, Methodology, Introduction to force vectors (1.1-2.1) Ch 1T Vector operations, Cartesian Vectors, Addit ion of Cartesian vectors (2.1-2.6) 2.1-2.6

    1 W Position vectors, Dot product, Condition for particle equillibrium (2.7-3.1) 2.7-3.1

    R Free body diagrams, Coplanar force systems, 3D force systems (3.2-3.4) 3.2-3.4

    M Moment of a force, Cross product, Vector formulation, Principle of moments (4.1-4.4)4.1-4.4

    T Moment of a couple, Simplification of force-couple systems (4.5-4.9) 4.5-4.9

    2 W Rigid body equill ibrium, Free body diagrams, Equations of equill ibrium (5.1-5.3) 5.1-5.3

    R Force members, Free body diagrams, Equillibrium, Constraints (5.4-5.7) 5.4-5.7

    M Exam 1 and Simple trusses (6.1)T Method of joints, sections (6.1-6.4) 6.1-6.4

    3 W Space trusses, frames and machines (6.5-6.6) 6.5-6.6

    R Internal forces, Shear and moment equations (7.1-7.2) 7.1-7.2

    M Distributed loads, shear and moment relations, cables (7.3-7.4) 7.3-7.4

    T Dry friction, Wedges, Frictional forces on screws (8.1-8.4) 8.1-8.4

    4 W Frictional forces on flat belts, bearing, disks, rolling resistance (8.5-8.8) 8.5-8.8

    R Review 1 Revice Ch 1-8

    M Exam 2 and Center of gravity, mass centroid (9.1) 9.1

    T Composite bodies, Pappus and Guldinus (9.1-9.3) 9.1-9.3

    5 W Distributed loading, fluid pressure (9.4-9.5) 9.4-9.5

    R Moments of inertia, Parallel ax is theorem, Radius of gyration (10.1-10.3) 10.1-10.3

    M Composite areas, product of inertia,inclined axes (10.4-10.6) 10.4-10.6

    T Mohr's circle and start of final review (10.7) 10.7 (Revice Ch 1-10)

    6 W Review 2 Revice Ch 1-10

    R Final exam

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    Chapter 1: General principles

    Objectives

    Intro to the basic quantities and

    idealizations of mechanicsNewtons laws

    SI unit system

    Numerical calculations procedure

    General guide for problem solving

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    1.1 Mechanics

    Mechanics is a branch of physics that is concerned with the state of

    rest or motion of bodies that are subjected to the action of forces

    Mechanics

    Rigid-body

    Deformable-body

    Fluid

    Rigid-body mechanics

    Statics Dynamics

    Statics deals with the equilibrium of bodies that are either at rest

    or move with constant velocity. Dynamics is dealing with bodies

    in accelerated motion

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    History

    Archimedes

    (287-212 B.C.)

    Lever principle

    Galileo Galilei

    (1564-1642.)Pendulums, falling

    bodies

    Newton

    (1642-1727)

    3 Fundamental laws

    Euler

    DAlembert

    Langrange

    and others

    The subjects of statics developed very early in history because its

    principles can be formulated simply from measurements of geometryand force

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    1.2 Fundamental concepts

    Basic quantities Length is used to locate the position of a point in

    space and describe the size of a physical system

    Time is conceived as a succession of events

    Mass is a measure of a quantity of matter that is

    used to compare the action of one body with that

    of another

    Force is considered as push or pull exerted by

    one body or another.

    - Direct contact (eg. A person pushing a wall)- Distant action (gravitational, electrical, magnetic

    forces)

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    1.2 Fundamental concepts

    Idealizations

    We use some idealizations in order to simplify the

    application of theory

    Particle: It has a mass, but its size can be neglected

    (eg size of earth is insignificant as compared to the size

    of its orbit)

    When a body is modelled as a particle, mechanics

    become simpler since the geometry of the body is not

    involved in the analysis of the problem

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    1.2 Fundamental concepts

    Idealizations

    A Rigid body can be considered as a combination of a large number of

    particles in which all the particles remain at a fixed distance from one

    another, both before and after applying a load

    A Concentratedforce represents the effect of a loading which is assumed

    to act at a point on a body. (eg. Contact force between wheel and ground)

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    Newtons three laws of motion

    The basis of engineering mechanics is formed by Newtons three laws

    of motion. These laws, based on experimental observation, apply to

    the motion of a particle as measured from a nonacceleratingreference

    frame.

    1st LawA particle originally at rest, or moving in

    a straight line with constant velocity, tends to

    remain in this state provided the particle is notSubjected to an unbalanced force

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    Newtons three laws of motion

    2nd LawA particle acted upon by an unbalancedforce F experiences an

    acceleration a that has the same direction as the force and a magnitude

    directly proportional to the force

    F = ma

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    Newtons three laws of motion

    3rd LawThe mutual forces of action and reaction between two particles

    are equal, opposite, and collinear

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    Newtons law of gravitational attraction

    F is force of gravitation between two particles

    G is constant of gravitation measured

    experimentally, G=66.73*10-12 m3/(kg s2)

    m1,m2 represent the mass of each particle

    r is the distance between the two particles

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    Newtons law of gravitational attraction

    Weight

    According to the equation described, any two particleshave a mutual attractive (gravitational) force acting between them

    For a particle located at the surface of the earth (or close enough) the

    only gravitational force, of significant magnitude, is that between the

    earth and the particle. This force is termed weight.

    If we put m1 = m and m2 =Me (mass of earth) and r is distance between

    the particle and the earths center

    Letting g=GMe/r2, then W = mg

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    Units of measurement

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    Conversion of units

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    The International System of units

    SI is used throughout

    Rules for use

    (please read carefully page 10)

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    Numerical calculations

    Dimensional homogeneity: Each term in an equation must be expressed

    in the same unitsSignificant figures:Number of significant figures determines accuracy of

    the number. Use engineering notation.

    Rounding off numbers: Any numerical figure ending in five or greater is

    rounded up and a number less less than five is rounded downCalculations: Do not round off calculations until expressing the final

    result. Round off the answer to three significant figures

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    General procedure for analysis

    Read the problem carefully and correlate physical situation with

    theory

    Tabulate the problem data and draw diagrams

    Apply the relevant principles, generally

    with equations

    Solve the equations and report the answer

    Judge the answer in technical terms and

    common sense to determine whether the

    answer seems reasonable

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    Chapter 2:Force vectors

    Objectives

    To show how to add forces and

    resolve them into components

    using the Parallelogram Law

    Cartesian vectors

    Introduce dot product

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    2.1 Scalars and vectors

    Ascalaris any positive or negative physical quantity that can becompletely specified by its magnitude (eg. length, mass, time)

    A vectoris any physical quantity that requires both a magnitude

    and a direction for its complete description (eg. force, moment)