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    MPA104

    Mechanical Design

    Engineering Statics

    Duncan Price

    IPTME, Loughborough University

    Copyright: [email protected] (2006)

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    Mechanics of Materials

    Mechanics of Materials can be divided into

    three categories:

    Mechanics of Rigid Bodies Staticsbodies at rest

    Dynamicsbodies in motion

    Mechanics of Deformable Bodies

    Mechanics of Fluids

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    Statics

    Statics is thoroughly used in the analysis of

    structures, for instance in architectural andstructural engineering. Strength of materials

    is a related field of mechanics that relies

    heavily on the application of static

    equilibrium.

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    Course Content

    12 Lectures:1-5 Forces, springs

    Free body diagramsResolution of forces (tutorial sheet)

    Equilibrants and resultants offorces (tutorial sheet)

    7 Class test (calculators needed)

    8-11 Levers, moments, reactions and

    centre of gravity (tutorial sheet)12 Online test

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    5

    Newtons Laws

    Sir Isaac Newton (1642-1729)

    Principia 1687

    Formulated three laws on which all

    conventional motion is based

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    Newton I

    A particle remains at rest or continues to move

    at a constant speed in a straight line unless

    there is a constant force acting on it.

    The most important law

    The one that most people dont understand

    The only one that doesnt have an equation

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    Newton II

    The resultant force on a particle is equal to therate of change of momentum of the particle.

    amFdtvd

    mFvmdt

    d

    F ;;

    The form F=ma is only valid if the mass is

    constant.

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    Newton III

    The forces of action and reaction between

    interacting bodies are equal in magnitude and

    opposite in direction.

    BAAB FF

    The force of the Earth on the Sun has the samemagnitude as the force of the sun on the earth

    The force of a tennis ball on a racket has the same

    magnitude as the force of the racket on the ball

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    Newtons Law of Gravitation (1)

    F = G M m / r2

    Where:

    M & m are particle masses

    G is the universal constant of gravitation

    (6.673 x 10-11 m3/kg s2)

    r is the distance between the particles.

    F in Newtons (kg m/s2)

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    Newtons Law of Gravitation (2)

    On Earth:

    F = m g

    Where:

    m is the mass of the body in question (in kg)g = 9.81 m/s2

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    Spring Forces (1)

    If a spring is stretched from L0to L it exerts a force on

    the object to which it is attached:

    F = K (LL0)

    K = spring constant = force required to stretch springby unit length (N/m).

    K depends on spring material and design.

    LO

    L

    FF

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    Spring Forces (2)

    F = K (LL0) is also known as Hookes Law:The force exerted by a spring is proportional to

    its extension.

    Slope = F/ (LL0) = KF

    (L-Lo)

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    Free body diagrams (1)

    FBD is an essential step in the solution of all

    problems involving forces on bodies

    it is a diagram of the external surface of thebody - not interested in internal forces

    all other bodies in contact with the one we are

    interested in are replaced by vectors

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    Free body diagrams (2)

    Sketch of person standing

    mg

    R1 R2

    F=ma

    R1+R2-mg=ma, but no acceleration so,

    R1+R2=mg

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    Free body diagrams (3)

    sketch

    mg

    T

    free bodydiagram

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    Free body diagrams (4)

    Rules:

    clear sketches

    draw in the correct orientation show all forces acting on the body

    dont show any internal forces between

    different parts of the body show the forces not the components

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    Representation of a force by a vector

    A force has the following characteristics:

    Magnitude

    Direction Point of application

    A quantity which has magnitude and direction is

    a vector.A quantity which has magnitude only is a scalar.

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    Vector addition

    F1F2

    F3

    F1

    F2

    F3FT

    These three forces act together

    on the particle. Their effect isequivalent to a single force

    which is the vector sum of the

    forces.

    FTis the resultant of the

    forces F1, F2and F3

    FT=F1+F2+F3

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    Trigonometry (1)

    A

    B

    C

    Pythagoras

    Theorem:

    A2= B2+ C2

    Internal anglesof a triangle

    add up to 180

    90 -

    90

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    Trigonometry (2)

    A

    (hypotenuse) B(opposite)

    C

    (adjacent)

    sine() = B/Acosine() = C/Atangent() = B/C

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    Trigonometry (3)

    sin(45) = 1/2 = 0.707

    cos(45) = 1/2 = 0.707

    tan(45) = 1/1 = 1

    sin-1(0.707) = 45

    cos-1(0.707) = 45

    tan-1(1) = 45

    2 m

    1 m

    1 m

    45

    45

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    Trigonometry (4)sin(30) = 1/2 = 0.5

    cos(30) = 3/2 = 0.866

    tan(30) = 13 =0.577

    sin(60) = 3/2 = cos(30)

    cos(60) = 1/2 = sin(30)tan(60) = 3/1 = 1.73

    Generally:

    cos() = sin(90- )

    tan() = sin()/cos()

    sin2() + cos2() = 1

    1 m

    2 m

    3m

    30

    60

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    -1

    -0.8

    -0.6

    -0.4

    -0.2

    0

    0.2

    0.4

    0.6

    0.8

    1

    -360 -315 -270 -225 -180 -135 -90 -45 0 45 90 135 180 225 270 315 360

    Sine and Cosine functions

    sin()

    cos()

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    -10

    -8

    -6

    -4

    -2

    0

    2

    4

    6

    8

    10

    -90 -45 0 45 90

    Tangent function

    tan()

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    Resolving forces (1)

    Forces can be broken down into any number ofcomponent forces

    It is often convenient to choose two

    perpendicular directions for resolution

    FFy

    F = Fx+Fy

    F = (Fx2+Fy

    2)1/2

    Scalar magnitudesFX

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    Resolving forces (2)

    F

    Fx

    Fy

    Fx=F cos

    Fy=F sin

    =tan-1(Fy/Fx)

    If the components are

    perpendicular, they may

    be added independently

    F1F2

    F3

    FT=F1+F2+F3 FTx=F1x+F2x+F3x FTy=F1y+F2y+F3y

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    Resolving forces (3)

    500 N

    30Fx=500 cos 30

    = 433 N

    Fy=500 sin 30

    = 250 N

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    Resolving forces (4)

    FTx= F1x+F2x+F3x

    = 20050 cos 30 + 80 cos 80

    = 171 N

    FTy= F1y+F2y+F3y

    = 050 sin 3080 sin 80

    = - 104 N (i.e. downwards)

    F1= 200 N

    F2 = 50 N

    F3= 80 N

    30

    80

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    Resolving forces (5)Fx = 171 N

    Fy= 104

    N

    FT= (Fx2+Fy2)

    = (1712+ 1042)

    = 200 N

    = tan-1

    (Fy/Fx)

    = tan-1(-104/171)

    = -31

    FT

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    Resolving forces (6)

    30 75

    100 N

    A

    B C horizontal components:

    FACcos75 = FABcos30

    FAC= FAB(cos30/cos75)

    vertical components:

    FACsin75 + FABsin30 = 100 N

    FAB

    (cos30/cos75)sin75 + FAB

    sin30 = 100

    FAB= 26.8 N FAC= 89.7 N

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    Resultant

    If two or more forces at a point they can bereplaced by a single force known as a

    resultant.

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    Equilibrium

    When two or more forces act upon a body and

    are so arranged that the body remains at rest

    or moves at a constant speed in a straightline*, the forces are said to be in equilibrium.

    * i.e. Newtons 1stlaw

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    Y-hangs

    What happens if we change the angle?

    90

    750 N

    A B

    C

    Horizontally

    ACsin45 = BCsin45

    AC = BC

    Vertically

    ACcos45 + BCcos45=750 N

    AC + BC =750 N/cos45

    2 AC = 750 N/cos45

    AC = 530 N = BC

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    Trusses (1)

    One of the basic methods to determine

    loads in individual truss members is called

    the Method of Joints. Each joint is treated as

    a separate object and a free-body diagram

    is constructed for the joint.

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    Trusses (2)

    30 45

    A

    B C

    500 N

    Horizontal forces

    ABcos30 = ACcos45

    AC = ABcos30/cos45

    Vertical forces

    ABsin30 + ACsin45 = 500 N

    ABsin30 + AB(cos30/cos45)sin45 = 500 N

    AB = 366 N

    AC = 448 N

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    Trusses (3)

    30 45

    A

    B C

    366 N

    Horizontal forces

    BC = ABcos30 = ACcos45

    = 316 N

    Vertical forces at B

    RB= ABsin30

    = 183 N

    Vertical forces at C

    RC= ACsin45

    = 317 N

    Check

    RB+ RC= 183 N + 317 N = 500 N

    448 N

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    Moment of a force

    The product of the force and the perpendiculardistance from the line of action of the force tothe axis.

    Moment about a = F d (units N m)

    d F

    a

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    Principle of Moments (1)

    If a body is at rest under the action of several forces, the total

    clockwise moment of the forces about any axis is equal to

    the anticlockwise moment of the forces about the same axis.

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    Principle of Moments (2)

    2 m 1.5 m

    x N60 N

    ab

    y N

    Moments about a: 60 2= x 1.5

    x = 120/1.5 = 80 N

    Moments about b: (2 + 1.5) 80 = 2 y

    y = 280/2 = 140 N (ignoring mass of beam)

    Or more simply: y = 60 + 80 = 140 N

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    Principle of Moments (3)

    2 m 1.5 m

    x N60 N

    ab

    y N

    Now let the beam weigh 5 kg

    Additional force of 49 N acting centrally.

    Moments about a: (60 2) + (49 0.25)= x 1.5

    x = 144.5/1.5 = 88.2 N

    Reaction of support y = 60 + 49 + 88.2 = 197.2 N

    49 N1.75 m

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    Principle of Moments (5)

    1.5 m 1.5 mab

    y N

    Now support the unloaded beam at a, b and c:

    Moments about b: 49 1.25 = y 1.5 + z 3

    Moments about a: 49 0.25 = x 1.5 - z 1.5

    Moments about c: 49 1.75 = x 3 + y 1.5

    49 N1.75 m

    x N

    0.5 m c

    z N

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    Principle of Moments (6)

    1.75 m

    Now support the unloaded beam at c only

    49 N1.75 m

    c

    z N

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    Centre of Gravity (2)If a vertical line through the centre of gravity falls outside the

    base upon which the body relies for stability, overturning will

    result, unless precautions, such as tying the base down, are

    taken.

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    Centre of Gravity (3)

    For a rectangle or square, the centre ofgravity occurs at the centre of the section.

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    Centre of Gravity (4)

    For a triangular section the centre ofgravity occurs at a point 1/3 of the height

    from the base.

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    Centre of Gravity (5)

    For a circular section the centre of gravityoccurs at the centre of the circle.

    r

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    Centre of Gravity (6)To determine the centre of gravity for a compound section:

    1. Divide the section into several parts (i.e. rectangles and

    triangles, circles) so that the centre of gravity of each

    individual part is known.

    2. Determine the area and position of centre of gravity of each

    part.

    3. Take moments about a convenient axis to determine the

    centre of gravity of the whole body.

    This is based on the principle that, along any one axis (or in any

    one direction):

    when the distance is measured from the same point in each case.

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    Centre of Gravity (7)

    Determine the position of the centre ofgravity of the L-section shown below:

    0.5 m 0.5 m

    1 m

    0.75 m

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    Centre of Gravity (8)

    Divide up section into two rectangles,identify c.o.g of each relative to O and

    calculate area.

    0.5 m

    0.25 m

    Area 1 = 0.5 m2

    0.25 m

    0.625 m Area 2 = 0.125 m2

    O

    Total area = 0.625 m2

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    Centre of Gravity (9)

    Let X = location in X axis of c.o.g0.5 m

    0.25 m

    0.5 m2

    0.125 m2

    O

    Total area = 0.625 m2

    0.625 X = 0.50.5 + 0.1250.25X = 0.45 m

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    Centre of Gravity (10)

    0.5 m2

    0.25 m

    0.625 m

    0.125 m2

    O

    Total area = 0.625 m2

    Let Y = location in Y axis of c.o.g

    0.625 Y = 0.125 0.625 + 0.5 0.25

    Y = 0.325 m

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    Centre of Gravity (11)

    Now let us drill a hole in the object, whereis the new centre of gravity?

    0.4 m

    0.25 m

    0.25 m

    Area 3 = 0.12564 m2

    Total area = 0.49936 m2

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    Centre of Gravity (12)

    Find new X and Y:

    0.25 m 0.12564 m2

    Total area = 0.49936 m2

    0.49936 X = 0.50.5 + 0.1250.250.125640.25X = 0.5 m

    0.49936 Y = 0.50.25 + 0.1250.6250.125640.25

    Y = 0.344 m

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    Centre of Gravity (14)

    Divide the section up into rectangles andtriangles:

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    Centre of Gravity (15)

    Select the first solution (but either methodwould give the same answer).

    Area 1 3x1.5/2 = 2.25m2

    Area 2 4x1.5 = 6.00m2

    Area 3 3x1.0 = 3.00m2

    Total = 11.25m2

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    Centre of Gravity (16)

    Select two axes A-A and B-B, at the extreme edge

    of the figure. The distance to the centre of gravityof each section can then be calculated from these

    axes.

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    Centre of Gravity (17)

    Let X be the horizontal distance to the

    centre of gravity of the whole figuremeasured from A-A and Y be the vertical

    distance to the centre of gravity of the

    whole figure measured from B-B.

    Taking moments about A-A:

    11.25X = (2.25x2.25)+6.0x2.25)+(3.0x1.5)

    = 5.6+13.5+4.5

    = 23.6

    X = 23.6/11.25 = 2.1 m

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    Centre of Gravity (18)

    Taking moments about B-B:

    11.25Y = (2.25x6.0) + (6.0x3.0) + (3.0x0.5)= 13.5 + 18.0 + 1.5

    = 33.0

    Y = 33.0/11.25 = 2.9m

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    Centre of Gravity (19)

    Now let us support the section at the middle

    and far rightWhat is the ratio of forces on each support?

    3 mX

    Y

    1.5 m

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    Centre of Gravity (20)

    Moments about Y.

    1.5 RX = 0.9

    RX= 0.6

    therefore RY= 0.4

    3 mX

    Y

    1.5 m