lecture 2 mech 211 spring 2014

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    Lecture 2

    Chapter 1: Example ProblemsChapter 2: Concurrent Force Systems

    Sections 2.1-2.2,2.4,2.5

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    TA Help SessionsTeaching Assistants:

    Eleazar MarquezDavid Trevino-Garcia

    Lecture 2-Kirkpatrick 2

    Wednesdays from 5:00PM-6:00PM

    Location:

    Mechanical Laboratory Building (MEL) 251

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    Important! Trigonometry

    Law of Sines:

    sin sin sin

    a b c

    = =

    b

    a

    Lecture 2-Kirkpatrick 3

    Law of Cosines:

    c

    2 2 2 2 cosc a b ab = +

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    Newtons Law of Gravitation(From Lecture 1)

    m2

    1 22

    m mF G r

    =

    Fr

    Lecture 2-Kirkpatrick

    m1

    FG = Universal Gravitational Constant

    Newtons Law of Gravity is a mathematical result from atheoretical model of how bodies interact.

    4

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    Some Important

    Numerical Values8 3 2 11 3 23.439(10 ) /( ) 6.673(10 ) /( )G ft slug s m kg s

    = = (Page 9 oftextbook)

    Lecture 2-Kirkpatrick 5

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    Calculation Of

    Acceleration of Gravity

    23 24

    7 6

    4.095(10 ) 5.976(10 )

    2.090(10 ) 6.371(10 )

    e

    e

    m slug kg

    r ft m

    = =

    = =

    8 3 2 11 3 23.439(10 ) /( ) 6.673(10 ) /( )G ft slug s m kg s = =

    Given

    Lecture 2-Kirkpatrick 6

    e ear were rea y a sp ere( )

    238 3 2

    2 7 2 2

    2 2

    2

    4.095(10 )3.439(10 ) /

    (2.090(10 ))

    (3.439)(4.095)(10)/ 32.24 /

    (2.090)

    e

    e

    m slugg G ft slug s

    r ft

    g ft s f s

    = =

    = =

    Note: 2 232.17 / 9.807 / g ft s m s= =

    Are the usual or official values used.

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    Example Problem: Problem 1.5/p14Given: The planet Venus has a diameter of 7700 miles and a mass of

    3.34(1023)slug.Find: Determine the gravitational acceleration gat the surface of Venus.

    Other Information:2

    venus

    venus

    venus

    mg G

    r=

    Lecture 2-Kirkpatrick 7

    8 3 23.439(10 ) /( )G ft slug s

    = where

    Therefore

    2

    238 3 2

    2

    2

    3.34(10 )(3.439(10 ) / ( ))

    ((7700 )(.5)(5280 / ))

    27.7965 / sec

    venusvenus

    venus

    venus

    venue

    mg G

    r

    slugg ft slug s

    miles ft mile

    g ft

    =

    =

    =

    (See page 9 of text)

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    Example Problem: Problem 1.21/p14Given: The first U.S. satellite, Explorer 1, had a mass of approximately 1

    slug. Its perigee (low altitude) was 175 miles and its apogee (highaltitude) was 2200 miles.

    Find: Determine the force exerted on the satellite by the earth at the lowand high points of the orbit.

    Forces to calculate: expearth lorer m m

    F G=

    Lecture 2-Kirkpatrick 8

    ( )

    ( )

    8 3 2 23

    exp

    7

    3.439(10 ) / ( ); 4.095 10 ; 1

    2.090 10 ; 175 5280 ; 2200 5280

    e lorer

    e perigee apogee

    G ft slug s m slug m slug

    ft ftr ft h mi h mimi mi

    = = =

    = = =

    earth

    altitude

    r h+

    where

    Results

    29.57 and 13.32perigee apogeeF lb F lb= =

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    Let MATLAB Do The Numbers

    Lecture 2-Kirkpatrick 9

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    Example Problem: Problem 1.24/p14At what distance, in kilometers, from the surface of the earth on a line fromcenter to center would the gravitational force of the earth on a body beexactly balanced by the gravitational force of the moon on the body.

    a b

    Lecture 2-Kirkpatrick 10

    Earth MoonBody

    Given

    ( )

    / /2 2

    / /

    8

    ;

    ;

    3.844 10

    e b moon bbody earth body moon

    body earth body moon

    m m m mF G F G

    a b

    F F a b R

    R m

    = =

    = + =

    =

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    Example Problem: Problem 1.24/p14

    Earth Moon

    a b

    Body

    Givene b moon b

    m m m m

    Lecture 2-Kirkpatrick 11

    ( )

    / /2 2

    / /

    8

    ;

    3.844 10

    body earth body moon

    body earth body moon

    a bF F a b R

    R m

    = + =

    =

    Find and . Then calculate and .ba eartha r moonb r

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    Example Problem: Problem 1.24/p14Therefore

    2 20e b moon b e

    moon

    m m m m mG G b a

    a b m= =

    And, we must solve simultaneously

    e em m

    Lecture 2-Kirkpatrick 12

    1 1

    1 01

    1 11 1 1

    moon moon

    e e

    moon moon

    e e

    moon moon

    m m b Ra b R

    m ma R

    m mb Rm m

    m m

    =

    = + =

    = = + +

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    Example Problem: Problem 1.24/p14Given

    ( )

    ( )

    ( )

    8

    88

    24

    1 1 3.4603 10

    0.38375 103.844 10

    e

    moon

    e

    moon

    ma R

    mb m

    m ma

    b mR m

    = +

    =

    =

    Lecture 2-Kirkpatrick 13

    ( )22

    .

    7.350 10

    e

    moon

    m

    m

    =

    =

    Also ( )

    ( )

    8

    8

    3.3965 10

    0.36637 10

    e

    moon

    ma r

    b r m

    =

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    Example Problem: Problem 1.53/p24Given: The equation, where r and Rare lengths and n

    is dimensionless. Also, k is the modulus of a coil spring (force per unit of

    length.

    4

    34

    Grk

    R n=

    Find: The dimensions of G

    Lecture 2-Kirkpatrick 14

    [ ] [ ] [ ]

    33 2

    4 4 24

    4F

    Lk R n FL FLGL L Lr

    = = = =

    Note: [G] reads dimensions of G

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    Chapter 2

    Concurrent Force Systems

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    Three Characteristics of Forces Forces are Vectors

    Magnitude

    Direction With respect to a fixed frame of reference

    Point of Application

    Lecture 2-Kirkpatrick 16

    Can think of force as a function of position whose value is avector.

    Body

    F

    Point of Applicationz

    x

    y0

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    More On Direction of a Vector With respect to a fixed frame of reference

    Line of Action

    Sense

    Lecture 2-Kirkpatrick 17

    x

    y

    z

    0

    Line of Action

    Sense:Denoted byarrowhead

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    Representation of VectorsF

    In Two DimensionsMagnitudeOne Angle

    x

    y

    Lecture 2-Kirkpatrick 18

    In Three DimensionsMagnitudeTwo Angles

    Will explain later!

    x

    y

    z

    0

    yx

    z F

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    Interesting Fact Consider a force F on a Rigid Body

    Lecture 2-Kirkpatrick 19

    Since the body is rigid,

    Point of action of F is anywhere on line ofaction

    Sometimes called a sliding vector.

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    Contact Forces Concentrated Forces

    Area of contact is small compared to size ofbody

    Can be treated as applied at a point

    Lecture 2-Kirkpatrick 21

    Distributed Forces Applied over an area of contact

    Realistically

    All contact forces are distributed Thus, contact forces are approximations of reality

    Good approximations!

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    Examples Concentrated forces

    Automobile sitting onbridge

    Lecture 2-Kirkpatrick 22

    Distributed forces

    Concrete bridge floorsitting on beam

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    Frankly! You will learn about types of loads by the

    many examples we will see. Most of the loads will be idealized so that

    Lecture 2-Kirkpatrick 23

    .

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    Other Stuff About Forces Concurrent Forces

    All forces act through a

    common point

    Lecture 2-Kirkpatrick 24

    Coplaner Forces All forces lie in a single

    plane

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    More Stuff About Forces Parallel Forces

    All forces are parallel

    Lecture 2-Kirkpatrick 25

    Collinear Forces All forces have the

    same line of action

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    Some Vector Algebra(Appendix A)

    Addition

    Parallelogram Law

    +A B

    B

    Lecture 2-Kirkpatrick 26

    A

    + = +A B B A Commutative Property

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    Vector Algebra

    (Cont.)

    Scalar Multiplication

    Changes length or magnitude

    A

    A

    Lecture 2-Kirkpatrick 27

    A

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    Vector Algebra

    (Cont.)

    Notation

    If A is a vector, its magnitude or length is written Sometimes we write

    Note ifA=1, then A is a unit vector

    AA = A

    Lecture 2-Kirkpatrick 28

    Dot Product cos = =A B B A A B

    A

    B

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    Vector Algebra

    (Cont.)

    Cross Product

    sin =A B A B n

    B

    Lecture 2-Kirkpatrick 29

    A

    vector perpendicular toplane ofA andB in

    direction of right handrule

    Note: =A A 0

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    Cross Products Relationship to Area

    B

    n

    Lecture 2-Kirkpatrick 30

    sin =A B A BA

    =Area of parallelogram

    Note A B = B A

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    Vector Algebra

    (Cont.)

    Component Representation of a Vector

    z

    x y zA A A= + +A i j kA = A i

    Lecture 2-Kirkpatrick 31

    x

    y0

    ij

    ky

    z

    A

    A

    =

    =

    A j

    A k

    w ereA

    ( ) ( ) ( )= + + A A i i A j j A k kAn Identity

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    Vector Algebra

    (Cont.)z

    k

    1, 1, 1

    0, 0, 0,

    = = =

    = = =

    i i j j k k

    i j i k j k

    Because unit vectors are mutually orthogonal

    Lecture 2-Kirkpatrick 32

    x

    y0

    ij , ,

    etc = = = i j k j k i k j i

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    Vector Algebra

    (Cont.)

    , ,

    etc

    = = = i j k j k i k j i

    Lecture 2-Kirkpatrick 33

    i

    k

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    Vector Algebra

    (Cont.)

    ( ) ( )x y z x y z

    x x y y z z

    A A A B B B

    A B A B A B

    = + + + +

    = + +

    A B i j k i j k

    2 2 2= = =

    Lecture 2-Kirkpatrick 34

    ( ) ( ) ( )

    x y z

    x y z

    y z z y z x x z x y y x

    A A A

    B B B

    A B A B A B A B A B A B

    =

    = + +

    i j k

    A B

    i j k

    y z