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I. Work and Energy Operate on Law of Motion i p i p i p F v mA v i i p i p dv m v dt 1 2 i i p i p i p d F v mv v dt kinetic energy T Integrate 2 2 1 1 t t i p t t dT F v dt dt dt D1 Integrals of the Motion Another form of Law of Motion yields one scalar differential equation Work

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  • I. Work and Energy

    Operate on Law of Motion

    i p i p i pF v m A v

    i i pi pd vm v

    dt

    12i

    i p i p i pdF v m v vdt

    kinetic energy T

    ii p d TF v T

    dt

    Integrate

    2 2

    1 1

    t t

    i p

    t t

    d TF v dt dt

    dt

    2 1W T T True for ANY system

    D1

    Integrals of the Motion

    Another form of Law of

    Motion yields one scalar

    differential equation

    Work

  • Concept takes on additional significance in a special subset of problems, i.e.,

    conservative systems If system is conservative, then each force is derivable from a

    potential function U

    2 2

    1 1

    t r

    i p i

    t r

    W F v dt F dr

    1 1 2 2 3 3 1 1 2 2 3 3 i F e F e F e dr e dr e dr eF dr

    1 1 2 2 3 3F dr F dr F dr

    If force is derivable form a potential function U, then

    1 2 31 2 3

    U U UF F F

    r r r

    So, 1 2 31 2 3

    i U U UF dr dr dr dr dUr r r

    2 2

    1 1

    r U

    i

    r U

    W F dr dU

    2 1W U U True for any conservative system

    So, if any system is conservative

    2 1 2 1W T T U U

    C2 D2

    assume working frame is inertial

    for this discussion, e.g., e

  • Define V (potential energy) = - U

    2 1 2 1 2 1W T T U U V V

    2 2 1 1T V T V E Total Mechanical Energy

    T V E Principle of Conservation of

    Mechanical Energy

    Examples of Conservative Forces

    uniform gravity F m g

    V m g h

    inverse-square gravity 2

    G M mF

    r

    G M mV

    r

    linear spring F k x 2

    2

    k xV

    D3 D3

  • II. Impulse and Momentum

    A. Linear Impulse and Linear Momentum

    2 2

    1 1

    t t

    i p

    iit t

    m A dtF dt

    linear impulse

    2

    1

    t i i p

    i

    t

    d vm dt

    dt

    2

    1

    ti

    i p

    it

    m d v

    2

    1

    2 1( ) ( )

    t

    i p i p

    it

    m v t m v tF dt

    Let i pp m v

    2

    1

    2 1

    t

    it

    p pF dt

    Note: If no forces act in a given direction, linear momentum in that

    direction is conserved (constant)

    potentially 3 constants

    D4

    principle of linear impulse and

    linear momentum

  • II. Impulse and Momentum

    B. Angular Impulse and Linear Momentum

    i pr F r m A

    i i OO d HM

    dt form previously introduced

    2 2

    1 1

    t t i i O

    O

    iit t

    d HdtM dt

    dt

    2

    1

    2 1( ) ( )

    t

    i O i OO

    it

    H t H tM dt

    angular impulse

    Note: If angular impulse is zero in a given direction, angular

    momentum in that direction is conserved (constant)

    potentially 3 constants

    D5

    principle of angular impulse

    and angular momentum

  • Example: Earth-Orbiting Spacecraft

    Consider Motion of spacecraft (satellite) moving in orbit about the Earth

    Now - to set up problem, derive EOM, and solve? must add to diagram and choose variables of interest

    but which ones? how many?

    For most general motion, might set up as 3D and define spherical

    coordinates

    But, motion might actually be 2D in which case can use radial/transverse

    coordinates for 2D (cylindrical with z = 0)

    How to make a justifiable choice?

    D6

    Assume that Earth is a particle and generates an inverse square gravitational

    force

    2

    sg

    Gm mF

    r

    distance between masses

  • Initially consider the possibility of constants or integrals of the motion

    ==> may offer/suggest insight

    Requires FBD same whether problem 2D or 3D

    1. Energy (list ALL forces)

    only gravity

    2

    sg r

    Gm mF u

    r

    if conservative, should be able to define appropriate potential

    function U

    sGm m

    Ur

    2

    sg r r

    Gm mUF u u

    r r

    U exists total energy conserved

    2. Linear Momentum

    Forces in FBD zero in any or all inertial directions? NO

    Linear Momentum NOT conserved

    D6

    Define

    :e inertial :u moving with s

    such that rur

    2

    sg r

    Gm mF u

    r

    D7

  • 3. Angular Momentum

    Moments (resulting from FBD forces) zero in any or all inertial

    directions?

    0M r F

    0e ed H

    Mdt

    constant eH tells us that the motion is 2D why?

    Model problem as 2D

    D8

    eH is constant in magnitude and direction

    Define

    :e inertial :u moving with s such that

    rur

    e u zu

    z ru u u

  • Kinematics

    srr ru

    e srv ru r u

    2 2e s rA u ur r r r

    e sF m A

    2 2 : sr sGm m

    u m r rr

    : 02su m r r

    2nd-order, coupled, nonlinear differential equations

    The complete solution ( ), ( )r t t is not trivial to produce But we can still get a lot of information without the complete solution

    Recall known constants of motion ,iH E

    Can write expressions for each; if they are true constants / integrals of

    the motion, then EOMs should appear when we differentiate expressions

    for constants

    D9 D9

  • :HC Angular Momentum

    e s e ss r s rH r m v ru m ru r u

    2 e

    s zH m r u

    2 02e e

    s z

    d Hm urr r

    dt

    02e e

    s z

    d Hm r ur r

    dt

    zero (EOM)

    :EC Energy

    E T V where 2 e s zH m r u 1

    2e s e s

    sT m v v

    22 2 22

    sm G m mr r

    r

    2 2 2 ssGm mdE

    m rr r r r rdt r

    sub: 2r r

    2 22

    2s sdE Gm

    m r m rr r rdt r

    22

    0sdE Gm

    m r r rdt r

    EOM

    D10

    V = - U

  • Complete solution to 2nd-order, coupled, nonlinear DE

    not available can we get some state information from constant? yes, specific states at given instants

    Given: @ t1, satellite at 400 km altitude

    velocity directed as shown above with magnitude 5km/se sv

    Find: velocity vector @ t2 when altitude is 500 km

    Define scalar quantities at times t1, t2

    t1 t2

    1 1( )s rr t r u

    2 2 ( )s

    rr t r u

    1 1 1 1 ( )e s rv t r u r u

    2 2 2 2

    ( )e s rv t r u r u

    D11

  • means that there are two places along

    path with altitude 500 km

    :HC Total Angular Momentum Conserved (magnitude and direction)

    2 e

    s zH m r u

    2 constante sm rH

    2 constante

    s

    Hh r

    m

    2 2

    1 1 2 2h r r 2 2 4.27 km/sr

    :EC Total Energy Conserved (scalar)

    2 2 2 constant2

    s sm Gm mE r rr

    s

    E=

    m constantss 2 2 2

    Gm mm= =r +r

    2 rE

    1 1 1 2 2 21 2

    1 12 2

    2 2 2 2 2 2Gm Gm= =r +r r +r r r

    E

    Note: 53.986 10 Gm km

    3/s

    2

    2 2.25 r km/s

    2 ( ) 2.25 4.27

    e s

    rv t u u km/s

    D12