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2.29 and 3.7, 3.14, 3.18, 3.20.pdf

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    22

    Problem 2.29

    The KEY

    To apply Newtons Law in polar form all the

    forces must be taken from an inertial frame

    You MUST see the motion of the car from thegroun an N!T from the re"ol"ing platform

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    33

    Problem 2.29 contd.

    So conitione#

    $% Motion will N!T be raial but a cur"e oneon the re"ol"ing platform

    &% 's friction acts opposite the motion# it acts in the irection of resultant of (ran (

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    55

    Contd.

    (orce is pro"ie by friction ha"ing ma,- "alue mg

    mgF,slidingAtmgF =

    22222

    0

    2422 gmvm4rm =+

    +ence#

    mv2rv4gm

    FrFF

    0

    22

    0

    22

    r

    +=

    +=

    0

    slidslid4

    22

    0

    22

    slid

    v

    rt;

    v4gr =

    =

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    77

    Solution

    m1 m2

    O

    2/

    x

    2m&is release at t = 0

    1an you physically imagine the motion3

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    88

    Proposition

    m1 m2

    O

    2/

    xm2is released at t = 0

    $- m&will e,ecute S+M aboutx=l 2mk=

    &- m$will N!T mo"e until m&crosses l mark

    't what t# this will happen33

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    99

    Fixing Time Scale

    m1 m2

    O

    2/

    x

    4e nee to look at the motion in two time omains*

    4Tt)2

    4Ttto0t)1

    == Case I

    Case II

    k

    m

    24

    124

    Tt 2

    ===

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    1010

    Fixing CMs

    Case I m1 m2

    O

    2/

    x

    ( )tcos22lxlxatm;0xatm 22211 ===(measured from the wall)

    ( )( )

    ( )

    ( )21

    2

    21

    21

    mm2

    tcos2lm

    mm

    tcos22

    lm0m

    t

    +

    =

    +

    +=

    4Tt0

    Note it is function of time

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    1212

    CM ater T!"

    The position of the 1M for instants t>T/4is gi"en by*

    ( )

    ( )

    ( )

    +

    +=

    +

    +

    +

    =

    +

    =

    2t2

    mm2

    lm

    4

    Tt

    mm2

    lm

    mm

    lm

    4

    Tt"4

    Tt

    21

    2

    21

    2

    21

    2

    C!

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    1313

    Complete Motion

    The complete motion of 1M is*

    ( )

    ( )

    ( ) 4T

    t0#ormm2

    tcos2lm

    t 21

    2

    +

    =

    ( ) ( )( ) 4Tt#or

    mm22t2lmt

    21

    2 >+

    +=

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    1414

    Problem 3.#"

    .t eals with conser"ation of linear momentum*

    $

    m

    !

    1,2,%, 4&&.'

    ( )$v'm!v(;0( #i +==

    7el of men wrt groun

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    1515

    Problem 3.#" contd.

    a% Let flat car attain a "elocity " when all men :umpeout simultaneously

    1onser"ing momentum#( )$v'm!v(;0( #i +==

    'm!

    'm$"

    +=

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    1616

    Problem 3.#" contd.

    b% Let "i;$an "ibe the "elocities of the flat car before an

    after the it).man :umps off an conser"e momentum

    ( )[ ] ( )[ ] ( )m$vvmi'!vmi1'! ii1i ++=++

    ( ) ( )mi1'!

    m$v

    mi1'!

    m$vv i1ii ++

    =++

    +=

    ( ) v

    mi1'!

    1m$vv

    iii = ++==

    / (inal "elocity

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    1717

    Problem 3.#" contd.

    c% The case b% yiel larger final "elocity

    ( ) ++= i mi1'!1

    m$v

    +a"e a look at the

    ++

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    1818

    Problem 3.#$

    E=uation of motion* mgdt

    dm$dt

    dvmF r*l ==

    2kmv

    dt

    dvm

    dt

    dmv

    dt

    dvmmg +=+=

    .constk

    gvtkvg

    dt

    dv 2 ===

    KEY* .nformation about $r*l

    's rainrop gains mass from clou at rest# $r*l=+v

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    1919

    Problem 3.2%dt

    dm$

    dt

    dvmF r*l=

    E=uation of motion of the rocket*

    mgmvm$dt

    dv

    m =

    ( ) ( ) .const

    g$v,t*1g$

    1v t =

    ==


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