Chapter 3 Kinematics of particles

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Jump to first page 1 Chapter 3 Kinematics of particles Differentiation: the ratio between two increments when they are extremely small, e.g. velocity. Increment: distance traveled at the end of the 1 st second = 10 m distance traveled at the end of the 3 rd second = 14 m increment of distance = 4 m increment of time = 2 s Ratio between two increments = 4 m/2s = 2 m/s (average velocity) More detailed measurement: distance traveled at the end of 1.01 second, the distance traveled is 10.025 m, the ratio becomes 0.025 m / 0.01 s = 2.5 m/s (instantaneous velocity).

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Chapter 3 Kinematics of particles. Increment: distance traveled at the end of the 1 st second = 10 m distance traveled at the end of the 3 rd second = 14 m increment of distance = 4 m increment of time = 2 s - PowerPoint PPT Presentation

Transcript of Chapter 3 Kinematics of particles

Page 1: Chapter 3   Kinematics of particles

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1

Chapter 3 Kinematics of particles

Differentiation: the ratio between two increments when they are extremely small, e.g. velocity.

Increment: distance traveled at the end of the 1st second = 10 m distance traveled at the end of the 3rd second = 14 m increment of distance = 4 m increment of time = 2 sRatio between two increments = 4 m/2s = 2 m/s (average velocity)More detailed measurement: distance traveled at the end of 1.01 second, the distance traveled is 10.025 m, the ratio becomes 0.025 m / 0.01 s = 2.5 m/s (instantaneous velocity).

Page 2: Chapter 3   Kinematics of particles

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3

11

1

,

))((

constant. a is where,0

nnn

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yx

z

O

)(tr

)( ttr r

)()( where, velocity Average av trttrrt

rv

rdt

rd

t

rv

t

0

limInstantaneous velocity

rvdt

vda

Acceleration

Position )(tr

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Cartesian coordinate system

zzyyxxr va

zzyyxxrv

zzyyxxr

ˆˆˆ

ˆˆˆ

ˆˆˆ

x

z

y

r

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2D Polar coordination system

rrr ˆ

θ̂r̂

r

y

xO

: unit vector // to (radial) : unit vector to (in -direction)

r̂θ̂ r̂

r

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Velocity

)(ˆ ttr

)(ˆ trd)tt(θ̂

θ̂d

)(ˆd tr

)(ˆ tθ

d

,ˆˆ

ˆ

rrrrrv

rrr

θ̂ dr̂d

θ̂ θ̂td

d

td

)t(r̂d)t(r̂

Since

θrrrv ˆˆ θvrv θrrˆˆ

radialvelocity

tangential velocity

angular velocity

O)(tr

)(ˆ tr

)(ˆ ttθ

)( ttr

d

)Δ(ˆ ttr

)t(θ̂

θx

y

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θθrθrrθrra 2 ˆ)2(ˆ)(

centripetal acceleration.

θθ rθθ rθθ rrrrrva ˆˆˆˆˆ Acceleration

rθ trt

t

t

tθ rθ ˆˆor))(ˆ(

d

)(d

d

)(ˆdor)ˆ(dˆd

Since

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3s.atofand Find04.02.0 and 02.02.0

Example23

t B a vtrtt

θ

(m/s)ˆ0.414ˆ0.24rad/s 0.74 ,s/m 24.0 m, 0.56 3s,at

(2) 20.06 0.2

(1) 0.08

ˆˆSolution

θrv θrr t

t θ

trθθrrrv

)(m/s ˆ 0.557ˆ 0.227-

s/rad 36.0 s, 3at

0.12 ,2 /sm 0.08

ˆ2ˆ

2

2

θ r a

θ t

t θ r

θ)θrθ(rr)2θrr( a

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s/rad 10-3.63)/2sin(s/m 71.730cos2.9014.080000 cos

ˆsin ˆcos

ˆ ˆ

ˆ)2(ˆ)(

4-g

2o2g

2

gg

θr

2

rθr-θaθ θa-θrr

θθa r θa- θa ra

θθrθrrθrra

)s/m(ˆ014.01080ˆ102.1 ˆˆ 33 θrθθrrrv

.rad/s 014.0 and ,m/s10x2.1 ,km 80 ,30at and calculate

,s/m 2.9under g travellinisrocket a If Example

3

o

2g

θr rθθ r ,va

Solution v

ga

r

r

θ̂

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system. coordinatepolar applyingby 90 at and Find .0 and s rad5 90 At

ck.linear tra a andrack circular t a along moving is P :Exampleo1

,o θavθ

0.08m

0.04m

P

AO

r

θ̂

θθr θ rrv ˆˆˆ Solution For OAP, 0.082 = 0.042 +r2+2 x 0.04 r cosTime derivative:At = 90o, r = 0.06928 m

θθ)r(θrrr0 sin0.042cos0.0422

θrvθr

θrrr

ˆ346.0ˆ2.0)s/m(2.004.0

08.020

θ)θrθ(rr )θrr(a 2 ˆ2ˆ

θθrθθr θθrθθrθrrrr

sin08.0cos08.0sin08.0sin08.0cos08.0220

2

2

θra r ,θrrrr

ˆ2ˆ15.1)s/m(5774.0such that08.00 ,90At 2o

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zzθθrθrrθrr rvazzθθrrrrv

zzrrr

ˆˆ)2(ˆ)(ˆˆˆ

ˆˆ

2

3D Cylindrical coordination system

x

z

y

R

z

rr̂

θ̂

θ̂

z

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Normal and Tangential Coordinates (n-t) :

tvtt

t

tv ˆˆs

ˆ)s(lim

rlim

0s0t

tvtvtvt

a ˆˆ)̂(d

d

)(sr

)( ssr

s

radius of curvature

O’

β

O’

s)s(t̂

)ss(ˆ t

)s(t̂

)ss(ˆ tt̂

β

nvs

nv

s

tv

t

s

s

tt ˆ

1

d

ˆd

d

ˆd

d

d

d

ˆdˆ

ntva /v ˆˆ ρ)( 2

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Position of A relative to B :

Velocity of A relative to B :

Acceleration of A relative to B : BABA

BABABAA/B

BAA/B

aaa

vvv rrr

rrr

/

/or

A

B

o

Ar

Br

BAr /

x

y