Opposition to Board of Governors SJ Motion and Statement of Facts
Force and Motion I: The Laws of Motion SJ 8th Ed.: Ch. 5.1 –5janow/Physics 111 Spring 2012... ·...
Transcript of Force and Motion I: The Laws of Motion SJ 8th Ed.: Ch. 5.1 –5janow/Physics 111 Spring 2012... ·...
Co
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Physics 111 Lecture 04
Force and Motion I: The Laws of Motion
SJ 8th Ed.: Ch. 5.1 –5.7
•Dynamics -Some history
•Force Causes Acceleration
•Newton’s First Law: zero net force
•Mass
•Newton’s Second Law
•Free Body Diagrams
•Gravitation
•Newton’s Third Law
•Application to Sample Problems
5.1
Th
e C
on
cep
t o
f a F
orc
e
5.2
New
ton
’s F
irst
Law
an
d
Inert
ial F
ram
es
5.3
Mass
5.4
New
ton
’s S
eco
nd
Law
5.5
Gra
vit
ati
on
al
Fo
rce a
nd
Weig
ht
5.6
New
ton
’s T
hir
d L
aw
5.7
Usin
g N
ew
ton
’s S
eco
nd
Law
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Dynamics -Newton’s Laws of Motion
Kinematics described motion only –no real Physics.
Why does a particle have a certain acceleration?
New concepts (in 17th century):
•Forces -pushes or pulls -
cause acceleration
•Inertia (mass) measures how much matter is being accelerated –
resistance to acceleration
Sir Isaac Newton 1642 –
1727
•Formulated basic laws of mechanics
•Invented calculus in parallel with Liebnitz
•Discovered Law of Universal Gravitation
•Many discoveries dealing with light and optics
•Ran the Royal Mint for many years during old age
•Many rivalries & conflicts, few friends,
no spouse or children, prototype “geek”
Newton’s 3 Laws of M
otion:
•Codified kinematics work by Galileo and other early experimenters
•Introduced mathematics (calculus) as the language of Physics
•Allowed detailed, quantitative prediction and control (engineering).
•Ushered in the “Enlightenm
ent”& “Clockwork Universe”.
•Are accurate enough (with gravity) to predict all com
mon
motions plus those of celestial bodies.
•Fail only for v ~ c and quantum
scale (very small).
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Force: causes any change in the velocities of
particles
A force is that which
causes an acceleration
Newton’s
definition:
Co
nta
ct
forc
es i
nvo
lve “
ph
ysic
al
co
nta
ct”
betw
een
ob
jects
F =
-kx
Fie
ld f
orc
es a
ct
thro
ug
h e
mp
ty s
pac
e w
ith
ou
t p
hysic
al
co
nta
ct
Action at a distance through intervening space? How?
Given atomic physics, Is there any such thing as a real contact force?
The four fundamental forces of nature are:
Gravitation, Electromagnetic, N
uclear, and W
eak force
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Force: what causes any change in the velocities
of particles
Units: 1 N
ewton = force that causes 1 kg to accelerate at 1 m/s
2
1 Pound = force that causes 1 slug to accelerate at 1 ft/s2
Forces are VECTORS
Operate with vector rules
Rep
lace a
fo
rce a
cti
ng
at
a p
oin
t b
y i
ts
co
mp
on
en
ts a
t th
e s
am
e p
oin
t.
iF
x
jF
y
Fr
= ===
Su
perp
osit
ion
: A
set
of
forc
es a
t a p
oin
t h
ave t
he s
am
e e
ffect
that
their
ve
cto
r re
su
ltan
t fo
rce w
ou
ld
= ===
F 1r
3Fr
2Fr
∑ ∑∑∑≡ ≡≡≡
ii
ne
tF
Fr
vN
ota
tio
n:
ne
tFr
Definition: A body is in EQUILIBRIU
M
if the net force applied to it equals zero
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Relative motion -Inertial Reference Frames in 1 Dimension
A f
ram
e o
f re
fere
nce a
mo
un
ts t
o s
ele
cti
ng
a c
oo
rdin
ate
sys
tem
.•
Descri
be p
oin
t P
in
bo
th f
ram
es u
sin
g x
1,
v1, a
1an
d x
2,
v2,
a2.
•O
rig
ins c
oin
cid
e a
t t
= 0
•C
on
sta
nt
v12
= r
ela
tive v
elo
cit
yo
f o
rig
in o
f 1
in
fra
me
2
•x
12
is t
he d
ista
nce b
etw
een
ori
gin
s a
t so
me t
ime t
.
Tra
nsfo
rm t
he c
oo
rdin
ate
s:
)t(x
)t(x
)t(x
12
12
+ +++= ===
Tra
nsfo
rm t
he v
elo
cit
ies
:
dt
dx
dt
dx
dt
dx
12
12
+ +++= ===
12
12
v
v
v + +++
= ===
Th
en
a12
= 0
an
d
Fin
d t
he a
cce
lera
tio
ns:
01
21
2
2
a
d
t
dv
a
d
t
dv
dt
dv
dt
dv
dt
dv
a1
21
21
1= ===
≡ ≡≡≡= ===
+ +++= ===
= ===
a
a 2
1= ===
Th
e a
ccele
rati
on
of
a m
ovin
g o
bje
ct
is t
he s
am
e f
or
a p
air
of
inert
ial
fra
mes.
Example: An accelerating car viewed from a train and the ground,with the train
itself moving at constant velocity
Inert
ial
fra
mes c
an
no
t b
e r
ota
tin
g o
r acce
lera
tin
g r
ela
tive
to
on
e a
no
ther
or
to t
he
fixed
sta
rs.
No
n-i
nert
ial
fra
me
s � ���
fic
titi
ou
s f
orc
es.
x2
y2
x1
y1
x12
x2
x1
P
v1
2
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Newton’s First Law (1686)
Don’t moving objects come to a stop if you stop pushing?
•Stopping implies negative acceleration, due to friction
or other forces opposing motion.
•What effect does inertia have on a curve on an icy road?
“T
he L
aw
of
Inert
ia”:
A b
od
y’s
velo
cit
y is c
on
sta
nt
(i.e
., a
= 0
) if
th
e n
et
forc
e a
cti
ng
on
it
eq
uals
zero
Alt
ern
ate
sta
tem
en
t: A
bo
dy r
em
ain
s in
un
ifo
rm m
oti
on
alo
ng
a
str
aig
ht
lin
e a
t co
nsta
nt
sp
eed
(o
r re
main
s a
t re
st)
un
less it
is
acte
d o
n b
y a
net
exte
rnal fo
rce.
Above assum
e an “inertial reference frame”:
•Equations of physics look simplest in inertial systems.
•Non-inertial frames (e.g., rotating) require fictitious forces &
accelerations in physics equations (e.g., centrifugal and Coriolisforces).
Fir
st
Law
(o
ur
text)
: A
n o
bje
ct
that
do
es n
ot
inte
ract
wit
h o
ther
ob
jects
(n
o n
et
forc
e,
iso
late
d)
can
be p
ut
into
a r
efe
ren
ce f
ram
e i
n w
hic
h t
he
ob
ject
has z
ero
accele
rati
on
(i.
e., i
t’s m
oti
on
can
be t
ran
sfo
rmed
to
an
in
ert
ial
fram
e i
f it
is n
ot
in o
ne a
lread
y).
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Mass: the Measure of Inertia
Apply the same force to different objects.
Different accelerations result. W
hy?
Example: Apply same force to baseball, bowling ball, autom
obile,RR train
Mass m
easu
res in
ert
ia:
•th
e a
mo
un
t o
f “m
att
er”
in a
bo
dy (
i.e., h
ow
man
y a
tom
s o
f each
typ
e)
•re
sis
tan
ce t
o c
han
ges i
n v
elo
cit
y (
i.e.,
accele
rati
on
) w
hen
a f
orc
e a
cts
For a givenforce applied to m1and m
2:
12
21
aa
mm
= ===A mass and resulting acceleration on it
are inversely proportional
Th
e s
am
e “
inert
ial m
ass”
valu
e a
lso
measu
res “
gra
vit
ati
on
al m
ass”
–-
a p
art
icle
’s e
ffect
in p
rod
ucin
g g
ravit
ati
on
al p
ull o
n o
ther
masses
Mass is a
scala
r:2
12
1m
mm
m
to m
w
ith
be
ha
ve
s
res
ult
Th
e
Att
ac
h+ +++
= ===
Mass is in
trin
sic
to
an
ob
ject:
•
it d
oesn
’t d
ep
en
d o
n t
he e
nvir
on
men
t o
r sta
te o
f m
oti
on
(fo
r v <
< c
), o
r ti
me.
Do
n’t
co
nfu
se m
ass w
ith
weig
ht
(a f
orc
e):
mg
W= ===
N.
3.3
Wb
ut
N.
20
W
then
kg
m
If
mo
on
ea
rth
≈ ≈≈≈≈ ≈≈≈
= ===2
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Newton’s Second Law
a
m
F
F i
in
et
rr
r= ===
≡ ≡≡≡∑ ∑∑∑
Su
mm
ari
zin
g:
Vector sum
of forces
acting ON a particle
Inertia of
particle
Acceleration resulting
from
Fn
et
SIMPLE PROPO
RTIONALITY W
HEN IN AN INERTIAL FRAME
Cart
esia
n c
om
po
nen
t eq
uati
on
s:
m
a
F
F x
iix
x,n
et
= ===≡ ≡≡≡∑ ∑∑∑
m
a
F
F y
iiy
y,n
et
= ===≡ ≡≡≡∑ ∑∑∑
m
a
F
F z
iiz
z,n
et
= ===≡ ≡≡≡∑ ∑∑∑
Oth
er
ways t
oW
rite
2n
dL
aw
:
dtr
dm
F
F
2
ii
ne
t2r
rr
= ===≡ ≡≡≡∑ ∑∑∑
vm
p
dtp
d
F w
here
net
rr
rr
≡ ≡≡≡= ===
DIRECTION O
F ACCELERATION AND N
ET FORCE ARE THE SAME
Un
its f
or
Fo
rce:
2T/
L M
]a[ ]
m[
]
F[= ===
= ===
SYSTEM FORCE MASS ACCELERATION
SI Newton (N) Kg m
/s2
CGS Dyne gm
cm/s
2
British Pound (lb) slug ft/s
2
1 d
yn
e =
10
-5N
1 g
m
= 1
0-3
kg
1 lb
=
4.4
5 k
g1 s
lug
=
14.
59
kg
1 k
gW
EIG
HS
2.2
lb
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4-1
: T
hre
e s
tud
en
ts c
an
all
pu
ll o
n t
he r
ing
(se
e s
ketc
h)
wit
h i
den
tical
forc
es o
f m
ag
nit
ud
e F
, b
ut
in d
iffe
ren
t d
irec
tio
ns w
ith
resp
ec
t to
th
e +
x
axis
. O
ne
of
them
pu
lls a
lon
g t
he +
x a
xis
wit
h f
orc
e F
1as s
ho
wn
.
Wh
at
sh
ou
ld t
he o
ther
two
an
gle
s b
e t
o m
inim
ize t
he
ma
gn
itu
de o
fth
e
rin
g’s
accele
rati
on
?
a)
θ θθθ2 222
= 0
, θ θθθ
3=
0b
) θ θθθ
2 222=
180,
θ θθθ3
= -
180
c)
θ θθθ2 222
= 6
0,
θ θθθ3
= -
60
d)
θ θθθ2 222
= 1
20,
θ θθθ3
= -
120
e)
θ θθθ2 222
= 1
50,
θ θθθ3
= -
150
Tug of war
x1Fr
2Fr
3Fr
θ θθθ3
θ θθθ2
4-2
: W
ha
t sh
ou
ld t
he
oth
er
two
an
gle
s b
e t
o m
axim
ize t
he m
ag
nit
ud
e o
f th
e r
ing
’s
accele
rati
on
?
a)
θ θθθ2 222
= 0
, θ θθθ
3=
0b
) θ θθθ
2 222=
180,
θ θθθ3
= -
180
c)
θ θθθ2 222
= 6
0,
θ θθθ3
= -
60
d)
θ θθθ2 222
= 1
20,
θ θθθ3
= -
120
e)
θ θθθ2 222
= 1
50,
θ θθθ3
= -
150
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Example:
A hockey puck whose mass is 0.30 kg is
sliding on a frictionless ice surface. Two
forces act horizontally on it as shown in the
sketch. Find the magnitude and direction of the
puck’s acceleration.
Ap
ply
2n
dL
aw
to
x a
nd
y d
irecti
on
s
)c
os
(F
)c
os
(F
m
a
F
F
F
1x
2x
1x
x,n
et
60
20
2+ +++
− −−−= ===
= ===+ +++
≡ ≡≡≡
)s
in(
F )
sin
(F
m
a
F
F
F
1y
2y
1y
y,n
et
60
20
2+ +++
− −−−= ===
= ===+ +++
≡ ≡≡≡
N
8.7
F x,
ne
t= ===
N
5.2
F y,
ne
t= ===
22
9s/
m
0
.3
8.7
m
F
a
x
ne
t,x
= ==== ===
= ===
2s/
m
17
0
.3
5.2
m
F
a
y
net,
y= ===
= ==== ===
Eva
lua
te:
FB
D
m =
0.3
kg
Co
nvert
to
po
lar
co
ord
ina
tes
:
ox
y-1
2/
2 y2 x
)a/
a( ta
n
m/s
3
4
]a
[a
a
3
12
1= ===
= ===θ θθθ
= ===+ +++
= ===
Th
e n
et
forc
e a
nd
accele
rati
on
ve
cto
rs h
ave t
he s
am
e d
irec
tio
nA
un
it v
ecto
r in
th
at
dir
ec
tio
n i
s:
j 0
.50
i
0.8
5
j3
4
17
i
34
29
j|
a|a
i |a|a
|
a|a
a
y
x+ +++
= ===+ +++
= ===+ +++
= ===≡ ≡≡≡
r
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Measuring Force and Mass
On frictionless surface (e.g., air track): Apply enough horizontal
force F
0to give the standard mass m
0the standard acceleration a
0
m0
= 1
kg
a0
= 1
m/s
2
00
am
F
0≡ ≡≡≡
The (standard) force unit thereby defined = 1N.
No
te:
x-c
om
po
nen
ts o
nly
ab
ove,
F&
aare
in
sam
e d
irecti
on
What about forces in the y –
direction, left out above?
Measuring another mass:
•Apply standard force, record resulting acceleration
m/
F
a0
≡ ≡≡≡a
/ F
m
0= ===
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Gravitational Force, Weight, “Normal”Force
Mass in free fallon Earth’s surface accelerates at
g:
FB
D
m
g h
as t
he s
am
ed
irecti
on
(to
ward
cen
ter
of
Eart
h)
an
d m
ag
nit
ud
e f
or
all
masses (
in a
vo
lum
e l
arg
e
co
mp
are
d t
o a
hu
man
).
jm
g
F g
− −−−= ===
rg
= 9
.8 m
/s2
=
32.2
ft/
s2
at
the E
art
h’s
su
rface
•“Action at a distance”
•The weight is independent of how a mass is
moving (perhaps other forces also act).
w
eig
ht"
the
"
F
g≡ ≡≡≡
r
Mass in contact with a “horizontal”surface (table, air track, …)
may be in equilibrium
for y
:
a
0
F
y
for
m
"E
qu
ilib
riu
"
yy
= ==== ===
↔ ↔↔↔∑ ∑∑∑
FB
D
m
jm
g
F g
− −−−= ===
r
N
ay
= 0
� ���
N =
Fg
(mdoes not accelerate)
su
rface
to
la
rp
erp
en
dic
u
fo
rce"
n
orm
al
"
N
≡ ≡≡≡≡ ≡≡≡
N is a contact force that adjusts to
Fg
Fgpushes on the surface –
-the surface pushesback with N
If a
ynot = 0, N
does not equal
Fg
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Newton’s Third Law
Bodies interact by pushing or pulling on each other
3rd
Law
(an
tiq
ue v
ers
ion
): E
ach
acti
on
has a
n e
qu
al
an
d o
pp
osit
e r
eacti
on
Mo
re m
od
ern
ve
rsio
n:
Wh
en
tw
o b
od
ies in
tera
ct
the f
orc
es t
hat
each
exert
s o
n t
he o
ther
are
alw
ays e
qu
al
in m
ag
nit
ud
e a
nd
op
po
sit
e in
dir
ecti
on
F
F 21
12
rr
− −−−= ===
Example: gravity acting at a distance
2
ob
ject
to
du
e 1
ob
ject
o
n
forc
e
F ≡ ≡≡≡
12
r
1 o
bje
ct
to
du
e
2 o
bje
ct
o
n
forc
e
F ≡ ≡≡≡
21
r
If you ever find a force w/o the 3
rdlaw reaction,
you can build a perpetual motion machine
Example: box on a level surface
•F
gis
th
e p
ull
of
Eart
h o
n t
he b
ox (
weig
ht)
•T
he 3
rdla
w r
eacti
on
is F
e -
the b
ox’s
pu
ll o
n t
he E
art
h•
Nis
th
e s
urf
ace’s
pu
sh
on
th
e b
ox
•F
sis
th
e b
ox’s
pu
sh
on
th
e s
urf
ace
•O
NL
Y f
orc
es
on
th
e b
ox (
Fg
& N
) a
ffect
it’s
mo
tio
n•
Fg
& N
are
NO
T a
3rd
law
pair
(F
sb
& N
are
a p
air
)•
Wh
y t
hen
do
es F
g=
N ?
??
m
jm
g
F g
− −−−= ===
r
N FeF
s
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Free Body Diagrams (FBDs)
Drawing the FBDsis the most important step in analyzing motion.
•DRAW FBDsFIRST –
before you start writing down equations.
•Pictorial sketches are not the same as FBDs.
•Model bodies in your system as point particles. There may be
several. Som
etimes you can treat the system as one object.
•Choose coordinates.
•Include in FBDsonly forces that act O
N your system.
•Exclude forces exerted BY bodies in your system on other bodies.
•Neglect internal forces. When you break up a system for analysis,
INCLUDE formerly internal forces that become external.
•Don’t forget action-at-a-distance forces (fields) such a gravity
m
F g
r
N
F g
r
m
NM
jM
g
F g
− −−−= ===
r
N
m
jm
g
F
' g− −−−
= ===
rIs this a FBD?
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Friction F
ricti
on
less
m
gFNF
Sli
din
g o
r sta
tic
fric
tio
n f
(la
ter)
m
gFNF
f
No
fri
cti
on
para
llel
to s
urf
ace
Fri
cti
on
is a
resis
tive f
orc
e p
ara
llel
to s
urf
ace
m/F
ax
= ===m/)f
F(a
x− −−−
= ===N
f∝ ∝∝∝
Co
nta
ct
forc
e -
alw
ays o
pp
ose
d t
o m
oti
on
Cords
Ten
sio
n o
nly
, n
o c
om
pre
ssio
n
Pu
llin
g c
rea
tes t
en
sio
n T
–th
e f
orc
e t
ran
sm
itte
d b
y t
he
co
rdT
is
th
e s
am
e e
ve
ryw
here
in
a z
ero
-mass
, u
ns
tretc
hab
leco
rd
3rdlaw pair
T
mSu
pp
ort
FB
D f
or
bo
dy
mT Fg
FB
D f
or
co
rd
TT’=
T
3rdlaw pair
FB
D f
or
su
pp
ort
T’
F
Eq
uilib
riu
mF
'T
TF g
= ==== ===
= ===
FBDs: show only forces on bodies
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Newton’s Laws -Summary
Newton’s First Law
A b
ody’s
velo
city is c
onsta
nt (
)
if th
e n
et exte
rnal fo
rce o
n it is
zero
0= ===
ar
-M
otion is a
long a
str
aig
ht lin
e-
Fin
d a
nd u
se a
n inert
ial fr
am
e o
f re
fere
nce
Newton’s Second Law
am
vecto
r
forc
e
net
F
F
ii
net
rr
r= ===
= ==== ===∑ ∑∑∑
In C
art
esia
n c
om
ponents
:
zz
yy
xx
ma
F
ma
F
ma
F
∑ ∑∑∑∑ ∑∑∑
∑ ∑∑∑= ===
= ==== ===
Newton’s Third Law
If b
ody A
exert
s a
foce
on b
ody B
, th
en b
ody B
exert
s a
nd e
qual and
Opposite forc
e o
n b
ody A
.
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Method for solving Newton’s Second Law problems
Systems with several components may have several unknowns….
…and need an equal number of independent equations
•Draw or sketch system. Adopt coordinates. N
ame the variables,
•Draw free body diagrams. Show forces acting on particles. Include
gravity (weights), contact forces, normal forces, friction.
•Apply Second Law to each part
•Make sure there are enough (N) equations; Extra conditions connecting
unknowns (constraint equations) may be applicable
•Simplify and solve the set of (simultaneous) equations.
•Interpret resulting form
ulas. Do they make intuitive sense? Are the
units correct? Refer back to the sketches and original problem
•Calculate num
erical results, and sanity check anwers
(e.g., right order of
magnitude?)
am
FF
in
et
rr
r= ===
= ===∑ ∑∑∑
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: Traffic Light in Equilibrium
Co
ncep
tuali
ze:
cab
les a
re m
assle
ss
an
d d
on
’t b
reak
no
mo
tio
n
Cate
go
rize:
eq
uil
ibri
um
pro
ble
m –
accele
rati
on
s =
0M
od
el
as p
art
icle
s i
n e
qu
ilib
riu
m2 F
BD
s
T3 Fg
FB
D o
f L
igh
tF
BD
of
Kn
ot
Fg
= 1
22 N
So
lve u
pp
er
for
T2:
FB
D o
f lig
ht
yie
lds T
3=
Fg
( a
lig
ht=
0)
FB
D o
f kn
ot
yie
lds:
)co
s(
T)
co
s(
T0
F
oo
2x
37
53
1− −−−
= ==== ===
∑ ∑∑∑
31
37
53
T)
sin
(T
)sin
(T
0
F
oo
2y
− −−−+ +++
= ==== ===
∑ ∑∑∑
11
53
37
33
1T
.T
T)
oc
os
(
)o
co
s(
2= ===
= ===
N .
)]
sin
(
.)
[sin
(
To
o22
153
33
137
1= ===
+ +++
N
.
T
47
31
= ===
N .
T 4
97
2= ===
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: Particle M
otion Under a N
et Force
mN
F
W
θ θθθ
x
yM
ass m
is m
ovin
g o
n a
fri
cti
on
less h
ori
zo
nta
l su
rface,
acte
d o
n b
y a
n e
xte
rnal
forc
e o
f m
ag
nit
ud
e F
, m
akin
g a
n a
ng
le θ θθθ
wit
h t
he x
-axis
.
Fin
d e
xp
ressio
ns f
or
the a
ccele
rati
on
alo
ng
th
e h
ori
zo
nta
l an
d v
ert
ical
dir
ecti
on
s
W =
weig
ht
Along x:
xx
ma
)
co
s(
F F
= ===
θ θθθ= ===
∑ ∑∑∑
m
)co
s(
F
a
x
θ θθθ= ===
Set
ay =
0.
Cro
sso
ve
r to
ay >
0w
hen
N a
lso
=0, i.
e, w
hen
Along y: Is
ayzero, or does particle accelerate upward?
yy
ma
W
N )
sin
(F
F
= ===− −−−
+ +++θ θθθ
= ===∑ ∑∑∑
W
N )
sin
(F
0 ⇒ ⇒⇒⇒
− −−−+ +++
θ θθθ= ===
W
)F
sin
(
= ===θ θθθ
When
Fyis > the weight, the
particle accelerates upward
m
W
)sin
(F
a
y
− −−−θ θθθ
= ===
N
0= ===
When
Fyis < the weight, the
particle does not accelerate
a
y0
= === )
sin
(F
W
N θ θθθ
− −−−= ===
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
4-3
: T
he
man
an
d t
he p
latf
orm
weig
h a
to
tal
of
500 N
. H
e p
ulls
up
ward
o
n t
he r
op
e w
ith
fo
rce F
. W
ha
t fo
rce w
ou
ld h
e n
eed
to
exert
in
ord
er
to a
ccele
rate
up
ward
wit
h a
= 0
.1 g
?
Is t
his
po
ssib
le?
a)
F =
50 N
b)
F =
1000 N
c)
F =
550 N
d
) F
= 5
00 N
e)
He
can
no
t li
ft h
imself
by h
is o
wn
bo
ots
trap
s a
t all
.
Bootstraps
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: Sliding and Hanging Blocks
Blo
ck S
, m
ass
M is
sli
din
g o
n a
fri
cti
on
less
ho
rizo
nta
l su
rfa
ce. B
lock H
, m
ass m
han
gs
fro
m a
m
assle
ss,
un
str
etc
hab
leco
rd w
rap
ped
over
a
massle
ss
pu
lle
y.
Fin
d e
xp
ressio
ns f
or
the
accele
rati
on
s o
f th
e
blo
cks a
nd
th
e t
en
sio
n in
th
e c
ord
.
W’=
mg
Mg
W= ===
NT
T’
No
fri
cti
on
,N
o m
as
s
W =
Mg
W =
Mg
NT
FBD for Block S
a
Ma
T
F
xs
= ==== ===
∑ ∑∑∑0
≡ ≡≡≡= ===
− −−−= ===
∑ ∑∑∑ys
ys
Ma
W
N
F
0= ===
= ===∑ ∑∑∑
xh
xh
ma
F
'm
a
T'
W
'F
yh
= ===− −−−
= ===∑ ∑∑∑
WW’’=
mg
= m
g
T’
FBD for Block H
a’
choose
positive down
Apply 2
ndLaw to blocks S & H separately for x & y
Constraints:
T’=
T,
a’
= a
Eliminate T,T’,a’
ma
Ma
W
'= ===
− −−−
Ma
m
a
mg
+ +++= ===
g
Mm
m
a
+ +++= ===
Find formula for T
g
MmM
m
M
a
T
+ +++
= ==== ===
could also use
system approach
To find this
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: Block Sliding on a Ramp [“Inclined Plane”]
Mass m
is a
cc
ele
rati
ng
alo
ng
a f
ricti
on
less
incli
ned
su
rface a
s s
ho
wn
, m
akin
g a
n a
ng
le θ θθθ
wit
h t
he h
ori
zo
nta
l.
Fin
d e
xp
ressio
ns f
or
the a
ccele
rati
on
an
d t
he n
orm
al
forc
e
mN
a
θ θθθW
= m
g
Wh
y d
oes t
he b
lock a
ccele
rate
?
Do y
ou e
xpect
N to e
qual W
?Forces acting ON the block are N
and W
•N is norm
al to the surface
•W is vertical as usual
Choose x-yaxes aligned to ramp, for which:
y
x
θ θθθ
N
W
90
90
90
90
− −−−θ θθθ
θ θθθW
y
Wx
rig
ht)
&
do
wn
(p
osit
ive
x
yA
ssu
me
a
a
,a
≡ ≡≡≡= ===
0F
BD
Apply 2nd Law to x and y
) W
sin
( W
)co
s(
WW
xy
θ θθθ= ===
θ θθθ= ===
)sin
(m
gm
a
W
F
x
xx
θ θθθ= ===
= ==== ===
∑ ∑∑∑
0
)m
gco
s(
N
WN
F
yy
= ===θ θθθ
− −−−= ===
− −−−= ===
∑ ∑∑∑
)m
gc
os
(
N θ θθθ
= ===
)g
sin
(
a
a
x
θ θθθ= ===
= ===
Does not depend on m
Check:
What happens as
θ θθθ� ���
90o
as
θ θθθ� ���
0o
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: “Atwood’s M
achine”with M
assless
Pulley
Bo
th m
asses
ha
ve
th
e s
am
e a
cc
ele
rati
on
a (
co
nstr
ain
t).
Th
e
ten
sio
n T
in
th
e u
ns
tre
tch
ab
lec
ord
is t
he
sam
e o
n b
oth
sid
es
of
the m
assle
ss
pu
lle
y (
an
oth
er
co
ns
train
t).
Fin
d e
xp
ressio
ns f
or
the
accele
rati
on
an
d t
he
ten
sio
nIn
th
e c
ord
.
Fin
d t
he f
orc
e W
totsu
pp
ort
ing
th
e p
ull
ey
a
a
Wto
t
No forces or
motion along x
am
g
mT
F
1
y= ===
− −−−= ===
∑ ∑∑∑1
1
T
m1g
aFBD for m
1
T
m2g
a
FBD for m
2
am
T
gm
F
2y
= ===− −−−
= ===∑ ∑∑∑
22
Add the equations
am
a
m T
g
m
gm
T
2
11
2+ +++
= ===− −−−
+ +++− −−−
g
m
m
mm
a
22
11
+ +++− −−−= ===
a =
0 f
or
m1
= m
2a i
s c
lockw
ise f
or
m2
> m
1 a
= g
fo
r m
1=
0
or
a =
-g
fo
r m
2=
0
Subtract the equations
am
a
m
T
gm
g
m
T
21
12
+ +++− −−−
= ===+ +++
− −−−− −−−
g
m
m
m2m
T
2
1
1
2
+ +++= ===
T =
0 f
or
m1
or
m2
eq
uals
zero
.
T =
m
1g
fo
r m
2=
m1
Wto
t
TT
0
2T
W
tot
= ===− −−−
FBD
for
pulley
g
m
m
m4m
W
2
1to
t12
+ +++= ===
Wto
t=
2m
1g
if
m2
= m
1
Oth
erw
ise n
ot
so
Co
pyri
gh
t R
. J
an
ow
–S
pri
ng
2012
Example: Your Weight in an Elevator
A p
assen
ger
wh
ose m
ass
m
=
72.2
kg
is
sta
nd
ing
on
a
pla
tfo
rm s
cale
in
an
ele
va
tor.
Wh
at
weig
ht
do
es t
he
scale
rea
d f
or
him
as
th
e e
leva
tor
(an
d
him
se
lf)
accele
rate
s u
p a
nd
do
wn
?
No forces or
motion along x
N
mg
F g
= ===FBD for
passenger
+
•F
g=
mg
is the real weight, which doesn’t change
•The building is an inertial frame, as is the elevator
when traveling at constant speed.
•When the elevator and passenger are accelerating
their non-inertial frame � ���
fictitious forces
N
is t
he s
cale
read
ing
= a
pp
are
nt
weig
ht
•Apply Second Law in the building’s reference frame
am
m
gN
F
y= ===
− −−−= ===
∑ ∑∑∑ )
ga(
m
N + +++
= ===
Interpretations:
N
= m
g
for
a
=
0N
orm
al w
eig
ht
for
ele
va
tor
at
rest
or
mo
vin
g w
ith
co
ns
tan
t v
N
> m
g
for
a
>
0In
cre
ased
ap
pare
nt
weig
ht
for
ele
va
tor
accele
rati
ng
up
N
< m
g
for
a
<
0D
ecre
ased
ap
pa
ren
t w
eig
ht
for
ele
va
tor
accele
rati
ng
do
wn
mg
=
fo
rce
exe
rted
by g
ravit
y
N
= 0 f
or
a =
-g
Fre
e f
all
-w
eig
htl
ess
Fic
titi
ou
s f
orc
e a
pp
ears
in
no
n-i
nert
ial
fra
me
ve
locit
y h
as n
o e
ffect
on
N –
ap
pare
nt
weig
ht