Circular Motion Gravitation Labs
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MISC
Subject
Physics
Date
Jan 9, 2024
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AP
Physics
B
Course
Outline
%
on
Dates
Unit
Exam
Title
Possible
Labs
Math
and
Data
Collection
Review
8/19-8/23
-Round
Things
-Determining
G
using
a
spring
scale
Newtonian
Mechanics
Kinematics
(1D/2D)
15
8/26-9/13
Kinematics
LTF
#1
Constant
Velocity
LTF
#2
Acceleration
on
a
Ramp
LTF
#3
Not-So
Free
Fall
LTF
#4
Freefalling
Washers
LTF
#5
Vector
Scavenger
Hunt
LTF
#6
Map
of
Texas
LTF
#7
Projectile
Motion
LTF
#8
Dart
Gun
-Force
Tables
Newton’s
Laws
17
9/16-10/8
Newton’s
Laws
LTF
#9
Newton's
2"
Law
LTF
#10
Atwood
Machine
LTF
#11
Coefficient
of
Friction
Work,
Power,
and
Energy
10/9-10/18
Work,
Power,
and
Energy
LTF
#15
Running
the
Stairs
LTF
#18
Roller
Coaster
Momentum
10/21-10/31
Momentum
LTF
#13
Crumple
Zone
LTF
#14
Conservation
of
Momentum
Particles/linear
momentum
Circular
Motion/Gravitation
14
11/7-11/22
Circular
Motion/Gravitation
Circular
motion/rotation
LTF
#12
Centripetal
Force
-Kepler's
Laws
Virtual
Lab
Oscillation/gravitation
LTF
#21
Waves
in
a
Spring
LTF
#16
The
Pendulum
Swings
LTF
#17
Simple
Harmonic
Motion
Wave
Motion
and
Sound
2/26-3/7
Wave
motion
and
sound
Fluid
mechanics
and
thermal
15
Thermodynamics
and
Fluids
13
11/25-12/13
Thermodynamics
&
Fluids
Fluid
mechanics
-Buoyancy
lab
-Pressure-depth
lab
Temperature
&heat
-Calorimetry
lab
Kinetic
theory/thermo
Electricity
and
magnetism
25
Centripetal
Force
Exploring
Uniform
Circular
Motion
An
object
that
moves
in
a
circle
at
constant
speed,
v,
is
said
to
experience
uniform
circular
motion
(UCM).
The
magnitude
of
the
velocity
remains
constant,
but
the
direction
of
the
velocity
is
continuously
changing,
as
shown
in
Figure
1.
Figure
]
Notice
that
the
velocity
vectors
are
not
pointing
in
the
same
direction.
The
velocity
vector
is
always
tangent
to
the
circular
path.
This
is
why,
should
the
string
break,
the
object
flies
off
in
a
straight
line.
Figure
2
An
object
revolving
in
a
circle
is
continuously
accelerating,
even
when
the
speed
remains
constant.
The
acceleration
vector
is
always
pointing
toward
the
center
of
the
circular
path
and
it
is
always perpendicular
to
the
velocity
vector,
as
shown
in
Figure
2.
Centripetal
(center-seeking)
acceleration,
a.,
is
defined
as:
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2012
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If
we
measure
the
period,
7,
the
time
needed
for
the
object
to
make
a
complete
revolution,
we
can
calculate
the
speed
of
the
object
in
UCM.
During
this
time,
it
travels
a
distance
equal
to
the
circumference
of
the circle,
277,
where
r
is
the
radius
of
the
circular
path.
The
object’s
speed,
then,
is
represented
by
v
=
%
According
to
Newton’s
second
law
(XF
=
ma),
an
object
that
is
accelerating
must
have
a
net
force
acting
upon
it
and
we
call
this
force
centripetal
force.
This
force
is
acting
in
the
same
direction
as
the
acceleration
which
is
toward
the
center
of
the
circle
(Figure
3).
Figure
3
The
equation
for
centripetal
force
can
be
expressed
as
271\
[vz}
T
an’y
F=ma=ma,=m|—
|=m|——|=m
r
Centripetal
force
is
the
net
force
which
points
toward
the
center
of
the
circle,
and,
as
examples,
can
take
the
form
of
a
gravitational
force,
frictional
force,
or
tension
in
a
string.
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
All
rights
reserved.
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us
online
at
www./tftraining.org.
PURPOSE
In
this
activity
you
will
verify
the
relationship
between
centripetal
force,
mass,
and
ve1001ty
in
an
object
in
uniform
circular
motion.
You
will
be
using
the
assumption
that
the
centripetal
force
generated
by
the
whirling
stopper
balances
the
force
of
weight
for
the
hanging
mass.
MATERIALS
Each
lab
group
will
need
the
followmg
calculator,
TI®
graphing
Centripetal
Force
Apparatus,
set
meter
stick
stopwatch
washers
or
hanging
weight
set
SAFETY
ALERT
1.
Goggles
must
be
worn
at
all
times.
2.
Make
sure
you
have
enough
room
to
swing
your
stopper
without
hitting
other
students.
3.
Check
to
see
that
your
cord
is
not
frayed
before
beginning
your
experiment.
PROCEDURE
1.
Put
your
goggles
on
and
leave
them
on
for
the
entire
laboratory
period.
2.
One
partner
should
construct
your
apparatus
as
pictured
in
Figure
4
below.
Rubber
stopper
T
Glass
tube
wrapped
with
tape
Figure
4
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
All
rights
reserved.
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us
online
at
www.ltftraining.org.
10.
a.
Mass
the
rubber
stopper
and
record
its
mass
in
kilograms
in
Data
Table
1
on
your
student
answer
page.
Attach
one
end
of
the
cord
securely
to
the
rubber
stopper.
b.
Pass
the
other
end
of
the
cord
through
the
glass
or
plastic
tube.
¢.
Bend
a
large
paperclip
into
a
hook
and
attach
it
to
the
free
end
of
the
cord.
This
hook
needs
to
support
several
large
washers.
.
The
other
partner
should
use
a
balance
to
mass
your
group’s
washers
+
hook.
Keep
adding
washers
until
the
mass
exceeds
100
grams.
Record
the
mass
of
your
stack
of
washers
and
hook
in
kilograms
in
Data
Table
1
on
your
student
answer
page.
Load
the
stack
of
washers
onto
the
hook.
If
the
stack
is
too
large
to
hang
securely
from
the
hook,
you
can
secure
the
stack
together
with
a
piece
of
string
and
hang
the
string
from
the
hook.
If
you
choose
this
method,
re-weigh
your
hook
as
well
as
the
stack
of
washers
with
the
string
attached.
Adjust
the
cord
so
that
there
is
about
0.75
m
of
cord
between
the
top
of
the
tube
and
the
stopper.
The
partner
that
is
going
to
operate
the
apparatus
should
support
the
stack
of
washers
in
one
hand
and
hold
the
tube
with
the
other.
Begin
whirling
the
stopper
by
moving
the
tube
in
a
circular
motion.
Slowly
release
the
stack
of
washers
and
adjust
the
speed
of
the
stopper
so
that
the
stack
of
washers
remains
relatively
stationary,
meaning
the
stack
is
no
longer
climbing
or
falling.
Important:
Keep
the
stopper
whirling
in
an
elevated,
horizontal
circle
as
pictured
in
Figure
4.
The
tube
should
be
held
high
enough
in
the air
so
that
the
spinning
stopper
does
not
threaten
any
part
of
the
spinner’s
head.
Make
several
trial
runs
to
master
the
technique.
Be
mindful
of
your
space
so
that
you
do
not
accidentally
hit
any
other
students
with
your
spinning
stopper.
When
you
have
learned
how
to
keep
the
velocity
of
the
stopper
and
the
position
of
the
washers
relatively
constant,
have
your
partner
measure
the
time
it
takes
for
20
revolutions
by
counting
down
the
revolutions
“5,4,3,2,1,
go!
1,2,3,
....
”
Record
this
time
in
Data
Table
1
on
your
student
answer
page.
The
partner
with
the
apparatus
should
stop
the
whirling
stopper
by
placing
his
or
her
finger
at
the
fop
of
the
tube
so
as
to
capture
the
length
of
the
radius
of
your
circle.
Use
caution
when
performing
this
task
so as
not
to
be
hit
by
the
stopper.
Once
the
stopper
comes
to
rest,
keep
your
finger
in
place
so
that
the
length
of
the
cord
will
not
change.
Measure
the
radius,
r,
from
the
center
of
the
tube
to
the
center
of
the
stopper.
Use
the
appropriate
number
of
significant
digits
and
record
the
value
in
Data
Table
1
on
your
student
answer
page.
Repeat
the
procedure
for
two
additional
trials
keeping
the
same
stopper
and
the
same
stack
of
washers,
but
varying
the
radius.
Keep
the
radius
between
0.50
m
and
0.90
m.
Record
all
data
to
the
appropriate
number
of
significant
digits
in
your
data
table.
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2012
Laying
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Texas.
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rights
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11.
Repeat
the
procedure
for
three
additional
trials
keeping
the
same
radius
[you
may
need
to
mark
your
cord
at
the
point
where
it
exits
the
tube
so
you
can
have
a
visual
cue
that
your
radius
is
consistent]
but
varying
the'size
of
your
stopper.
Record
all
data
to
the
appropriate
number
of
significant
digits
in
your
data
table.
12.
Repeat
the
procedure
for
a
final
three
trials
keeping
the
same
radius
and
same
stopper,
but
varying
the
mass
of
your
washer
stack.
Record
all
data
to
the
appropriate
number
of
significant
digits
in
your
data
table.
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
All
rights
reserved.
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us
online
at
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Centripetal
Force
Exploring
Uniform
Circular
Motion
DATA
AND
OBSERVATIONS
IS
o
T
e
e
|
AR
P
DDatanlableil
B
ST
A
S
T
T
T
|
e
Trial
Mass
of
Mass
of
stopper
Total
Time
Radius
Washers
(kg)
(ke)
(s)
(m)
Copyright
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2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
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rights
reserved.
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us
online
at
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ANALYSIS
1.
Calculate
the
force
of
weight,
Fiy,
of
the
hanging
mass
and
enter
it
in
Table
2
as
centripetal
force,
F..
F,
=mg=F,
and
g=9.8fl2
s
2.
Calculate
the
period
of
revolution
by
dividing
the
total
time
by
the
number
of
revolutions
and
enter
it
in
Table
2.
time(s)
-
20
revolutions
3.
Calculate
the
circumference
of
revolution
from
the
radius
and
enter
it
inTable
2.
circumference
=
zd
=
27zr
4.
Use
the
circumference
and
period
to
find
the
velocity
and
enter
it
in
Table
2.
circumference
V
=
-
T
11010
(PR
OF.N
D
@)
B)
B7.§
4
(O
AN
Trial
Centripetal
Force,
F
Period,
T
Circumference
Velocity
N)
(s)
(m)
(m/s)
1
2
3
4
5
6
7
8
9
Copyright
©
2012
Laying
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Foundation®,
Inc.,
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Texas.
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rights
reserved.
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CONCLUSION
QUESTIONS
1.
Survey
the
data
in
Table
2.
What
is
the
relationship
between
the
velocity
of
a
whirling
object
and
the
centripetal
force
that
is
exerted
on
it?
What
is
the
relationship
between
the
radius
of
revolution
and
the
velocity
of
an
object
in
uniform
circular
motion?
What
is
the
relationship
between
the
mass
and
velocity
of
an
object
in
uniform
circular
motion?
Step
one
of
the
analysis
section
assumes
that
'y
=
F,
by
using
the
assumption
that
the
centripetal
force
supplied
by
the
weight
of
the
washers
causes
the
whirling
stopper
to
move
in
a
curved
path.
What
additional
assumption
is
made
regarding
the
value
for
the
centripetal
acceleration?
A
student
neglects
to
reweigh
the
stack
of
washers
after
tying
them
together
before
performing
one
of
the
trials.
How
will
this
error
affect
the
reported
centripetal
force?
State
clearly
whether
the
centripetal
force
increases,
decreases,
or
remains
the
same
and
mathematically
justify
your
answer.
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
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rights
reserved.
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us
online
at
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6.
A
13.0-g
rubber
stopper
is
attached
to
a
0.93-m
string.
The
stopper
is
swung
in
a
horizontal
circle,
making
one
revolution
in
1.18s.
Calculate
the
centripetal
force
exerted
by
the
string
on
the
stopper.
7.
A
coin
is
placed
on
a
vinyl
stereo
record
making
33'
revolutions
per
minute.
a.
In
what
direction
is
the
acceleration
of
the
coin?
b.
Calculate
the
magnitude
of
the
acceleration
when
the
coin
is
placed
10.0
cm from
the
center
of
the
record.
8.
A
carnival
ride
has
a
2.0
m
radius
and
rotates
once
each
0.90
s.
a.
Calculate
the
speed
of
a
rider
at
this
radius.
b.
Calculate
the
centripetal
acceleration
of
the
rider.
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
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rights
reserved.
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us
online
at
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9.
As
you
whirled
the
mass
in
a
circular
path,
you
did
your
best
to
keep
it
swinging
in
a
horizontal
circle.
Is
it
possible
to
keep
the
mass
whirling
in
a
perfectly
horizontal
circle
(parallel
to
the
floor)?
Explain
your
answer
and
draw
and
label
the
forces acting
on
the
mass
from
a
side
view
using
the
diagram
below.
i
B
10.
A
student
tries
to
swing
a
stopper
of
mass
40
grams
in
a
horizontal
circle,
but
finds
that
the
stopper
“droops”
down
a
little
due
to
the
gravitational
force
acting
on
the
stopper,
as
shown
in
the
figure
below. The
string
has
a
length
L =
0.50
m,
and
is
swung
so
that
it
remains
an
angle
of
8
=
60°
from
the
vertical.
Sy
O
el
e
i
e
a.
On
the
diagram
above,
draw
and
label
all
of
the
forces
acting
on
the
stopper
as
it
travels
around
the
circle.
(Remember:
centripetal
force
is
not
an
“extra”
force
that
acts
on
the
mass,
but
is
the
sum
of
the
forces
which
point
toward
the
center
of
the
horizontal
circle.)
b.
Can
we
say
that
the
tension
in
the
string
is
the
centripetal
force?
Explain
your
answer.
c.
Show
the
horizontal
and
vertical
components
of
the
tension
force
on
the
diagram
above.
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2012
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d.
Determine
the
vertical
component
7},
of
the
tension
in
the
string.
e.
Determine
the
horizontal
component
7
of
the
tension
in
the
string.
f.
Determine
the
tangential
speed
v
necessary
to
keep
the
mass
revolving
in
this
circle.
Copyright
©
2012
Laying
the
Foundation®,
Inc.,
Dallas,
Texas.
All
rights
reserved.
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us
online
at
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Physics
SITF
LAYING
THE
FOUNDATION
Building
Academic
Excellence
The
Pendulum
Swings
Happiness
Is
A
Straight
Line
In
this
activity,
you
will
determine
the
relationship
between
the
period
7
of
a
pendulum
and
its
mass
m,
amplitude
4,
and
length
L.
Your
teacher
will
instruct
you
on
how
to
construct
your
pendulum.
You
will
make
and
record
measurements
throughout
this
activity,
and
you
will
create
your
own
graphs
to
display
your
data.
Purpose
You
will
investigate
the
relationship
between
the
mass,
amplitude,
and
length
of
a
pendulum
and
its
period.
From
the
data
collected,
you
will
also
apply
your
graphing
skills
either
manually
or
by
using
computer
graphing
software
to
generate
graphs
and
find
relationships.
You
will
also
linearize
your
data
if
necessary.
Materials
Each
lab
group
will
need
the
following:
meter
stick
string
protractor,
with
hole
tape,
masking
scissors
3
washers,
2
in.
stopwatch
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1
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Student
Activity
—
The
Pendulum
Swings
Procedure
1.
Listen
carefully
to
your
teacher’s
instructions.
You
will
be
asked
to
describe
your
actual
procedure
in
your
laboratory
report.
2.
Organize
your
data
according
to
the
three
data
tables
following,
and
use
a
computer
graphing
program
or
graph
paper
to
graph
the
period
versus
each
of
the
variables
tested
(mass,
amplitude,
and
length).
For
this
activity,
keep
the
period
on
the
y-axis
for
each
graph.
|
0.40
10
1
0.60
10
1
0.80
10
1
1.00
10
1
1.20
10
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2
Student
Activity
—
The
Pendulum
Swings
Lab
Report
Include
the
following
sections
when
writing
your
lab
report:
I.
Title
II.
Purpose
III.
Apparatus
(labeled
sketch)
IV.
Procedure
V.
Data
VI.
Analysis
VII.
Conclusion
(include
the
answers
to
the
Conclusion
Questions
here)
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3
Student
Activity
—
The
Pendulum
Swings
Conclusion
Questions
1.
What
are
the
variables
in
this
experiment?
2.
What
data
should
be
recorded
for
your
pendulum?
3.
What
steps
did
you
take
to
maximize
accuracy
and
precision,
and
minimize
your
systemic
error
while
collecting
your
data?
4.
What
effect
does
varying
the
mass
of
the
pendulum
have
on
its
period?
Justify
your
answer.
5.
What
effect
does
varying
the
amplitude
of
the
swing
of
the
pendulum
have
on
its
period?
Justify
your
answer.
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Student
Activity
-
The
Pendulum
Swings
Conclusion
Questions
(continued)
6.
What
effect
does
varying
the
length
of
the
pendulum
have
on
its
period?
Justify
your
answer.
7.
According
to
your
data
relating
the
period
of
the
pendulum
to
its
length,
would
it
be
accurate
to
say
that
the
period
of
a
pendulum
is
directly
proportional
to
its
length,
inversely
proportional
to
its
length,
directly
proportional
to
the
square
of
the
length,
or
directly
proportional
to
the
square
root
of
the
length?
Explain
your
answer.
8.
Add
another
column
to
your
data
table
for
length
variations
and
square
the
period.
Graph
the
period
squared
versus
the
length.
Write
an
equation
that
relates
the
period
to
the
length,
and
include
the
value
of
the
slope.
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5
Student
Activity
—
The
Pendulum
Swings
Conclusion
Questions
(continued)
9.
You
will
be
given
a
period
and
asked
to
calculate
and
construct
a
pendulum
of
the
appropriate
length
using
the
equation
you
derived.
Your
teacher
will
time
your
pendulum
and
its
period.
Use
the
space
provided
to
calculate
the
length
of
your
pendulum
and
to
compute
your
percent
error.
10.
Use
the
slope
of
your
straight
line
and
rearrange
the
equation
for
a
simple
pendulum,
T=27r\/Z
g
to
determine
a
value
for
the
acceleration
due
to
gravity,
g.
Find
the
percent
error
between
your
value
for g
and
the
accepted
value
of
9.81
m/s?.
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6
Simple
Harmonic
Motion
Investigating
a
Mass
Oscillating
on
a
Spring
A
spring
that
is
hanging
vertically
from
a
support
with
no
mass
at
the
end
of
the
spring
has
a
length
L
(called
its
rest
length).
When
a
mass
is
added
to
the
spring,
its
length
increases
by
x.
The
equilibrium
position
of
the
mass
is
now
a
distance
L
+
x
from
the
spring’s
support.
The
spring
exerts
a
restoring
force,
'
=
-kx,
where
x
is
the
distance
the
spring
is
displaced
from
equilibrium
and
k
is
the
force
constant
of
the
spring
(also
called
the
spring
constant).
The
negative
sign
indicates
that the
force
exerted
by
the
spring
on
the
mass
is
directed
opposite
to
the
direction
of
the
displacement
of
the
mass.
The
restoring
force
causes
the
mass
to
oscillate
up
and
down,
and
is
always
directed
toward
the
equilibrium
position.
The
period
of
oscillation
depends
on
the
mass
and
the
spring
constant.
PURPOSE
In
this
lab
you
will
determine
the
spring
constant
for
a
spring,
predict
the
period
of
oscillation
for
several
different
masses
using
the
measured
spring
constant,
and
find
their
relative
error.
A
graph
of
position
vs.
time
and
velocity
vs.
time
for
a
mass
in
simple
harmonic
motion
will
be
constructed
and
analyzed
for
the
energy
aspects
of
the
motion.
MATERIALS
Each
lab
group
will
need
the
following:
calculator,
TI®
graphing
clamp,
pendulum
computer
electronic
file
LabQuest®
meter
stick
ring
stand
sensor,
motion
detector
spring
weights,
hanging
sets
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PROCEDURE
PART
I:
FINDING
THE
SPRING
CONSTANT
&
1.
Attach
a
clamp
to
a
ring
stand
so
that
your
spring
will
hang
over
the
edge
of
the
table.
I
1~
Z
v
Figure
1
2.
Hang
a
mass
hanger
on
the
spring
so
that
it
will
slightly
stretch
your
spring
and
hang
at
rest.
With
your
meter
stick,
measure
the
distance
from
the
bottom
of
the
hanger
to
the
floor
where
the
motion
detector
will
eventually
be
positioned.
Make
all
successive
measurements
from
this
same
position,
which
will
serve
as
the
equilibrium
position.
This
will
be
considered
your
unstretched
length.
3.
Measure
the
amount
of
stretch
for
5
different
masses
added
to
the
spring.
The
amount
of
stretch
is
the
difference
between
the
unstretched
length
and
the
stretched
length.
Record
your
measurements
in
Data
Table
1
on
your
student
answer
page.
PART
II:
ADDITIONAL
METHOD
FOR
FINDING
THE
SPRING
CONSTANT
K
1.
Attach
a
motion
detector
to
your
computer
and
start
the
appropriate
software.
2.
Place
the
motion
detector
on
the
floor
directly
beneath
the
spring.
Make
sure
that
the
mass
does
not
come
closer
than
the
measurement
limit
for
your
motion
detector,
usually
15
cm
for
Vernier
motion
detectors
or
PASCO
Motion
Detector
II’s.
When
Logger
Pro
is
opened,
if
it
does
not
automatically
identify
your
motion
detector, then
drag
the
motion
detector
icon
to
Digital
Channel
1.
A
graph
of
position
vs.
time
and
a
second
graph
of
velocity
vs.
time
should
open.
"W
I~
Figure
2
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3.
Using
each
of
the
5
masses
from
Part
I,
set
the
mass
into
smooth
oscillations,
with
amplitudes
of
about
10
cm
(depending
on
the
original
length
of
your
spring).
Start the
motion
detector
data
collection.
Gather
data
for
about
3
seconds
or
until
you
have
more
than
10
complete
oscillations
with
each
of
the
5
masses.
4.
Using
the
analysis
tool
on
Logger
Pro
or
your
software,
find
the
time
for
ten
complete
oscillations
of
your
spring.
Record
this,
as
well
as
the
mass
on
the
spring,
in
Table
2
on
your
student
answer
page.
PART
III:
ENERGY
IN
SIMPLE
HARMONIC
MOTION
1.
With
the
motion
detector
placed
on
the
floor
as
in
Part
II,
zero
the
motion
detector
when
the
mass
is
motionless.
To
zero
the
motion
detector,
click
on
the
LabPro
icon
on
the
tool
bar.
Double
click
on
the
motion
sensor
icon,
and
then
select
“zero”.
This
is
your
equilibrium
position.
This
will
have
to
be
repeated
with
each
mass.
2.
Set
the
mass
into
smooth
oscillations
with
amplitude
of
about
10
cm
(depending
on
the
original
length
of
your
spring).
Collect
data
for
about
three
seconds.
3.
Using
the
analysis
tool,
determine
both
the
position
and
velocity
for
the
mass
at
its
maximum
amplitude
and
for
the
next
position
of
zero
amplitude.
Record
these
values
in
Table
3
on
your
student
answer
page.
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Simple
Harmonic
Motion
Investigating
a
Mass
Oscillating
on
a
Spring
DATA
AND
OBSERVATIONS
PART
I:
DETERMINING
THE
SPRING
CONSTANT
k
Data
Table
1
Run
#
|
Mass
on
Spring
|
Force
[Position
1
with
only|
Position
2
with
Amount
of
(kg)
N)
hanger
added
mass
stretch
(m)
(m)
(m)
1
2
3
4
5
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ANALYSIS
PART
I:
DETERMINING
THE
SPRING
CONSTANT
K
1.
On
the
mass
below,
draw
and
label
the
forces acting
on
the
mass
when
it
is
hanging
at
rest
on
the
end
of
the
spring.
I
2.
Using
either
graph paper
or
graphing
software,
construct
a
graph
of
Force
(N)
vs.
Amount
of
Stretch
(m).
Find
the
slope
of
this
graph.
a.
What
are
the
units
for
the
slope?
b.
The
equation
relating
the
magnitude
of
the
force
and
the
stretch
is
F
=
kx
.
How
does
this
equation
relate
to
the
slope
of
your
graph?
Force
vs
Stretch
-
Linear
Fit
For:
Data
Set:Force
y=
mx+b
/fl
m(Slope):
2.85
Nim
1.0
b(Y-Intercept):
0.117
N
/
Correlation:0.999
[l
(O]
S
p
i
<4
o
[F
0.5
/@/
1
1
I
I
T
L)
T
I
|
L)
L)
T
1
0.10
0.20
0.30
Stretch
¢
(m)
(0.247568,
0.662008)
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Data
Set
Streteh
(%)
Force
(m)
™
|
1
0.04400
0.29500
|
&
PEIEen
0.11500
0.44100
3
0.18500
0.63700
AN
0.25900
0.89300
5
0.32500
1,03000
.
4
||
PART
IlI:
ADDITIONAL
METHOD
FOR
FINDING
THE
SPRING
CONSTANT
K
1.
The
period
of
oscillation
for
your
mass
spring
system
can
be
calculated
using
the
following
equation.
Rearrange
this
equation
to
solve
for
the
spring
constant
k,
and
show
your
work
below.
For
each
of
your
five
Runs,
calculate
a
value
for
the
spring
constant
and
then
find
the
average
of
these
values.
Place
your
calculations
in
Table
2.
T=27r\/E
k
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i
1)
[
Mass
on
Spring
Time
for
10
Measured
Period
|
Calculated
value
for
Run
#
(kg)
oscillations
(s)
k
(s)
(N/m)
1
2
3
4
5
Avg.
n/a
n/a
n/a
2.
Compare
the
average
value
for
&
that
you
calculated
in
Part
II
to
the
value
you
found
for
& in
Part
I.
Find
a
relative
error
for
the
two
values.
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PART
III:
ENERGY
IN
SIMPLE
HARMONIC
MOTION
1.
For
this
oscillating
system,
the
energy
of
the
system
should
remain
constant
for
short
periods
of
time
involving
one
or
two
oscillations.
Over
time
friction
will
convert
some
of
the
energy
to
heat,
but
for
a
single
oscillation,
the
elastic
potential
energy
Us
of
the
system
at
maximum
amplitude
should
be
relatively
close
to
the
kinetic
energy
KE
when
the
system
returns
to
the
equilibrium
position.
Calculate
these
values
and
compare
them
by
finding
a
relative
error.
U,
=
L
T2
1
KE
=—mv
2
:
,
—
KE|
Relative
Error
=
x100
Table
3
Mass
on
|
Amplitude
Velocity
at
Calculated
[Calculated]
Relative
Run
#
Spring
|
of
stretch
[equilibrium
position
EPE
KE
Error
(kg)
(m)
(m/s)
Q)
@
(“e)
|
|WIN|—
2.
The
errors
in
this
part
of
the
lab
may
be
relatively
large.
Write
a
statement
analyzing
the
errors
in
this
lab
and
suggest
ways
that
the
errors
might
be
reduced.
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CONCLUSION
QUESTIONS
1.
A
person
who
weighs
670
N
steps
onto
a
spring
scale
in
the
bathroom,
and
the
spring
compresses
by
0.79
cm.
(a)
What
is
the
spring
constant?
Be
sure
to
specify
your
units.
(b)
What
is
the
weight
of
another
person
who
compresses
the
spring
by
0.34
cm?
2.
What
is
the
shape
of
the
plot
of
data
for
the
oscillating
spring-mass
system
on
your
graph?
Describe
the
shape
physically.
3.
In
terms
of
the
changes
in
force,
displacement,
acceleration,
and
energy,
describe
one
full
oscillation
of
a
mass
on
a
spring.
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4.
When
a
2.8-kg
object
is
suspended
from
a
spring,
the
length
increases
by
0.018
m.
If
the
frequency
of
vibration
is
f=
3.0
Hz,
how
much
mass
is
attached
to
this
spring?
5.
What
is
the
maximum
speed
of
the
mass
in
question
4?
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Physics
SITF
LAYING
THE
FOUNDATION
Building
Academic
Excellence
Waves
in
a
Spring
Observing
the
Characteristics
of
Waves
Purpose
In
this
activity,
you
will
observe
and
investigate
important
wave
properties.
What
you
observe
about
waves
in
a
spring
can
be
applied
to
other
types
of
waves
including
sound
waves,
water
waves,
and
light
waves.
Materials
Each
lab
group
will
need
the
following:
meter
stick
spring
(slinky)
stopwatch
spring,
6
ft
(snakey)
SAFETY
ALERT!
»
Coiled
springs
are
social
creatures.
Avoid
releasing
either
end
of
the
stretched
spring.
The
untangling
process
can
be
quite
difficult.
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©
2012
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Texas.
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reserved.
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Student
Activity
—
Waves
in
a
Spring
Procedure
Answer
the
questions
as
you
perform
this
activity.
You
and
your
lab
partner
should
hold
opposite
ends
of
a
spring
and
stretch
it
out
on
the
floor
to
an
appropriate
length.
Experiment
to
determine
the
best
stretch
distance
for
your
spring
but
be
careful
not
to
exceed
the
elastic
limit
of
the
material.
Data
and
Observations
Longitudinal
and
Transverse
Waves
1.
Pinch
a
clump
of
coils
together
with
your
free
hand
and
release
the
clump
of
coils.
Do
not
let
go
of
the
end
of
the
spring.
Observe
the
pulse
that
travels
back
and
forth
through
the
spring.
Why
is
it
called
a
longitudinal
pulse?
Sketch
the
wave
pulse
in
the
space
provided.
2.
Give
one end
of
the
spring
a
few
vigorous
sideways
(fransverse)
shakes.
How
is
this
wave
different
from
the
longitudinal
wave?
Sketch
the
wave
pulse
in
the
space
provided.
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2012
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Student
Activity
—
Waves
in
a
Spring
Data
and
Observations
(continued)
3.
The
stretched
spring
is
the
medium
through
which
the
pulse
travels.
Send
a
short
transverse
pulse
down
the
spring.
Observe
the
shape
of
the
pulse
as
it
moves
along
the
spring.
a.
How
does
the
shape
change? Can
you
suggest
a
reason
for
this
change?
b.
Upon
what
does
the
initial
amplitude
of
the
pulse
depend?
c.
Does
the
speed
of
the
pulse
appear
to
change
with
its
shape?
d.
Generate
single
pulses
of
various
(small,
medium,
and
large)
amplitudes.
Does
the
pulse
speed
appear
to
depend
on
the
size
of
the
pulse?
e.
What
could
you
do
to
produce
wave
pulses
that
travel faster
in
the
spring?
Can
this
be
done
by
shaking
the
spring
more
vigorously?
How
about
shaking
the
spring
faster?
Copyright
©
2012
Laying
the
Foundation®,
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Texas.
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reserved.
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Data
and
Observations
(continued)
Student
Activity
—
Waves
in
a
Spring
4.
Measure
the
length
of
a
stretched
spring
(do
not
change
this
length) and
the
travel
time
of
a
pulse
generated
at
one
end.
Use
a
stopwatch
to
time
how
long
a
wave
takes
to
travel
up
and
down
the
spring.
Calculate
the
speed
of
the
traveling
wave
pulse
for
pulse
sizes
that
are
small,
medium,
and
large.
Record
your
results
in
Table
1.
Is
the
speed
of
the
wave
pulse
affected
by
the
amplitude
of
the
pulse?
Use
your
data
and
d =
vt to
answer
this
question.
Transverse
Small
Transverse
Medium
Transverse
Large
Longitudinal
--
5.
Change
the
length
of
your
stretched
spring
and
determine
the
pulse
speed
as
you
did
previously.
Record
your
results
in
Table
2.
Examine
three
different
lengths
for
the
stretched
spring.
Is
the
speed
of
the
wave
pulse
affected
by
the
length
of
the
stretched
spring
(the
tension)?
Under
different
tensions,
does
the
stretched
spring
represent
the
same
or
different
media?
Table
2.
Spring
Length
Copyright
©
2012
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Student
Activity
—
Waves
in
a
Spring
Data
and
Observations
(continued)
Interference
6.
Have
your
lab
partner
generate
a
wave
pulse
toward
you
on
the
same
side
of
the
spring
that
you
send
a
pulse
toward
your
partner.
This
interaction
between
the
two
wave
pulses
is
called
interference.
a.
Describe
the
interference
of
the
two
wave
pulses.
How
does
the
pulse
amplitude
during
interference
compare
with
the
individual
amplitudes
before
and
after
this
interaction?
b.
Repeat
the
experiment
but
with
the
two
pulses
traveling
on
opposite
sides
of
the
spring.
Compare
the
interference
with
that
of
the
previous
interaction.
When
the
two
pulses
meet,
does
the
displacement
of
the
spring
at
that
instant
get
larger
or
smaller?
c.
Did
the
two
pulses
pass
through
each
other
or
bounce
off
each
other?
If
you
are
not
sure,
have
your
partner
send
a
transverse
wave
pulse
down
the
spring
at
the
same
time
you
send
a
longitudinal
wave
pulse.
What
can
you
say
about
the
interaction
of
these
two
wave
pulses?
Do
the
wave
pulses
bounce
off
each
other
or
do
they
pass
through
each
other?
d.
What
conclusions
can
you
draw
about
the
displacement
of
the
medium
at
a
point
where
two
pulses
interfere?
(This
is
called
the
principle
of
superposition.)
Copyright
©
2012
Laying
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Foundation®,
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reserved.
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Student
Activity
—
Waves
in
a
Spring
Data
and
Observations
(continued)
Reflection
7.
With
the
far
end
of
the
spring
held
firmly
in
place
by
your
lab
partner
(the
“fixed
end”),
send
a
single
pulse
down
one
side
of
the
spring.
Observe
the
reflected
pulse.
a.
Compare
the
amplitude
of
this
pulse
with
that
of
the
transmitted
pulse
just
before
reflection.
What
is
the
orientation
of
the
reflected
pulse
relative
to
the
transmitted
pulse?
b.
Attach
a
light
string
about
2
m
long
to
the
far
end
of
the
spring,
and
maintain
the
tension
on
the
spring
by
holding
the
end
of
this
string.
This
is
called
a
free-end
termination
for
the
spring.
Send
a
pulse
down
one
side
of
the
spring
as
before
and
observe
the
pulse
reflected
from
the
“free”
end.
Compare
the
reflected
pulse
from
the
“free”
end
of
the
spring
with
the
reflected
pulse
from
the
fixed
end.
Periodic
and
Standing
Waves
8.
By
moving
your
hand
steadily
back
and
forth,
you
can
produce
a
series
of
pulses
called
a
periodic
wave.
The
distance
between
any
two
adjacent
crests
or
troughs
on
a
periodic
wave
is
called
the
wavelength.
The
rate
at
which
you
move
your
hand
back
and
forth
determines
the
frequency.
Generate
a
periodic
wave
and
take
a
“snapshot”
of
the
wave.
Sketch
the
picture
on
the
axes
provided
in
Figure
1.
On
your
diagram,
show
the
amplitude
of
the
periodic
wave.
Sketch
one
wavelength
and,
using
the
total
distance
of
the
wave,
determine
the
value
for
this
wavelength.
How
does
the
wavelength
depend
on
the
frequency?
distance
displacement
o
Figure
1.
Periodic
wave
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Student
Activity
—
Waves
in
a
Spring
Data
and
Observations
(continued)
9.
Have
your
partner
generate
a
continuous
periodic
wave
while
you
try
and
match
it.
You
have
produced
a
standing
wave.
While
your
partner
holds
the
end
of
the
spring
steady,
you
will
form
transverse
standing
waves
having
first
one,
two,
three,
and
then
four
loops.
Find
the
frequency
needed
to
produce
each
standing
wave
pattern.
The
frequency
is
the
number
of
times
your
hand
moves
through
a
complete
cycle
(back
and
forth)
every
second.
It
will
be
easier
to
find
the
frequency
if
you
time
10
cycles
of
your
hand. After
you
find
the
frequency,
you
will
be
able
to
find
the
speed
of
the
waves
just
created
using
v
=
f4.
Table
3.
Standing
Waves
2
A=L
3
A=%x%xL
4
A=Y
xL
Record
your
results
in
Table
3,
where
L
is
the
distance
between
both
lab
partners
holding
either
end
of
the
spring.
a.
What
are the
loops
called?
b.
What
are the
places
called
where
the
spring does
not
appear
to
move?
c.
What
is
the
general
relationship
between
the
number
of
loops
and
the
frequency
of
the
wave?
Copyright
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2012
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reserved.
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Student
Activity
—
Waves
in
a
Spring
Analysis
1.
How
does
the
product
of
frequency
and
wavelength
(fA)
for
the
various
standing
wave
patterns
compare
with
one
another?
2.
How
do
these
values
compare
with
the
speeds
of
the
pulses
calculated
for
the
transverse
wave?
3.
How
are
the
speed,
frequency,
and
wavelength
of
a
transverse
wave
related
to
one
another?
4.
Consider
the
power
(number
of
joules
of
work
per
second)
you
are
expending
as
you
sweep
your
hand
back
and
forth
to
create
transverse
standing
waves.
Does
the
power
you
expend
to
create
waves
depend
on
the
frequency
of
the
waves?
5.
Does
the
power
required
depend
on
the
amplitude
of
the
wave?
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2012
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Student
Activity
—
Waves
in
a
Spring
Conclusion
Questions
1.
Suppose
a
flute
player
and
a
tuba
player
start
playing
at
the
same
time,
each
from
equally
far
away.
Which
instrument
will
you
hear
first?
Why?
2.
Which
travels
faster:
red
light
or
blue
light?
Blue
light
has
a
greater
frequency.
3.
For
the
waves
shown
in
Figure
2,
sketch
the
sum
of
the
two
waves.
a
?
d
e
b
|
I
0
c
-1
-2
=
=
4
3
2
1
0
-1
-2
Figure
2.
Sum
of
two
waves
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Student
Activity
—
Waves
in
a
Spring
Conclusion
Questions
(continued)
4.
What
happens
to
the
displacement
when
two
waves
meet
in
phase
(crest
on
crest)?
5.
What
happens
to
the
displacement
when
two
waves
meet
out
of
phase
(crest
on
trough)?
6.
What
happens
to
the
pulses
after
they pass
through
each
other?
7.
Explain
how
the
reflection
of
a
wave
from
a
rigid
barrier
(a
fixed
end)
and
a
less
rigid
barrier
(a
free
end)
affect
the
wave’s
phase.
8.
What
happens
to
the
speed,
wavelength,
and
frequency
of
a
wave
when
it
reaches
the
boundary
between
two
media?
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©
2012
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the
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inc.,
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reserved.
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Student
Activity
—
Waves
in
a
Spring
Conclusion
Questions
(continued)
9.
A
string
is
attached
to
a
vibrating
machine
that
has
a
frequency
of
120
Hz,
as
shown
in
Figure
3.
The
other
end
of
the
string
is
passed
over
a
pulley
of
negligible
mass
and
friction,
and
is
attached
to
a
weight
hanger
that
holds
a
mass
m
=
0.5
kg.
Figure
3.
Vibrating
machine
with
standing
wave
a.
Determine
the
tension
in
the
string.
b.
The
speed
of
the
wave
in
the
string
is
related
to
the
tension
by
the
equation
where
F_
is
the
tension
in
the
string
and
4
is
the
linear
density
of
the
string.
If
the
linear
density
of
this
string
is
0.05
kg/m,
determine
the
speed
of
the
wave
in
the
string.
c.
Determine
the
wavelength
of
the
wave
in
the
string.
d.
Determine
the
length
of
the
string
from
the
point
of
attachment
on
the
vibrating
machine
to
the
pulley.
e.
Would
you
need
to
increase
or
decrease
the
mass
on
the
hanger
to
produce
fewer
loops?
Explain.
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Explor#learning
................................................................................................................
Student
Exploration:
Orbital
Motion
—
Kepler’s
Laws
Vocabulary:
astronomical
unit,
eccentricity,
ellipse,
force,
gravity,
Kepler's
first
law,
Kepler's
second
law,
Kepler's
third
law,
orbit,
orbital
radius,
period,
vector,
velocity
Prior
Knowledge
Questions
(Do
these
BEFORE
using
the
Gizmo.)
1.
The
orbit
of
Halley’s
Comet,
shown
at
right,
has
an
oval
shape.
In
which
part
of
its
orbit
do
you
think
Halley’s
Comet
travels
fastest?
Slowest?
Mark
these
points
on
the
diagram
at
right.
2.
How
might
a
collision
between
Neptune
and
Halley’s
Comet
affect
Neptune’s
orbit?
Gizmo
Warm-up
The
path
of
each
planet
around
the
Sun
is
determined
by
two
factors:
its
current
velogity
(speed
and
direction)
and
the
force
of
gravity
on
the
planet.
You
can
manipulate
both
of
these
factors
as
you
investigate
planetary
orbits
in
the
Orbital
Motion
—
Kepler's
Laws
Gizmo™.
On
the
CONTROLS
pane
of
the
Gizmo,
turn
on
Show
trails
and
check
that
Show
vectors
is
on.
Click
Play
().
1.
What
is
the
shape
of
the
planet’s
orbit?
2.
Watch
the
orbit
over
time.
Does
the
orbit
ever
change,
or
is
it
stable?
3.
Click
Reset
((©)).
Drag
the
tip
of
the
purple
arrow
to
shorten
it
and
reduce
the
planet’s
initial
velocity.
Click
Play.
How
does
this
affect
the
shape
of
the
orbit?
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Activity
A:
Shape
of
orbits
Get
the
Gizmo
ready:
¢
Click
Reset.
e
Turn
on
Show
grid.
7~
-1T123
Introduction:
The
velocity
of
a
planet
is
represented
by
an
arrow
called
a
vector.
The
vector
is
described
by
two
components:
the
i
component
represents
east-west
speed
and
the
j
component
represents
north-south
speed.
The
unit
of
speed
is
kilometers
per
second
(km/s).
Question:
How
do
we
describe
the
shape
of
an
orbit?
1.
Sketch:
The
distance
unit
used
her
is
the
astronomical
unit
(AU),
equal
to
the
average
Earth-Sun
distance.
Place
the
planet
on
the
i
axis
at
r
=
-3.00i
AU.
Move
the
velocity
vector
so
that
v
=
-8.0j
km/s
(|v|
=
8.00
km/s).
The
resulting
vectors
should
look
like
the
vectors
in
the
image
at
right.
(Vectors
do
not
have
to
be
exact.)
Click
Play,
and
then
click
Pause
((CD)
after
one
revolution.
Sketch
the
resulting
orbit
on
the
grid.
[
N
w
&~
o
arta,=by+
b
i
=
el
LelbA-5C
W
2.
Identify:
The
shape
of
the
orbit
is
an
ellipse,
a
type
of
flattened
circle.
An
ellipse
has
a
center
(C)
and
two
points
called
foci
(F1
and
F,).
If
you
picked
any
point
on
the
ellipse,
the
sum
of
the
distances
to
the
foci
is
constant.
For
example,
in
the
ellipse
at
right:
Turn
on
Show
foci
and
center.
The
center
is
represented
by
a
red
dot,
and
the
foci
are
shown
by
two
blue
dots.
What
do
you
notice
about
the
position
of
the
Sun?
3.
Experiment:
Try
several
other
combinations
of
initial
position
and
velocity.
A.
What
do
you
notice
about
the
orbits?
B.
What
do
you
notice
about
the
position
of
the
Sun?
You
have
just
demonstrated
Keplér’s
first1aw,
one
of
three
laws
discovered
by
the
German
astronomer
Johannes
Kepler
(1571-1630).
Kepler's
first
law
states
that
planets
travel
around
the
Sun
in
elliptical
orbits
with
the
Sun
at
one
focus
of
the
ellipse.
(Activity
A
continued
on
next
page)
Wizmos
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Activity
A
(continued
from
previous
page)
4.
Observe:
Use
the
Gizmo
to
create
an
orbit
that
is
nearly
circular.
Then
create
an
orbit
that
is
flattened.
Observe
the
foci
in
each
ellipse.
A.
What
do
you
notice
about
the
spacing
of
the
foci
when
the
ellipse
is
very
round?
B.
What
do
you
notice
about
the
spacing
of
the
foci
when
the
ellipse
is
very
flat?
5.
Calculate:
The
eccentricity
of
an
ellipse
is
a
number
that
describes
the
flatness
of
the
ellipse.
Eccentricity
is
equal
to
the
distance
between
foci
divided
by
the
total
width
of
the
ellipse.
There
are
no
units
for
eccentricity.
Click
Reset.
Move
the
planet
to
r
=
—5.00i
AU
(does
not
have
to
be
exact)
and
drag
the
velocity
vector
to
set
the
velocity
close
to
—8.0j
km/s.
Click Play,
and
then
click
Pause
after
one
full
revolution.
A.
What
is
the
distance
between
the
foci?
B.
What
is
the
approximate
width
of
the
ellipse?
C.
What
is
the
eccentricity
of
the
ellipse?
D.
Click
Reset,
and
change
the
initial
velocity
to
—4.0j
km/s.
Click
Play.
What
is
the
eccentricity
of
this
ellipse?
Distance
between
foci:
Width:
Eccentricity:
6.
Draw
conclusions:
Think about
the
eccentricity
and
shape
of
each
ellipse.
A.
What
is
the
relationship
between
the
eccentricity
of
an
ellipse
and
its
shape?
B.
What
is
the
eccentricity
of
a
circle?
Explain.
C.
What
is
the
eccentricity
of
a
completely
flat
ellipse?
Explain.
The
eccentricity
of
Earth’s
orbit
is
0.17.
What
can
you
infer
about
the
shape
of
Earth’s
orbit?
@}izmos
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Activity
B:
Get
the
Gizmo
ready:
\"[
o
Velocity
and
area
P
ClcREse
Tl
2__,
3
y
e
Turn
off
Show
foci
and
center.
Introduction:
After
establishing
that
planetary
orbits
were
ellipses,
Kepler
next
looked
at
the
speed
of
a
planet
as
it
traveled
around
the
Sun.
Question:
How
does
the
velocity
of
a
planet
vary
as
it
travels
in
its
orbit?
1.
Observe:
Place
the
planet
at
—5.00i
AU
and
set
the
velocity
to
-4.0j
km/s
(does
not
have
to
be
exact).
Turn
off
Show
vectors.
Click Play.
Observe
the
speed
of
the
planet.
A.
At
what
point
does
the
planet
move
fastest?
B.
At
what
point
does
it
move
slowest?
2.
Observe:
Click
Reset,
and
turn
on
Show
vectors.
Look
at
the
green
vector
that
represents
the
force
of
gravity
pulling
on
the
planet.
Click
Play.
A.
In
which
direction
does
the
green
vector
always
point?
B.
In
which
part
of
the
orbit
does
the
gravity
vector
point
in
almost
the
same
direction
as
the
velocity
vector?
C.
In
which
part
of
the
orbit
does
the
gravity
vector
point
in
the
opposite
direction
as
the
velocity
vector?
3.
Explain:
Based
on
your
observations
of
the
gravity
vector,
why
does
the
planet
accelerate
as
it
approaches
the
Sun
and
slow
down
as
it
moves
away
from
the
Sun?
4.
Measure:
Click
Reset.
Imagine
a
line
connecting
the
planet
to
the
Sun.
As
the
planet
moves
around
the
Sun,
the
line
will
sweep
out
an
area.
Click
Play,
and
then
click
Sweep
area.
Record
the
area
below,
and
then
press
Sweep
area
four
more
times
to
complete
the
table.
Trial
1
2
3
4
5
Area
(km?)
(Activity
B
continued
on
next
page)
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Activity
B
(continued
from
previous
page)
5.
Analyze:
What
pattern
do
you
notice?
6.
Test:
Try
the
same
experiment
with
several
different
orbits
and
different
numbers
of
days
to
sweep
an
area.
Does
the
same
rule
hold
true
for
each
orhit?
Kepler’s
second
law
states
that
a
planet
accelerates
as
it
approaches
the
Sun
and
decelerates
as
it
moves
farther
from
the
Sun.
As
it
orbits,
the
planet
sweeps
out
equal
areas
in
equal
times.
7.
Think
and
discuss:
Why
do
you
think
the
area
swept
out
by
a
planet
in
a
given
period
of
time
remains
constant,
even
as
the
planet
speeds
up
and
slows
down?
(Hint:
Think
of
each
area
swept
out
as
a
triangle.
The
height
of
the
triangle
is
the
distance
between
the
planet
and
the
Sun,
while
the
base
of
the
triangle
is
equal
to
the
distance
the
planet
travels
in
the
given
time
period.)
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Get
the
Gizmo
ready:
&
AEHvIy
GE
e
Click
Reset.
A
Radius
and
period
e
Set
the
Sun
mass
to
medium,
close
to
the
mass
sl
e
of
our
Sun,
e
e
Introduction:
Kepler's
last
law
relates
the
period
(T)
of
a
planet,
or
the
time
it
takes
to
complete
an
orbit,
to
the
planet’s
orbital
radius
(a),
or
average
distance
from
the
Sun.
Question:
How
does
the
period
of
a
planet
relate
to
its
average
distance
from
the
Sun?
1.
Predict:
How
do
you
expect
the
period
of
a
planet
to
change
as
its
average
distance
from
the
Sun
increases?
2.
Measure:
Place
the
planet
at
-4.00i
AU
and
set
the
velocity
to
-15.00j
km/s
(does
not
have
to
be
exact).
Click
Play,
and
then
click
Pause
when
the
planet
completes
one
orbit.
A.
B.
What
is
the
approximate
period
of
the
planet
in
days?
Select
the
TABLE
tab
and
click
Record
data.
What
is
the
actual
period
(T)
of
the
planet
in
Earth
days
and
years?
days
years
What
is
the
orbital
radius
(a)
of
the
planet?
Click
Reset.
Place
the
planet
at
-2.00i
AU
and
set
the
velocity
to
-20.0j
km/s.
Click
Play
and
Record
data.
\What
is
the
period
now?
days
years
What
is
the
new
orbital
radius?
How
does
the
distance
between
the
planet
and
the
Sun
affect
its
period?
3.
Gather
data:
Experiment
with
the
Gizmo
to
create
a
series
of
larger
and
larger
orbits.
Record
each
orbit’s
radius
(a)
and
period
(7).
Leave
the
last
two
columns
blank
for
now.
Orbit
a
(AU)
T
(years)
1
alhlwWw|IN
(Activity
C
continued
on
next
page)
&}izmos
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Activity
C
(continued
from
previous
page)
4.
Analyze:
How
does
the
period
change
as
the
orbital
radius
increases?
5.
Interpret:
Select
the
GRAPH
tab,
and
check
that
the
graph
of
T
vs.
a
is
selected.
Use
the
zoom
controls
to
adjust
the
graph
so
you
can
see
all
your
data
and
it
fills
the
graph.
A.
What
does
the
graph
indicate?
B.
Does
the
graph
of
T
vs.
a
form
a
straight
line?
6.
Investigate:
Choose
other
options
in
the
dropdown
menus
until
you
find
a
graph
that
makes
a
perfectly
straight
line.
(If
you
cannot
see
your
data,
click
the
[@
controls
to
zoom
out.)
Which
relationship
makes
a
straight
line?
When
you
have
achieved
a
straight
line,
take
a
snapshot
of
the
graph
and paste
it
into
a
blank
document
you
will
turn
in
with
this
worksheet.
7.
Calculate:
On
the
table
on
the
previous
page,
label
the
third
column
“a®
and
the
fourth
column
“T2”
Use
a
calculator
to
cube
each
value
of
a
and
square
each
value
of
T.
What
do
you
notice?
Kepler’s
third
law
states
that
the
cube
of
a
planet’s
orbital
radius
is
proportional
to
the
square
of
a
planet’s
period:
a’
=
kT2
for
some
constant
k.
If
the
radius
is
measured
in
astronomical
units,
the
period
is
measured
in
Earth
years,
and
the
mass
of
the
star
is
equal
to
the
mass
of
our
Sun,
the
value
of
k
is
equal
to
1
AU%/y?.
8.
Challenge:
The
orbital
radii
of
the
planets
are
given
in
the
table
below.
Calculate
the
period
of
each
planet
(in
Earth
years),
and
then
check
your
values
with
your
teacher.
Planet
a
(AU)
T
(years)
Planet
a
(AU)
T
(years)
Mercury
0.39
Jupiter
5.20
Venus
0.72
Saturn
9.54
Earth
1.00
Uranus
19.18
Mars
1.52
Neptune
30.06
%}izmos
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Explorslearning
...............................................................................................................
Teacher
Guide:
Orbital
Motion
—
Kepler’s
Laws
fifé?
Learning
Objectives
Students
will
...
e
Observe
that
planetary
orbits
are
stable
(assuming
zero
friction).
¢
Understand
that
planets
travel
in
elliptical
orbits
with
the
Sun
at
one
focus.
o
Calculate
the
eccentricity
of
an
ellipse.
e
Explain
why
planets
accelerate
as
they
approach
the
Sun
and
decelerate
as
they
move
away
from
the
Sun.
¢
Discover
that
planets
sweep
out
equal
areas
in
equal
times.
e
Show
that
the
square
of
a
planet’s
period
is
proportional
to
the
cube
of
its
orbital
radius.
@‘)
Vocabulary
astronomical
unit,
eccentricity,
ellipse,
force,
gravity,
Kepler’s
first
law,
Kepler's
second
law,
Kepler's
third
law,
orbit,
orbital
radius,
period, vector,
velocity
fii%
Lesson
Overview
’
Several
decades
after
Nicholas
Copernicus
revived
the
heliocentric
(Sun-centered)
model
of
the
solar
system,
Johannes
Kepler
sought
to
determine
the
mathematical
laws
that
govern
planetary
motion.
His
painstaking
work
resulted
in
the
discovery
of
three
fundamental
laws
of
planetary
motion.
The
Orbital
Motion
—
Kepler's
Laws
Gizmo™
allows
students
to
model
planetary
orbits
and
discover
Kepler's
laws
for
themselves.
A
planet
orbits
a
star.
The
Student
Exploration
sheet
contains
three
activities:
e
Activity
A
—
Students
observe
that
planets
orbit
in
ellipses
with
the
Sun
at
one
focus.
e
Activity
B
—-
Students
discover
that
planets
sweep
out
equal
areas
in
equal
times.
e
Activity
C
—
Students
find
the
relationship
between
a
planet’s
orbital
radius
and
period.
Suggested
Lesson
Sequence
o
o
1.
Pre-Gizmo
activity:
Solar
System
Explorer
(€&
45
—
60
minutes)
Use
the
Solar
System
Explorer
Gizmo
to
introduce
students
to
the
geometry
of
planetary
orbits.
While
doing
the
Student
Exploration
sheet
for
this
Gizmo,
students
will
see
that
planetary
orbits
are
nearly,
but
not
exactly,
circular.
After
doing
the
Solar
System
Explorer
Gizmo,
have
your
students
practice
drawing
ellipses
and
calculating
their
eccentricity.
This
activity
is
described
in
the
Solar
System
Explorer
Teacher
Guide.
In
addition,
you
may
wish
to
discuss
the
historical
background
to
Kepler’s
laws
of
planetary
motion.
(See
the
Scientific
Background
for
details.)
Explain
the
influence
of
Nicholas
Copernicus,
Tycho
Brahe,
and
others
on
Kepler's
work.
wizmos
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2.
Prior
to
using
the
Gizmo
(68
10
—
15
minutes)
Before
students
are
at
the
computers,
pass
out the
Student
Exploration
sheets
and
ask
students
to
complete
the
Prior
Knowledge
Questions.
Discuss
student
answers
as
a
class,
but
do
not
provide
correct
answers
at
this
point.
Afterwards,
if
possible,
use
a
projector
to
introduce
the
Gizmo
and
demonstrate
its
basic
operations.
Demonstrate
how
to
take
a
screenshot
and paste
the
image
into
a
blank
document.
3.
Gizmo
activities
(€&
15
—
20
minutes
per
activity)
Assign
students
to
computers.
Students
can
work
individually
or
in
small
groups. Ask
students
to
work
through
the
activities
in
the
Student
Exploration
using
the
Gizmo.
Alternatively,
you can
use
a
projector
and
do
the
Exploration
as
a
teacher-led
activity.
4.
Discussion
questions
(&8
15
—
30
minutes)
As
students
are
working
or
just
after
they
are
done,
discuss
the
following
questions:
¢
What
would
happen
if
a
planet
were
hit
by
a
large
object
that
slowed
it
down?
Would
it
have
a
different
orbit
or
would
it
spiral
into
the
Sun?
[As
long
as
the
planet
didn’t
directly
hit
the
Sun,
it
would
go
into
a
different
stable
orbit.]
e
What
would
happen
to
an
orbit
of
a
planet
if
it
were
traveling
through
a
medium
that
caused
the
planet
to
gradually
slow
down?
[The
planet
would
spiral
into
the
Sun.
This
doesn’t
happen
in
our
solar
system
because
there
is
no
friction
in
empty
space.]
¢
In
which
direction
does
the
gravity
vector
always
point?
e
Try
to
create
a
series
of
orbits
that
are
nearly
circular.
How
does
the
speed
of
the
planet
relate
to
its
distance
from
the
Sun?
Why
is
this
true?
[The
closer
the
planet
is
to
the
Sun,
the
faster
it
must
go
to
maintain
a
nearly
circular
orbit.]
e
How
does
the
mass
of
the
Sun
affect
the
speed
of
a
planet
in
orbit?
¢
If
the
Sun
mass
and
Planet
mass
are
set
to
medium,
can
you
create
an
orbit
that
has
an
orbital
radius
closeto
1
AU?
What
is
the
period
of
this
orbit?
[This
orbit
is
similar
to
Earth’s
orbit
and
has
a
period
close
to
1
Earth
year.]
e
As
a
planet
orbits
the
Sun,
does
the
Sun
move?
[To
investigate
this
question,
have
students
set
the
Sun
mass
to
small,
the
Planet
mass
to
large,
and
click
Play.
Students
can
then
zoom
in
on
the
Sun
as
much
as
possible
to
see
its
motion,
which
is
an
ellipse
that
has
the
same
shape
as
the
planet’s
orbit.]
5.
Follow-up
activity:
Swinging
milk
carton
(82
10
—
20
minutes)
Planets
orbit
stars
because
of
the
force
of
gravity
acting
on
the
planet.
At
the
same
time,
the
planet
exerts
an
equal
force
on
the
star.
To
model
these
forces,
tie
a
rope
securely
around
the
handle
of
a
1-gallon
milk
carton.
Choose
an
outdoor
location
with
plenty
of
open
space.
Students
can
take
turns
whirling
the
heavy
container
around
their
bodies.
Students
will
feel
the
strong
pull
of
the
milk
carton
on
their
arms.
They
will
also
discover
that
as
the
speed
of
the
milk
carton
increases,
the
force
required
to
hold
on
to
the
carton
increases
as
well.
Experiment
with
different
lengths
of
rope
and
compare
the
speed
of
the
orbiting
milk
carton
with
different
orbital
radii.
Point
out
that
once
the
carton
is
orbiting,
the
orbit
can
be
maintained
with
only
an
inward
pull,
just
as
gravity
pulls
the
planet
toward
the
Sun.
@;izmos
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Scientific
Background
Johannes
Kepler
(1571-1630)
was
a
transitional
figure
in
the
development
of
modern
astronomy.
On
one
hand,
Kepler
was
a
theologian
and
astrologer
whose
motivation
for
studying
the
stars
was
to
illuminate
God’s
plan
for
the
universe.
But
Kepler
was
also
a
pioneer
of
using
mathematics
to
analyze
and
find
patterns
in
quantitative
data.
Although
Kepler’'s
laws
were
a
key
step
in
the
development
of
modern
science,
he
never
abandoned
his
mystical
idea
that
the
spacing
of
planetary
orbits
was
determined
by
the
nesting
of
geometric
solids,
illustrated
at
right.
Kepler's
big
break
came
in
1600,
when
he
was
invited
to
work
for
the
Danish
astronomer
Tycho
Brahe.
Kepler
spent
years
analyzing
Tycho’s
data
to
determine
the
exact
shape
of
the
orbit
of
Mars.
After
unsuccessfully
applying
a
variety
of
geometric
shapes
to
the
orbit,
Kepler
eventually
discovered
that
an
elliptical
model
with
the
Sun
at
one
focus
matched
observations
perfectly.
Subsequent
analysis
confirmed
that
all
planetary
orbits
are
elliptical.
This
is
Kepler’s
first
law.
While
analyzing
the
orbit
of
Mars,
Kepler
observed
that
planets
travel
faster
when
closer
to
the
Sun
and
more
slowly
when
farther
from
the
Sun.
Kepler
then
discovered
a
remarkable
relationship:
A
line
joining
a
planet
to
the
Sun
sweeps
out
equal
areas
in
equal
times.
In
the
diagram
at
left,
both
pink
wedges
were
swept
out
in
the
same
time
period
and
are
equal
in
area.
This
is
Kepler's
second
law.
Kepler's
third
law
was
discovered
later,
in
1619.
Throughout
his
life,
Kepler
was
obsessed
by
the
“harmonies”
that
ruled
the
universe.
Kepler
was
convinced
that
there
was
a
harmonious
relationship
between
the
period
of
a
planet
(T)
and
its
average
orbital
radius
(a).
After
much
trial
and
error,
Kepler
discovered
that
the
square
of
the
period
is
proportional
to
the
cube
of
the
radius.
If
the
period
is
measured
in
Earth
years
and
the
orbital
radius
is
measured
in
astronomical
units
(AU),
the
two
values
are
nearly
equal:
72
=
a°.
Although
Kepler
did
not
understand
the
causes
of
planetary
motions,
his
work
inspired
Isaac
Newton.
Newton’s
Philosophiae
Naturalis
Principia
Mathematica,
published
in
1687,
demonstrated
that
all
of
Kepler's
laws
arise
from
the
law
of
universal
gravitation.
Selected
Web
Resources
Planetary
motion:
http://farside.ph.utexas.edu/teaching/336k/Newton/node45.html
Drawing
ellipses
activity:
http://www.sciencebyjones.com/ellipse
lab.htm
Kepler's
laws:
http://csep10.phys.utk.edu/astr161/lect/history/kepler.html,
http://www.physicsclassroom.com/class/circles/u6l4a.cfm,
http://www.mathacademy.com/pr/prime/articles/kepler/index.asp
Kepler
biography:
http://www-groups.dcs.st-and.ac.uk/~history/Biographies/Kepler.html
Related
Gizmos:
Solar
System
Explorer.
http://www.explorelearning.com/gizmo/id?441
Solar
System:
http://www.explorelearning.com/gizmo/id?636
Gravity
Pitch:
http://www.explorelearning.com/gizmo/id?648
Gravitational
Force:
http://www.explorelearning.com/gizmo/id?411
%}izmos
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