13.
D uring
t he
f all,
w hich
6
b right
c onstellations
a re
v isible
f rom
C hicago?
C an
y ou
identify
t he
b right
s tars
P olaris,
D eneb,
A ltair
a nd
V ega?
W hich
a re
i ncluded
i n
t he
summer
t riangle?
14.
C an
y ou
d escribe
t he
i mportance
o f
G alileo’s
t wo
p ublications
l isted
b elow?
a.
T he
S tarry
M essenger
b.
D ialogue
o n
t he
T wo
G reat
W orld
S ystems
15.
C an
y ou
e xplain
P tolemy’s
g eocentric
m odel
o f
t he
U niverse?
16.
C an
y ou
e xplain
w hy
T ycho
B rahe
i s
s till
k nown
t oday
f or
h is
o bservational
d ata
and
h is
h iring
o f
J ohannes
K epler?
17.
C an
y ou
i dentify
w hich
o f
t he
f ollowing
d escriptions
g o
w ith
w hich
o f
K epler’s
3
laws
o f
p lanetary
m otion?
a.
T his
l aw
i s
a bout
t he
s peed
o f
p lanet
t raveling
a round
t he
s un.
A s
a
p lanet
orbits
t he
s un,
t he
l ine
j oining
t he
S un
a nd
t he
p lanet
s weeps
t hrough
e qual
areas
i n
e qual
t imes.
b.
T his
l aw
i s
a bout
t he
l ength
o f
t ime
a
p lanet
t akes
t o
o rbit
t he
S un
( period
of
r evolution).
I f
y ou
u se
t he
u nit
A U
( Astronomical
U nit)
t o
m easure
t he
average
d istance
o f
t he
p lanet
f rom
t he
s un,
K epler’s
e quation
a ppears
i n
i ts
simplest
f orm:
P 2
=
R 3
w here
P
=
p eriod
o f
r evolution
a nd
R
=
a verage
distance
o f
p lanet
f rom
s un
( semimajor
a xis)
c.
P lanets
o rbit
t he
S un
i n
e llipses