LAB #3
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University of Southern Mississippi *
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Course
111
Subject
Astronomy
Date
Dec 6, 2023
Type
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10
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AST 111: Lab #3
Relative Motions of the Earth-Moon-Sun System: Part 2
(Phases of the Moon)
Objectives
•
To kinesthetically investigate the causes of the phases of the Moon
•
To construct a lunar phase diagram
•
To determine when a lunar phase will occur
•
To determine the times on Earth that a lunar phase will occur
•
To understand the scale of the Earth-Moon system
Materials
•
Table-top planetarium
•
Ruler
•
Softball
•
Ping-Pong ball
•
Flashlight
References
•
None
Introduction
As seen elsewhere, the relative positions and motions of the Earth, Moon,
and Sun give rise to our most common everyday units of time, the day and the
month. But they also are important for understanding the phases of the Moon,
eclipses of the Moon and Sun, the seasons and even climatic changes on the
Earth. The purpose of this lab and the next will be to improve our understanding
of how these phenomena are determined by these relative motions.
As we have seen in a previous lab, the Moon’s orbit can be separated into
two types: the sidereal (i.e. with respect to the stars) and the synodic (i.e. with
respect to the Sun). The Moon’s sidereal period
–
about 27 1/3 days long
–
can
be said to be its “real” orbital period, but the synodic period –
about 29 ½ days
long
–
is the period people pay attention to, because it shows the cycle of the
phases of the Moon. Here we will examine in detail the characteristics of the
lunar phases.
24
Activity #1: The Phases of the Moon
–
Part 1
The Moon is the second-brightest natural object in the sky, following of
course the Sun. The Sun gives off light of its own accord, and therefore always
appears as a bright disk. In contrast, the Moon merely reflects light.
1
The
appearance of the Moon therefore depends not only on the side of the Moon
facing the Sun, but also on the amount of the sun-lit side of the Moon facing the
Earth. The specific appearance of the Moon is called a
phase
.
We will begin our investigation of lunar phases by walking through the
orbit of the Moon about the Earth, in conjunction with a short discussion using a
lighted planetarium with models of the Earth and Moon.
(a) The instructor will ask three students to act as the Sun, the Earth, and
the Moon:
(i)
The first student will represent the Sun by holding a bright
flashlight at one end of the room. The room will be darkened
in order to emphasize the effects.
(ii)
A second student will represent the Earth by holding a small
sphere, such as a softball. The model Earth should be held
in a place so that a model Moon can freely orbit the model
Earth.
(iii)
A third student will represent the Moon by holding a smaller
sphere, such as a Ping-Pong ball. The student will have to
hold the model Moon in such a way that the other students in
the classroom will be able to see it. Also, the student will
have to hold the model Moon slightly higher than the model
Earth so that their shadows do not hit each other (we will
learn why in a future lab).
(b) The model Sun, Earth and Moon should be held first in a manner as
shown by Figure 3-1a on the following page. Also refer to Figure 3-1b
for a close-up of the Earth and Moon. In all figures, we view the system
from above the Earth’s North Pole. Neither figure is to scale.
(c) Note which side of the Moon (and Earth) is lit by sunlight and which
side is in darkness. Use a pencil or pen to shade the dark sides of the
Moon and Earth in Figure 3-1b.
1
Oddly enough, even though the full Moon is capable of casting shadows at night, only six percent of the
sunlight hitting the Moon is reflected back to space. The percentage of light reflected is called
albedo
and
depends primarily on the composition of the surface.
25
Figure 3-1a. A
Model of the “New” Phase of the Moon (not to scale).
Figure 3-1b. A Close-
Up of the “New” Phase of the Moon (not to scale).
(d) From this orientation, which side (left or right) of the Moon is in
sunlight? Which side is in darkness?
(e) Similarly for the Earth, which side (left or right) is in sunlight? Which
side is in darkness?
(f) In order for the Moon to be in your sky for this phase, on which side of
the Earth must you be? Will that side be experiencing day or night?
Light from the
Sun (Flashlight)
The Moon
The Earth
Incoming Sunlight
The Moon
The Earth
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26
(g) Which side of the Moon is facing the Earth, the light or dark side?
(h) Given this particular set of relative positions of the Sun, Earth, and
Moon, how much of the lit Moon do you expect to see in this phase?
(i) Now we will take a look at the opposite case or phase. Hold the model
Sun, Earth and Moon in the manner shown by Figure 3-2a on the
following page. Also refer to Figure 3-2b for a close-up of the Earth and
Moon. Again, neither figure is to scale.
(j) Note which side of the Moon (and Earth) is lit by sunlight and which
side is in darkness. Use a pencil or pen to shade the dark sides of the
Moon and Earth in Figure 3-2b.
(k) From this orientation, which side (left or right) of the Moon is in
sunlight? Which side is in darkness?
(l) Similarly for the Earth, which side (left or right) is in sunlight? Which
side is in darkness?
(m) In order for the Moon to be in your sky for this phase, on which side of
the Earth must you be? Will that side be experiencing day or night?
(n) Which side of the Moon is facing the Earth, the light or dark side?
(o) Given this particular set of relative positions of the Sun, Earth, and
Moon, how much of the lit Moon do you expect to see in this phase?
27
Figure 3-
2a. A Model of the “Full” Phase of the Moon (not to scale).
Figure 3-2b. A Close-
Up of the “Full” Phase of the Moon (not to scale).
Activity #2: The Phases of the Moon
–
Part 2
It is relatively easy to visualize the appearance (phase) of the Moon when
it is aligned with the Earth and the Sun. It is harder when the Moon is not so
aligned. First we will consider the phase of the Moon when it is at a right angle to
the Earth and Sun.
(a) Now hold the model Sun, Earth and Moon in the manner shown by
Figure 3-3a on the following page. Refer to Figure 3-3b for a close-up
of the Earth and Moon. Neither figure is to scale.
(b) Note which side of the Moon (and Earth) is lit by sunlight and which
side is in darkness. Use a pencil or pen to shade the dark sides of the
Moon and Earth in Figure 3-3b.
Light from the
Sun (Flashlight)
The Moon
The Earth
Incoming Sunlight
The Moon
The Earth
28
Figure 3-
3a. A Model of a “Quarter” Phase of the Moon (not to scale).
Figure 3-3b. A Close-
Up of a “Quarter” Phase of the Moon (not to scale).
(c) On which side of the Earth (left, right, upper, lower) do you need to be
for the Moon to be in your sky?
(d) How much of the entire side of the Moon is visible from the Earth?
(e) How much of the entire Moon is visible from the Earth? Hint: it is not
the same answer as question (d) above.
Light from the
Sun (Flashlight)
The Moon
Incoming Sunlight
The Moon
The Earth
The Earth
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29
(f) What is the range of time on the side of the Earth that has the Moon in
its sky? Is this the same as the range of time that the Moon can be
seen from the Earth? If not, why not? Hint: the Earth rotates
counterclockwise in these figures.
(g) How far has the Moon moved in its orbit (in terms of fractions) about
the Earth from New to Quarter? Hint: the Moon orbits the Earth
counterclockwise in these figures.
Next we will construct a lunar phase diagram. This diagram allows us to
determine the characteristics of any lunar phase.
Figure 3-4 shows the Earth at the center with sunlight approaching from
one direction. The eight smaller circles represent various positions of the Moon in
its orbit about the Earth. All motions (the Earth’s rotation and the Moon’s orbit)
are counterclockwise and we are looking down on the Earth’s North Pole.
(h) Shade in the dark sides of each Moon in Figure 3-4 (i.e. the lunar
phase diagram). Also shade in the dark side of the Earth.
(i) The Earth has four triangles, representing specific times of the day
–
noon, 6 pm, midnight, and 6 am. Identify which triangle corresponds to
which time on Earth and write the answer in the boxes near each
triangle on Figure 3-4.
(j) For each numbered Moon, write the name of its phase in Table 3-1. A
“crescent” moon shows a sliver of moon, while a “gibbous”
2
moon
shows most, but not all, of the lit moon facing us.
(k) What do
you think the terms “waxing” and “waning” mean for lunar
phases?
(l) For each phase, determine the time each moon rises, the time each
moon passes the meridian and the time each moon sets. Record the
results in Table 3-1.
(m) For each phase, determine whether the Sun lights the eastern or the
western side of the Moon. Record the results in Table 3-1.
2
The term “gibbous” means “humpback”, which may help to remember its shape.
30
Table 3-1. Characteristics of the Lunar Phases
1
New
Noon
Far
Phase
of
Moon
#
Moon
Rises
at…
Moon on
meridian
at…
Moon
Sets
at…
Side of
Moon lit
by Sun
Appearance
of the Moon
from the Earth
2
3
4
5
6
7
8
Waxing
Gibbous
Third
(or last)
Quarter
Waning
Crescent
Noon
6 p.m.
Midnight
West
9 p.m.
6 p.m.
Near
East
Noon
9 a.m.
31
Incoming sunlight
Figure 3-4. A Lunar Phases Diagram.
1
2
3
8
7
5
6
4
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(n) For each phase, sketch the appearance of the Moon as seen from
Earth in Table 3-1. Sketch the amount of Moon lit by sunlight (a few
examples have already been drawn).
(o) The orbit of the Moon about the Earth is 29.5 days long. About how
long does each of these eight phases last?
(p)
If the Moon’s phases are waxing, does the Sun light the e
astern or
western side of the Moon? What if the Moon’s phases are waning?
(q)
Does it make sense to talk about a “dark” side of the Moon? Is that the
same as the far side of the Moon?
(r) Suppose the Moon rises at 3 p.m. What is its phase?
(s) The eastern half of the Moon is lit with sunlight. What is its phase?
(t) Which do you expect to be noticed by more people, a first quarter
phase or a third (last) quarter phase? Why?
(u) Is it possible for other natural objects to show phases? If so, list at
least three of them.