SlideShare a Scribd company logo
1 of 12
Download to read offline
Teacher’s Guide




© Leslie Evans
Bob Crelin • Illustrated by Leslie Evans



                                   Teacher’s Guide
                                          Northern Hemisphere edition
                                                  Bob Crelin
                  © Leslie Evans                                                            © Leslie Evans




UNDERSTANDING THE PHASES OF THE MOON
A fun, four-stage classroom unit for understanding the Moon’s phases (2–3 class periods)

Objectives
Students will be able to do the following:
1) Model how the relationship of our Earth, Moon, and Sun creates moon phases.
2) Chart the sequence and names of the eight primary Moon phases.
3) Identify each Moon phase by its appearance.
4) Identify the Moon’s position in orbit during each primary phase.

Materials you will need:
• Copy of the book Faces of the Moon by Bob Crelin (Charlesbridge)
• Room that can be darkened, with enough open floor space to fit students standing in a circle
• Bare light bulb on a stand (example: a floor lamp with shade removed)
• Earth globe
• Extension cord
• Moon Orbit Spin Chart (included)
• Paper fastener

Each student will need:
• Pencil or pen
• 2"–4" (5–10 cm) Styrofoam ball mounted on a Popsicle stick (suppliers: craft/art supply store)
• Moon Phase Chart (included)
• Strip of eight Phase Squares (included)
• Scissors
• Glue stick

NOTE: Before starting this unit, make paper photocopies of the Moon Phase Chart and the Phase
Squares. Cut the Phase Squares into strips of the eight lunar phases. Photocopy the Moon Orbit
Spin Chart on heavier card stock paper and assemble using a paper fastener.

                                                      1
Advanced preparation
The introduction (Stage 1) is brief and a prelude to the hands-on classroom activity (Stage 2).
Making the following preparations before starting will allow the students to move easily between
the steps while retaining concepts and terminology.

For best results, choose a room that can be made completely dark when the lights are turned
off (dark window coverings can help) Clear the floor space of obstacles and place a tall lamp
with bare bulb (the brighter, the better) in the center of the room. Use an extension cord if
necessary. Covering or taping down the lamp/extension cord will help to prevent students from
tripping on it. For the hands-on demonstration, make sure that there is plenty of space for the
students to stand and form a circle (with elbow room) around the lamp (see Figure 1 on page
3). Desks are not required. Students can sit on the floor during the introduction (Stage 1) and
while constructing their charts (Stage 3). Have materials, including photocopies of the Moon
Phase Chart and Phase Square strips, ready to hand out to students.




               Stage 1 • Introduction

               (run time: approximately 5–10 minutes)
               In storytelling fashion, students sit, listen, and look as the basic concepts and
               terms used throughout the lesson are introduced.


Concept: The Moon cycle
Read aloud the first two verses on pages 2–3 of Faces of the Moon:
"Do you wonder, when you see the Moon..."
Explain that the word "month" comes from “Moon.” Long ago, a month represented the time it
took to complete one cycle of the changing Moon phases (approximately 29.5 days). Today, we
call this a "lunar month," compared to our modern "calendar month."


Concept: Moon phases as light and shadow
Read aloud the next two verses on pages 4–5:
"Each changing face (or lunar phase)..."
Explain that we are able to see the Moon from Earth because the Sun’s light shines on it. The
sunlit part of the Moon makes the phase, or shape, of the Moon that we see (the rest of the Moon
is in shadow).


Concept: Earth’s relationship to the Moon and Sun
Read aloud the next two verses on pages 6–7:
"For as she orbits Earth in space,"
Explain that the sunlit part of the Moon changes because we are watching from the surface of
Earth as the Moon moves in orbit around our planet. The changing Moon phases have been
given names that describe their appearance, and their place in the phase cycle.
                                               2
Stage 2 • Modeling the Phasing Moon
             (run time: approximately 20–30 minutes)
             After a brief explanation of the activity, students participate by following the step-
             by-step directions of the instructor, and by learning about each phase from the
             book.

Explain to the class that by building a model of the Moon’s orbit, we can demonstrate why we
see the changing phases of the Moon.

To make a model of the Moon phases, we will need three "players" from our solar system.
Ask students to identify who these players are. (Answer: Moon, Sun, and Earth)
Show the items that represent each player:
• The Styrofoam ball on the Popsicle stick for the Moon
• The light bulb on the stand for the Sun
• The globe for Earth (for now)

Briefly review (and demonstrate) with students the basic orbital motions of these players:
• Earth orbits around the Sun.
• The Moon orbits around Earth.
It helps to visually demonstrate these motions by walking the globe (Earth) in a counterclock-
wise “orbit” around the light bulb (Sun), while circling the Styrofoam ball (Moon) counterclock-
wise around the globe.




Figure 1




The Hands-on Activity*       *Elements of this exercise are based on an Astro-Adventures learning activity, Dennis Schatz and Doug Cooper • pacsci.org



Turn on the light bulb “Sun” in the center of the room. Turn off all other room lights.
For safety, remind students not to touch the hot light bulb.
Have each student get a Styrofoam Moon ball on a stick. Have the students stand and form a
circle around the light bulb Sun (see Figure 1). Tip: Students should leave elbow room between
themselves for easier movement during the demonstration.

Explain that the globe will not represent Earth in the activity, because as we learned earlier, we
watch the Moon phases change from Earth’s surface. Instead, each student’s head will represent
Earth for the demonstration. Because their eyes are set in their head, they can watch the changing
appearance of the Moon from their “Earth.”


                                                              3
Stage 2 • Modeling the Phasing Moon, continued
                                                                   Figure 2
Have the students place their hand on their left shoulder.                                Moon
                                                                       Earth
This represents their “eastern” side. Explain that, during the                                                    Sun

demonstration, they will turn towards the east, or left, side to
simulate the Moon’s counterclockwise orbital motion around
Earth (see Figure 2).

Explain to the students that they will demonstrate the Moon’s
orbit in step-by-step movements, following your direction.
                                                                                                            eft
                                                                                             a rd s   the l
                                                                               ro tat e to w

Introduce the assembled Moon Orbit Spin Chart (Figure 3)
to the students. Point out the parts of the chart that represent
their head, their Styrofoam Moon ball, and the light bulb Sun.      Figure 3
Show how the orbit circle has eight numbered stops that
represent the eight primary Moon phases. When modeling
the “orbit,” students will pause together at each stop (see
Figure 4 on page 6). At each stop, they will observe the
appearance of their Moon ball, and listen to a rhyme that
names and describes this Moon phase.

Show the students the Orbit Spin Chart dial set at stop #1
(as shown in Figure 3). Ask them to position themselves and
their Moon as shown on the chart. Each student should hold
their Moon out in front of their head and face the light bulb
Sun.



       Stop #1 - New Moon
Remind students that it is the Sun’s light shining on the Moon that shows us the phase we see.
Ask them how much sunlight they see on their Moon in position #1. They should see no sunlight,
because the shadowed side of the Moon is facing their “Earth” (their head). Ask if anyone knows
what phase this is. (Answer: New Moon)
Read aloud page 8 of Faces of the Moon (stanza describing this New Moon phase):
"The Moon's first phase, we call it NEW..."
After reading the New Moon stanza, have the class say, "New Moon" together.

       Stop #2 - Waxing Crescent
Explain that, together, the students will now begin to rotate, stopping at each phase around the
Moon's orbit. Hold the Orbit Spin Chart up for all to see, and move the dial from stop #1 (New
Moon) to stop #2 (Waxing Crescent). Ask the students to turn to the east (left) as shown on the
chart. Once students are in the correct position, ask them to look at their Moon ball to notice
the sunlight illuminating the right edge of it.



                                                  4
Stage 2 • Modeling the Phasing Moon, continued

Page 11 of the book shows a die-cut illustration of the Waxing Crescent Moon. Have students
compare this illustration to the sunlit crescent on their own Moon ball. Read aloud page 10
(stanza describing the Waxing Crescent phase): "A few days pass, and Moon's less shy..." Have
the class say, "Waxing Crescent" together.

The term “Waxing”
This is a good point in the lesson to associate the term "waxing" with the apparent growth of
the Moon. A great comparison is the old practice of “candle dipping,” in which each dip of a
candle wick in hot wax would make the candle grow thicker. The growing Moon can be seen
as "waxing," like the candle.


        Stop #3 - First Quarter
Next, move the chart dial to stop #3. Ask the students to rotate to this position. They should
notice that the sunlight has “grown” to fill the right half of their Moon ball. Compare the Moon
ball with the illustration of the First Quarter Moon on page 13 of the book. Read aloud page 12:
"We notice Moon's FIRST QUARTER phase..." The class says, "First Quarter" together.

       Stop #4 - Waxing Gibbous
Continue to stop #4 on the Orbit Spin Chart. The students move accordingly and notice the
increasing sunlight on the right side of their Moon ball. Show the Waxing Gibbous illustration
on page 15 and read page 14: "Once she's past First Quarter Moon,..." The class says, "Waxing
Gibbous" together.

        Stop #5 - Full Moon
Move to stop #5. Make sure that students hold their Moon ball a little above their head in this
position so as not to cast a shadow on the ball. If positioned correctly, they should see a Full
Moon, without shadow. Pages 17 and 18 portray the Full Moon, and pages 16 and 19 describe
it: "Next comes Moon's most famous phase..." The class says, "Full Moon" together.

       Stop #6 - Waning Gibbous
Mention that the Moon has now “waxed” full of sunlight. As students continue on to stop #6 in
the orbit, they should notice how the sunlight begins to decrease, or "wane" on their Moon ball.
A shadow now begins to “grow” on the Moon's right side, as shown in the illustration on page
20. Read aloud page 21: "Once past Full, the shadows start..." The class says, "Waning Gibbous"
together.

       Stop #7 - Last Quarter
Continue to stop #7. The students move and notice that the sunlit part has decreased. Their
Moon ball is now lit on the left half. Show the Last Quarter illustration on page 22 and read page
23: "At Moon's LAST QUARTER of her trip,..." The class says, "Last Quarter" together.


        Stop #8 - Waning Crescent
Move the chart dial to stop #8. The students move and compare the crescent of sunlight on their
Moon ball to the illustration on page 24. Read page 25 aloud: "From early dawn to morning
blue,..." The class says, "Waning Crescent" together.

                                                5
Stage 2 • Modeling the Phasing Moon, continued

Then move the chart dial–and ask the students to rotate–back to STOP #1, where they began
their orbit. Read page 27 aloud: "Then Moon returns where she'd begun..." Ask the students
to tell you all together the name of this phase (New Moon). Remind them that they have just
modeled one complete Moon orbit around our Earth. This represents the 29.5-day “lunar month.”

To support this visual demonstration of the changing phases, have the students now do an
additional complete rotation (in the same direction), turning slowly without stopping this time. Ask
them to watch the changing pattern of light and shadow on their Moon ball as they go. Remind
them to keep their Moon ball a little above their head to prevent a “head-shadow lunar eclipse”
at the Full Moon position.
                                          STOP #1
Figure 4                          She sees only the
                              Moon’s shadowed side:
                                       NEW MOON




                                               STOP #3
                               She sees the right half of
                                  her Moon in sunlight:
                                     FIRST QUARTER




                                                  STOP #6
                            She sees the shadow forming
                            on the right side of her Moon:
                                      WANING GIBBOUS




                                                    6
Stage 3 • Recording Our Observations

              (run time: approximately 20–30 minutes)
              Students create their own charts to record what they’ve learned from the hands-
              on Moon phase activity.

Students can move to their desks, or to a clear spot on the floor, to assemble their Moon charts.
Each student will need a pencil or pen, a copy of the Moon Phase Chart, a strip of the eight
Phase Squares, a pair of scissors, and a glue stick.




Show the students how the Moon Phase Chart is modeled after the Orbit Spin Chart used during
the demonstration, with the Sun, Earth and Moon in the same relative positions. Once assembled,
the chart will show and name the pattern of Moon phases throughout a lunar month. For best
results and participation, ask the students to follow the steps together as a class. A simple
mistake, like a reversed Phase Square, can throw off the rest of the phase pattern.

First, ask students to separate the eight Phase Squares by cutting them apart along the white
lines. Before cutting, many students will notice that the phases on the strip are out of sequence.

Next, ask students to find the box marked #1 on their Moon Phase Chart. Remind students that
this is where they began the Moon’s orbit in the demonstration. Ask if someone can identify the
phase they saw when the Moon ball was in this position, between Earth (their head) and the Sun.
(Answer: New Moon)

Ask students to write "New Moon" on the line above box #1. Next ask the class what Phase
Square would represent the New Moon phase. (Answer: the blank black square). Instruct students
to glue the blank square in box #1. Tip: For less messy results, direct the students to apply glue
to the blank box on the chart, instead of on the back of each Phase Square.



                                                 7
Stage 3, continued
Continue “in orbit” to box #2 on the chart. Ask if someone can identify what phase happens here.
(Answer: Waxing Crescent) If there is hesitance, or confusion, give the students clues: “as you
turned to your left, the light began to shine on the right side of the Moon ball,” etc.

Once students have identified the Waxing Crescent, have them write the phase name above box
#2 and glue the correct Phase Square in place. For each phase, show the corresponding phase
illustration from Faces of the Moon so students can double-check their Phase Square choice.

Continue this procedure until all eight Phase Squares are correctly glued in place and all of the
phase names are labeled (see Figure 5).

     Figure 5




                Stage 4 • Reviewing What We’ve Learned

                (run time: approximately 10 minutes)
                Students now test their Moon knowledge through a fun review exercise.


Ask students to turn their Moon Phase Chart over, so they cannot see it. Draw a random Moon
phase on the board or a piece of paper and ask if someone can identify the phase by name.
Ask students if they can name the phases that would be seen before and after this phase. Once
a phase has been correctly identified, ask if someone in the class can move the dial of the Orbit
Spin Chart to show where in orbit this phase occurs. Continue quizzing the class with random
phases until all of the phases and orbital positions have been correctly identified. Allow students
to take home the charts to share.

The back of Faces of the Moon includes Moon “Memo-Rhymes” which are great reinforcement
phrases set in rhyme. Once learned, these Moon facts are rarely forgotten. Have fun!

                                                8
Copy this page on card stock (heavier
paper). Cut out black spin dial and
attach with paper fastener.




                                           attach dial


                                          with fastener
                                              here




                  here

                      fasten
                 er




                                    ial
                       k   spin d
                t blac
         cut ou
Moo
                                                    n’s
                                          O
                            it
                                 rb                 5.
                                                                     UP



6.
                                      UP
                                                                     5         4.
                                                                                         UP




                                      6                                                  4

7.                                                                                  3.
                      UP                                          WATCHING                             UP
                                                                    FROM



                      7                                                                                3

8.                                                                                  2.
                                      UP                                                 UP




                                      8                   1.                             2
                                                                     UP




                                                                    1
                           29
                                .5                                                                it
                                     da
                                          ys                                                 rb
                                               to                                        O
                                                    com                            ’s
                                                          plete              M oon
           sunlight




                                                                                                            sunlight




N a me :
                                                               Sun
Phase Squares – cut out strips of the eight Moon phases - one strip per student

More Related Content

Viewers also liked

One or more_bound_planet_per_milk_way_stars
One or more_bound_planet_per_milk_way_starsOne or more_bound_planet_per_milk_way_stars
One or more_bound_planet_per_milk_way_starsSérgio Sacani
 
Observations the postcorecollapse_globular_cluster_ngc_6752
Observations the postcorecollapse_globular_cluster_ngc_6752Observations the postcorecollapse_globular_cluster_ngc_6752
Observations the postcorecollapse_globular_cluster_ngc_6752Sérgio Sacani
 
The baryon oscillation_spectroscopic_survey_of_sdss_iii
The baryon oscillation_spectroscopic_survey_of_sdss_iiiThe baryon oscillation_spectroscopic_survey_of_sdss_iii
The baryon oscillation_spectroscopic_survey_of_sdss_iiiSérgio Sacani
 
Viollent colisional history_of_vesta
Viollent colisional history_of_vestaViollent colisional history_of_vesta
Viollent colisional history_of_vestaSérgio Sacani
 
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infrared
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infraredUv bright nearby_early_type_galaxies_observed_in_the_mid_infrared
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infraredSérgio Sacani
 
Detection of visible light from the darkest world
Detection of visible light from the darkest worldDetection of visible light from the darkest world
Detection of visible light from the darkest worldSérgio Sacani
 

Viewers also liked (16)

One or more_bound_planet_per_milk_way_stars
One or more_bound_planet_per_milk_way_starsOne or more_bound_planet_per_milk_way_stars
One or more_bound_planet_per_milk_way_stars
 
Observations the postcorecollapse_globular_cluster_ngc_6752
Observations the postcorecollapse_globular_cluster_ngc_6752Observations the postcorecollapse_globular_cluster_ngc_6752
Observations the postcorecollapse_globular_cluster_ngc_6752
 
Expansion universe
Expansion universeExpansion universe
Expansion universe
 
Hollows in mercury
Hollows in mercuryHollows in mercury
Hollows in mercury
 
Aa17123 11
Aa17123 11Aa17123 11
Aa17123 11
 
Aa16870 11
Aa16870 11Aa16870 11
Aa16870 11
 
Eso1147a
Eso1147aEso1147a
Eso1147a
 
Tmnrv1n1jul2011
Tmnrv1n1jul2011Tmnrv1n1jul2011
Tmnrv1n1jul2011
 
Hartmann wood 1971
Hartmann wood 1971Hartmann wood 1971
Hartmann wood 1971
 
Aa16869 11
Aa16869 11Aa16869 11
Aa16869 11
 
The baryon oscillation_spectroscopic_survey_of_sdss_iii
The baryon oscillation_spectroscopic_survey_of_sdss_iiiThe baryon oscillation_spectroscopic_survey_of_sdss_iii
The baryon oscillation_spectroscopic_survey_of_sdss_iii
 
Viollent colisional history_of_vesta
Viollent colisional history_of_vestaViollent colisional history_of_vesta
Viollent colisional history_of_vesta
 
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infrared
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infraredUv bright nearby_early_type_galaxies_observed_in_the_mid_infrared
Uv bright nearby_early_type_galaxies_observed_in_the_mid_infrared
 
Gas cloud black_hole
Gas cloud black_holeGas cloud black_hole
Gas cloud black_hole
 
Detection of visible light from the darkest world
Detection of visible light from the darkest worldDetection of visible light from the darkest world
Detection of visible light from the darkest world
 
Quadrantideos origens
Quadrantideos origensQuadrantideos origens
Quadrantideos origens
 

Similar to Fotm tg

Modeling Moon Phases and Eclipses
Modeling Moon Phases and EclipsesModeling Moon Phases and Eclipses
Modeling Moon Phases and EclipsesDSVSTraining
 
Our Planet’S Moon
Our Planet’S MoonOur Planet’S Moon
Our Planet’S Moongueste24a76
 
Our Planet’s Moon
Our Planet’s MoonOur Planet’s Moon
Our Planet’s Moonguestc914d0
 
Our Planet’s Moon
Our  Planet’s  MoonOur  Planet’s  Moon
Our Planet’s Moonguestc914d0
 
Changes In Our World
Changes In Our WorldChanges In Our World
Changes In Our Worldrdlewis123
 
Our Planet’S Moon
Our Planet’S MoonOur Planet’S Moon
Our Planet’S Moonguestc914d0
 
Objectives The purpose of this lab is to get you to understand th.docx
Objectives The purpose of this lab is to get you to understand th.docxObjectives The purpose of this lab is to get you to understand th.docx
Objectives The purpose of this lab is to get you to understand th.docxhopeaustin33688
 
Solar System Powerpoint Lesson
Solar System Powerpoint LessonSolar System Powerpoint Lesson
Solar System Powerpoint Lessoners331
 
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docx
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docxNATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docx
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docxrosemarybdodson23141
 
Sss Grades 3 5 Unit 4
Sss Grades 3 5 Unit 4Sss Grades 3 5 Unit 4
Sss Grades 3 5 Unit 4gbushey
 
Technology Integrated Lesson
Technology Integrated LessonTechnology Integrated Lesson
Technology Integrated LessonBlair Young
 
3 28 moon ntes student ppt
3 28 moon ntes student ppt3 28 moon ntes student ppt
3 28 moon ntes student pptaalleyne
 
Science Standard 4 ~
Science Standard 4 ~Science Standard 4 ~
Science Standard 4 ~guest5b9bf8
 
Science Standard 4 ~
Science Standard 4 ~Science Standard 4 ~
Science Standard 4 ~guestbf83e2
 
Science lesson plan eled 4312-004
Science lesson plan   eled 4312-004Science lesson plan   eled 4312-004
Science lesson plan eled 4312-004Lilly Shea
 

Similar to Fotm tg (20)

The Moon
The MoonThe Moon
The Moon
 
Modeling Moon Phases and Eclipses
Modeling Moon Phases and EclipsesModeling Moon Phases and Eclipses
Modeling Moon Phases and Eclipses
 
Moon.potx
Moon.potxMoon.potx
Moon.potx
 
Our Planet’S Moon
Our Planet’S MoonOur Planet’S Moon
Our Planet’S Moon
 
Our Planet’s Moon
Our Planet’s MoonOur Planet’s Moon
Our Planet’s Moon
 
Our Planet’s Moon
Our  Planet’s  MoonOur  Planet’s  Moon
Our Planet’s Moon
 
Changes In Our World
Changes In Our WorldChanges In Our World
Changes In Our World
 
E328 Unit and Lesson
E328 Unit and LessonE328 Unit and Lesson
E328 Unit and Lesson
 
Our Planet’S Moon
Our Planet’S MoonOur Planet’S Moon
Our Planet’S Moon
 
Objectives The purpose of this lab is to get you to understand th.docx
Objectives The purpose of this lab is to get you to understand th.docxObjectives The purpose of this lab is to get you to understand th.docx
Objectives The purpose of this lab is to get you to understand th.docx
 
Solar System Powerpoint Lesson
Solar System Powerpoint LessonSolar System Powerpoint Lesson
Solar System Powerpoint Lesson
 
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docx
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docxNATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docx
NATS 1740 AssignmentSun, Earth and Moon SystemThis assignmen.docx
 
Sss Grades 3 5 Unit 4
Sss Grades 3 5 Unit 4Sss Grades 3 5 Unit 4
Sss Grades 3 5 Unit 4
 
Technology Integrated Lesson
Technology Integrated LessonTechnology Integrated Lesson
Technology Integrated Lesson
 
Moon Phases Stations Lab
Moon Phases Stations Lab Moon Phases Stations Lab
Moon Phases Stations Lab
 
Moon Phases Stations Lab
Moon Phases Stations LabMoon Phases Stations Lab
Moon Phases Stations Lab
 
3 28 moon ntes student ppt
3 28 moon ntes student ppt3 28 moon ntes student ppt
3 28 moon ntes student ppt
 
Science Standard 4 ~
Science Standard 4 ~Science Standard 4 ~
Science Standard 4 ~
 
Science Standard 4 ~
Science Standard 4 ~Science Standard 4 ~
Science Standard 4 ~
 
Science lesson plan eled 4312-004
Science lesson plan   eled 4312-004Science lesson plan   eled 4312-004
Science lesson plan eled 4312-004
 

More from Sérgio Sacani

Formation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disksFormation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disksSérgio Sacani
 
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bNightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bSérgio Sacani
 
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Sérgio Sacani
 
Disentangling the origin of chemical differences using GHOST
Disentangling the origin of chemical differences using GHOSTDisentangling the origin of chemical differences using GHOST
Disentangling the origin of chemical differences using GHOSTSérgio Sacani
 
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...Sérgio Sacani
 
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...Sérgio Sacani
 
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoIsotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoSérgio Sacani
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsSérgio Sacani
 
Observational constraints on mergers creating magnetism in massive stars
Observational constraints on mergers creating magnetism in massive starsObservational constraints on mergers creating magnetism in massive stars
Observational constraints on mergers creating magnetism in massive starsSérgio Sacani
 
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...Sérgio Sacani
 
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...Sérgio Sacani
 
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...Sérgio Sacani
 
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPRFirst Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPRSérgio Sacani
 
The Sun’s differential rotation is controlled by high- latitude baroclinicall...
The Sun’s differential rotation is controlled by high- latitude baroclinicall...The Sun’s differential rotation is controlled by high- latitude baroclinicall...
The Sun’s differential rotation is controlled by high- latitude baroclinicall...Sérgio Sacani
 
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGNHydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGNSérgio Sacani
 
Huygens - Exploring Titan A Mysterious World
Huygens - Exploring Titan A Mysterious WorldHuygens - Exploring Titan A Mysterious World
Huygens - Exploring Titan A Mysterious WorldSérgio Sacani
 
The Radcliffe Wave Of Milk Way is oscillating
The Radcliffe Wave Of Milk Way  is oscillatingThe Radcliffe Wave Of Milk Way  is oscillating
The Radcliffe Wave Of Milk Way is oscillatingSérgio Sacani
 
Thermonuclear explosions on neutron stars reveal the speed of their jets
Thermonuclear explosions on neutron stars reveal the speed of their jetsThermonuclear explosions on neutron stars reveal the speed of their jets
Thermonuclear explosions on neutron stars reveal the speed of their jetsSérgio Sacani
 
Identification of Superclusters and Their Properties in the Sloan Digital Sky...
Identification of Superclusters and Their Properties in the Sloan Digital Sky...Identification of Superclusters and Their Properties in the Sloan Digital Sky...
Identification of Superclusters and Their Properties in the Sloan Digital Sky...Sérgio Sacani
 
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...Sérgio Sacani
 

More from Sérgio Sacani (20)

Formation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disksFormation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disks
 
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bNightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
 
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FUOri...
 
Disentangling the origin of chemical differences using GHOST
Disentangling the origin of chemical differences using GHOSTDisentangling the origin of chemical differences using GHOST
Disentangling the origin of chemical differences using GHOST
 
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
 
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...
PossibleEoarcheanRecordsoftheGeomagneticFieldPreservedintheIsuaSupracrustalBe...
 
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoIsotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on Io
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
 
Observational constraints on mergers creating magnetism in massive stars
Observational constraints on mergers creating magnetism in massive starsObservational constraints on mergers creating magnetism in massive stars
Observational constraints on mergers creating magnetism in massive stars
 
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...
Observation of Gravitational Waves from the Coalescence of a 2.5–4.5 M⊙ Compa...
 
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...
The SAMI Galaxy Sur v ey: galaxy spin is more strongly correlated with stella...
 
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...
Is Betelgeuse Really Rotating? Synthetic ALMA Observations of Large-scale Con...
 
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPRFirst Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
First Direct Imaging of a Kelvin–Helmholtz Instability by PSP/WISPR
 
The Sun’s differential rotation is controlled by high- latitude baroclinicall...
The Sun’s differential rotation is controlled by high- latitude baroclinicall...The Sun’s differential rotation is controlled by high- latitude baroclinicall...
The Sun’s differential rotation is controlled by high- latitude baroclinicall...
 
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGNHydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
Hydrogen Column Density Variability in a Sample of Local Compton-Thin AGN
 
Huygens - Exploring Titan A Mysterious World
Huygens - Exploring Titan A Mysterious WorldHuygens - Exploring Titan A Mysterious World
Huygens - Exploring Titan A Mysterious World
 
The Radcliffe Wave Of Milk Way is oscillating
The Radcliffe Wave Of Milk Way  is oscillatingThe Radcliffe Wave Of Milk Way  is oscillating
The Radcliffe Wave Of Milk Way is oscillating
 
Thermonuclear explosions on neutron stars reveal the speed of their jets
Thermonuclear explosions on neutron stars reveal the speed of their jetsThermonuclear explosions on neutron stars reveal the speed of their jets
Thermonuclear explosions on neutron stars reveal the speed of their jets
 
Identification of Superclusters and Their Properties in the Sloan Digital Sky...
Identification of Superclusters and Their Properties in the Sloan Digital Sky...Identification of Superclusters and Their Properties in the Sloan Digital Sky...
Identification of Superclusters and Their Properties in the Sloan Digital Sky...
 
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...
Digitized Continuous Magnetic Recordings for the August/September 1859 Storms...
 

Recently uploaded

A Domino Admins Adventures (Engage 2024)
A Domino Admins Adventures (Engage 2024)A Domino Admins Adventures (Engage 2024)
A Domino Admins Adventures (Engage 2024)Gabriella Davis
 
Injustice - Developers Among Us (SciFiDevCon 2024)
Injustice - Developers Among Us (SciFiDevCon 2024)Injustice - Developers Among Us (SciFiDevCon 2024)
Injustice - Developers Among Us (SciFiDevCon 2024)Allon Mureinik
 
Maximizing Board Effectiveness 2024 Webinar.pptx
Maximizing Board Effectiveness 2024 Webinar.pptxMaximizing Board Effectiveness 2024 Webinar.pptx
Maximizing Board Effectiveness 2024 Webinar.pptxOnBoard
 
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024BookNet Canada
 
Pigging Solutions Piggable Sweeping Elbows
Pigging Solutions Piggable Sweeping ElbowsPigging Solutions Piggable Sweeping Elbows
Pigging Solutions Piggable Sweeping ElbowsPigging Solutions
 
Scaling API-first – The story of a global engineering organization
Scaling API-first – The story of a global engineering organizationScaling API-first – The story of a global engineering organization
Scaling API-first – The story of a global engineering organizationRadu Cotescu
 
Handwritten Text Recognition for manuscripts and early printed texts
Handwritten Text Recognition for manuscripts and early printed textsHandwritten Text Recognition for manuscripts and early printed texts
Handwritten Text Recognition for manuscripts and early printed textsMaria Levchenko
 
Benefits Of Flutter Compared To Other Frameworks
Benefits Of Flutter Compared To Other FrameworksBenefits Of Flutter Compared To Other Frameworks
Benefits Of Flutter Compared To Other FrameworksSoftradix Technologies
 
Breaking the Kubernetes Kill Chain: Host Path Mount
Breaking the Kubernetes Kill Chain: Host Path MountBreaking the Kubernetes Kill Chain: Host Path Mount
Breaking the Kubernetes Kill Chain: Host Path MountPuma Security, LLC
 
How to Remove Document Management Hurdles with X-Docs?
How to Remove Document Management Hurdles with X-Docs?How to Remove Document Management Hurdles with X-Docs?
How to Remove Document Management Hurdles with X-Docs?XfilesPro
 
GenCyber Cyber Security Day Presentation
GenCyber Cyber Security Day PresentationGenCyber Cyber Security Day Presentation
GenCyber Cyber Security Day PresentationMichael W. Hawkins
 
The 7 Things I Know About Cyber Security After 25 Years | April 2024
The 7 Things I Know About Cyber Security After 25 Years | April 2024The 7 Things I Know About Cyber Security After 25 Years | April 2024
The 7 Things I Know About Cyber Security After 25 Years | April 2024Rafal Los
 
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmatics
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmaticsKotlin Multiplatform & Compose Multiplatform - Starter kit for pragmatics
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmaticscarlostorres15106
 
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...Integration and Automation in Practice: CI/CD in Mule Integration and Automat...
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...Patryk Bandurski
 
Understanding the Laravel MVC Architecture
Understanding the Laravel MVC ArchitectureUnderstanding the Laravel MVC Architecture
Understanding the Laravel MVC ArchitecturePixlogix Infotech
 
08448380779 Call Girls In Greater Kailash - I Women Seeking Men
08448380779 Call Girls In Greater Kailash - I Women Seeking Men08448380779 Call Girls In Greater Kailash - I Women Seeking Men
08448380779 Call Girls In Greater Kailash - I Women Seeking MenDelhi Call girls
 
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...HostedbyConfluent
 
Human Factors of XR: Using Human Factors to Design XR Systems
Human Factors of XR: Using Human Factors to Design XR SystemsHuman Factors of XR: Using Human Factors to Design XR Systems
Human Factors of XR: Using Human Factors to Design XR SystemsMark Billinghurst
 
Unblocking The Main Thread Solving ANRs and Frozen Frames
Unblocking The Main Thread Solving ANRs and Frozen FramesUnblocking The Main Thread Solving ANRs and Frozen Frames
Unblocking The Main Thread Solving ANRs and Frozen FramesSinan KOZAK
 
Install Stable Diffusion in windows machine
Install Stable Diffusion in windows machineInstall Stable Diffusion in windows machine
Install Stable Diffusion in windows machinePadma Pradeep
 

Recently uploaded (20)

A Domino Admins Adventures (Engage 2024)
A Domino Admins Adventures (Engage 2024)A Domino Admins Adventures (Engage 2024)
A Domino Admins Adventures (Engage 2024)
 
Injustice - Developers Among Us (SciFiDevCon 2024)
Injustice - Developers Among Us (SciFiDevCon 2024)Injustice - Developers Among Us (SciFiDevCon 2024)
Injustice - Developers Among Us (SciFiDevCon 2024)
 
Maximizing Board Effectiveness 2024 Webinar.pptx
Maximizing Board Effectiveness 2024 Webinar.pptxMaximizing Board Effectiveness 2024 Webinar.pptx
Maximizing Board Effectiveness 2024 Webinar.pptx
 
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024
#StandardsGoals for 2024: What’s new for BISAC - Tech Forum 2024
 
Pigging Solutions Piggable Sweeping Elbows
Pigging Solutions Piggable Sweeping ElbowsPigging Solutions Piggable Sweeping Elbows
Pigging Solutions Piggable Sweeping Elbows
 
Scaling API-first – The story of a global engineering organization
Scaling API-first – The story of a global engineering organizationScaling API-first – The story of a global engineering organization
Scaling API-first – The story of a global engineering organization
 
Handwritten Text Recognition for manuscripts and early printed texts
Handwritten Text Recognition for manuscripts and early printed textsHandwritten Text Recognition for manuscripts and early printed texts
Handwritten Text Recognition for manuscripts and early printed texts
 
Benefits Of Flutter Compared To Other Frameworks
Benefits Of Flutter Compared To Other FrameworksBenefits Of Flutter Compared To Other Frameworks
Benefits Of Flutter Compared To Other Frameworks
 
Breaking the Kubernetes Kill Chain: Host Path Mount
Breaking the Kubernetes Kill Chain: Host Path MountBreaking the Kubernetes Kill Chain: Host Path Mount
Breaking the Kubernetes Kill Chain: Host Path Mount
 
How to Remove Document Management Hurdles with X-Docs?
How to Remove Document Management Hurdles with X-Docs?How to Remove Document Management Hurdles with X-Docs?
How to Remove Document Management Hurdles with X-Docs?
 
GenCyber Cyber Security Day Presentation
GenCyber Cyber Security Day PresentationGenCyber Cyber Security Day Presentation
GenCyber Cyber Security Day Presentation
 
The 7 Things I Know About Cyber Security After 25 Years | April 2024
The 7 Things I Know About Cyber Security After 25 Years | April 2024The 7 Things I Know About Cyber Security After 25 Years | April 2024
The 7 Things I Know About Cyber Security After 25 Years | April 2024
 
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmatics
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmaticsKotlin Multiplatform & Compose Multiplatform - Starter kit for pragmatics
Kotlin Multiplatform & Compose Multiplatform - Starter kit for pragmatics
 
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...Integration and Automation in Practice: CI/CD in Mule Integration and Automat...
Integration and Automation in Practice: CI/CD in Mule Integration and Automat...
 
Understanding the Laravel MVC Architecture
Understanding the Laravel MVC ArchitectureUnderstanding the Laravel MVC Architecture
Understanding the Laravel MVC Architecture
 
08448380779 Call Girls In Greater Kailash - I Women Seeking Men
08448380779 Call Girls In Greater Kailash - I Women Seeking Men08448380779 Call Girls In Greater Kailash - I Women Seeking Men
08448380779 Call Girls In Greater Kailash - I Women Seeking Men
 
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...
Transforming Data Streams with Kafka Connect: An Introduction to Single Messa...
 
Human Factors of XR: Using Human Factors to Design XR Systems
Human Factors of XR: Using Human Factors to Design XR SystemsHuman Factors of XR: Using Human Factors to Design XR Systems
Human Factors of XR: Using Human Factors to Design XR Systems
 
Unblocking The Main Thread Solving ANRs and Frozen Frames
Unblocking The Main Thread Solving ANRs and Frozen FramesUnblocking The Main Thread Solving ANRs and Frozen Frames
Unblocking The Main Thread Solving ANRs and Frozen Frames
 
Install Stable Diffusion in windows machine
Install Stable Diffusion in windows machineInstall Stable Diffusion in windows machine
Install Stable Diffusion in windows machine
 

Fotm tg

  • 2. Bob Crelin • Illustrated by Leslie Evans Teacher’s Guide Northern Hemisphere edition Bob Crelin © Leslie Evans © Leslie Evans UNDERSTANDING THE PHASES OF THE MOON A fun, four-stage classroom unit for understanding the Moon’s phases (2–3 class periods) Objectives Students will be able to do the following: 1) Model how the relationship of our Earth, Moon, and Sun creates moon phases. 2) Chart the sequence and names of the eight primary Moon phases. 3) Identify each Moon phase by its appearance. 4) Identify the Moon’s position in orbit during each primary phase. Materials you will need: • Copy of the book Faces of the Moon by Bob Crelin (Charlesbridge) • Room that can be darkened, with enough open floor space to fit students standing in a circle • Bare light bulb on a stand (example: a floor lamp with shade removed) • Earth globe • Extension cord • Moon Orbit Spin Chart (included) • Paper fastener Each student will need: • Pencil or pen • 2"–4" (5–10 cm) Styrofoam ball mounted on a Popsicle stick (suppliers: craft/art supply store) • Moon Phase Chart (included) • Strip of eight Phase Squares (included) • Scissors • Glue stick NOTE: Before starting this unit, make paper photocopies of the Moon Phase Chart and the Phase Squares. Cut the Phase Squares into strips of the eight lunar phases. Photocopy the Moon Orbit Spin Chart on heavier card stock paper and assemble using a paper fastener. 1
  • 3. Advanced preparation The introduction (Stage 1) is brief and a prelude to the hands-on classroom activity (Stage 2). Making the following preparations before starting will allow the students to move easily between the steps while retaining concepts and terminology. For best results, choose a room that can be made completely dark when the lights are turned off (dark window coverings can help) Clear the floor space of obstacles and place a tall lamp with bare bulb (the brighter, the better) in the center of the room. Use an extension cord if necessary. Covering or taping down the lamp/extension cord will help to prevent students from tripping on it. For the hands-on demonstration, make sure that there is plenty of space for the students to stand and form a circle (with elbow room) around the lamp (see Figure 1 on page 3). Desks are not required. Students can sit on the floor during the introduction (Stage 1) and while constructing their charts (Stage 3). Have materials, including photocopies of the Moon Phase Chart and Phase Square strips, ready to hand out to students. Stage 1 • Introduction (run time: approximately 5–10 minutes) In storytelling fashion, students sit, listen, and look as the basic concepts and terms used throughout the lesson are introduced. Concept: The Moon cycle Read aloud the first two verses on pages 2–3 of Faces of the Moon: "Do you wonder, when you see the Moon..." Explain that the word "month" comes from “Moon.” Long ago, a month represented the time it took to complete one cycle of the changing Moon phases (approximately 29.5 days). Today, we call this a "lunar month," compared to our modern "calendar month." Concept: Moon phases as light and shadow Read aloud the next two verses on pages 4–5: "Each changing face (or lunar phase)..." Explain that we are able to see the Moon from Earth because the Sun’s light shines on it. The sunlit part of the Moon makes the phase, or shape, of the Moon that we see (the rest of the Moon is in shadow). Concept: Earth’s relationship to the Moon and Sun Read aloud the next two verses on pages 6–7: "For as she orbits Earth in space," Explain that the sunlit part of the Moon changes because we are watching from the surface of Earth as the Moon moves in orbit around our planet. The changing Moon phases have been given names that describe their appearance, and their place in the phase cycle. 2
  • 4. Stage 2 • Modeling the Phasing Moon (run time: approximately 20–30 minutes) After a brief explanation of the activity, students participate by following the step- by-step directions of the instructor, and by learning about each phase from the book. Explain to the class that by building a model of the Moon’s orbit, we can demonstrate why we see the changing phases of the Moon. To make a model of the Moon phases, we will need three "players" from our solar system. Ask students to identify who these players are. (Answer: Moon, Sun, and Earth) Show the items that represent each player: • The Styrofoam ball on the Popsicle stick for the Moon • The light bulb on the stand for the Sun • The globe for Earth (for now) Briefly review (and demonstrate) with students the basic orbital motions of these players: • Earth orbits around the Sun. • The Moon orbits around Earth. It helps to visually demonstrate these motions by walking the globe (Earth) in a counterclock- wise “orbit” around the light bulb (Sun), while circling the Styrofoam ball (Moon) counterclock- wise around the globe. Figure 1 The Hands-on Activity* *Elements of this exercise are based on an Astro-Adventures learning activity, Dennis Schatz and Doug Cooper • pacsci.org Turn on the light bulb “Sun” in the center of the room. Turn off all other room lights. For safety, remind students not to touch the hot light bulb. Have each student get a Styrofoam Moon ball on a stick. Have the students stand and form a circle around the light bulb Sun (see Figure 1). Tip: Students should leave elbow room between themselves for easier movement during the demonstration. Explain that the globe will not represent Earth in the activity, because as we learned earlier, we watch the Moon phases change from Earth’s surface. Instead, each student’s head will represent Earth for the demonstration. Because their eyes are set in their head, they can watch the changing appearance of the Moon from their “Earth.” 3
  • 5. Stage 2 • Modeling the Phasing Moon, continued Figure 2 Have the students place their hand on their left shoulder. Moon Earth This represents their “eastern” side. Explain that, during the Sun demonstration, they will turn towards the east, or left, side to simulate the Moon’s counterclockwise orbital motion around Earth (see Figure 2). Explain to the students that they will demonstrate the Moon’s orbit in step-by-step movements, following your direction. eft a rd s the l ro tat e to w Introduce the assembled Moon Orbit Spin Chart (Figure 3) to the students. Point out the parts of the chart that represent their head, their Styrofoam Moon ball, and the light bulb Sun. Figure 3 Show how the orbit circle has eight numbered stops that represent the eight primary Moon phases. When modeling the “orbit,” students will pause together at each stop (see Figure 4 on page 6). At each stop, they will observe the appearance of their Moon ball, and listen to a rhyme that names and describes this Moon phase. Show the students the Orbit Spin Chart dial set at stop #1 (as shown in Figure 3). Ask them to position themselves and their Moon as shown on the chart. Each student should hold their Moon out in front of their head and face the light bulb Sun. Stop #1 - New Moon Remind students that it is the Sun’s light shining on the Moon that shows us the phase we see. Ask them how much sunlight they see on their Moon in position #1. They should see no sunlight, because the shadowed side of the Moon is facing their “Earth” (their head). Ask if anyone knows what phase this is. (Answer: New Moon) Read aloud page 8 of Faces of the Moon (stanza describing this New Moon phase): "The Moon's first phase, we call it NEW..." After reading the New Moon stanza, have the class say, "New Moon" together. Stop #2 - Waxing Crescent Explain that, together, the students will now begin to rotate, stopping at each phase around the Moon's orbit. Hold the Orbit Spin Chart up for all to see, and move the dial from stop #1 (New Moon) to stop #2 (Waxing Crescent). Ask the students to turn to the east (left) as shown on the chart. Once students are in the correct position, ask them to look at their Moon ball to notice the sunlight illuminating the right edge of it. 4
  • 6. Stage 2 • Modeling the Phasing Moon, continued Page 11 of the book shows a die-cut illustration of the Waxing Crescent Moon. Have students compare this illustration to the sunlit crescent on their own Moon ball. Read aloud page 10 (stanza describing the Waxing Crescent phase): "A few days pass, and Moon's less shy..." Have the class say, "Waxing Crescent" together. The term “Waxing” This is a good point in the lesson to associate the term "waxing" with the apparent growth of the Moon. A great comparison is the old practice of “candle dipping,” in which each dip of a candle wick in hot wax would make the candle grow thicker. The growing Moon can be seen as "waxing," like the candle. Stop #3 - First Quarter Next, move the chart dial to stop #3. Ask the students to rotate to this position. They should notice that the sunlight has “grown” to fill the right half of their Moon ball. Compare the Moon ball with the illustration of the First Quarter Moon on page 13 of the book. Read aloud page 12: "We notice Moon's FIRST QUARTER phase..." The class says, "First Quarter" together. Stop #4 - Waxing Gibbous Continue to stop #4 on the Orbit Spin Chart. The students move accordingly and notice the increasing sunlight on the right side of their Moon ball. Show the Waxing Gibbous illustration on page 15 and read page 14: "Once she's past First Quarter Moon,..." The class says, "Waxing Gibbous" together. Stop #5 - Full Moon Move to stop #5. Make sure that students hold their Moon ball a little above their head in this position so as not to cast a shadow on the ball. If positioned correctly, they should see a Full Moon, without shadow. Pages 17 and 18 portray the Full Moon, and pages 16 and 19 describe it: "Next comes Moon's most famous phase..." The class says, "Full Moon" together. Stop #6 - Waning Gibbous Mention that the Moon has now “waxed” full of sunlight. As students continue on to stop #6 in the orbit, they should notice how the sunlight begins to decrease, or "wane" on their Moon ball. A shadow now begins to “grow” on the Moon's right side, as shown in the illustration on page 20. Read aloud page 21: "Once past Full, the shadows start..." The class says, "Waning Gibbous" together. Stop #7 - Last Quarter Continue to stop #7. The students move and notice that the sunlit part has decreased. Their Moon ball is now lit on the left half. Show the Last Quarter illustration on page 22 and read page 23: "At Moon's LAST QUARTER of her trip,..." The class says, "Last Quarter" together. Stop #8 - Waning Crescent Move the chart dial to stop #8. The students move and compare the crescent of sunlight on their Moon ball to the illustration on page 24. Read page 25 aloud: "From early dawn to morning blue,..." The class says, "Waning Crescent" together. 5
  • 7. Stage 2 • Modeling the Phasing Moon, continued Then move the chart dial–and ask the students to rotate–back to STOP #1, where they began their orbit. Read page 27 aloud: "Then Moon returns where she'd begun..." Ask the students to tell you all together the name of this phase (New Moon). Remind them that they have just modeled one complete Moon orbit around our Earth. This represents the 29.5-day “lunar month.” To support this visual demonstration of the changing phases, have the students now do an additional complete rotation (in the same direction), turning slowly without stopping this time. Ask them to watch the changing pattern of light and shadow on their Moon ball as they go. Remind them to keep their Moon ball a little above their head to prevent a “head-shadow lunar eclipse” at the Full Moon position. STOP #1 Figure 4 She sees only the Moon’s shadowed side: NEW MOON STOP #3 She sees the right half of her Moon in sunlight: FIRST QUARTER STOP #6 She sees the shadow forming on the right side of her Moon: WANING GIBBOUS 6
  • 8. Stage 3 • Recording Our Observations (run time: approximately 20–30 minutes) Students create their own charts to record what they’ve learned from the hands- on Moon phase activity. Students can move to their desks, or to a clear spot on the floor, to assemble their Moon charts. Each student will need a pencil or pen, a copy of the Moon Phase Chart, a strip of the eight Phase Squares, a pair of scissors, and a glue stick. Show the students how the Moon Phase Chart is modeled after the Orbit Spin Chart used during the demonstration, with the Sun, Earth and Moon in the same relative positions. Once assembled, the chart will show and name the pattern of Moon phases throughout a lunar month. For best results and participation, ask the students to follow the steps together as a class. A simple mistake, like a reversed Phase Square, can throw off the rest of the phase pattern. First, ask students to separate the eight Phase Squares by cutting them apart along the white lines. Before cutting, many students will notice that the phases on the strip are out of sequence. Next, ask students to find the box marked #1 on their Moon Phase Chart. Remind students that this is where they began the Moon’s orbit in the demonstration. Ask if someone can identify the phase they saw when the Moon ball was in this position, between Earth (their head) and the Sun. (Answer: New Moon) Ask students to write "New Moon" on the line above box #1. Next ask the class what Phase Square would represent the New Moon phase. (Answer: the blank black square). Instruct students to glue the blank square in box #1. Tip: For less messy results, direct the students to apply glue to the blank box on the chart, instead of on the back of each Phase Square. 7
  • 9. Stage 3, continued Continue “in orbit” to box #2 on the chart. Ask if someone can identify what phase happens here. (Answer: Waxing Crescent) If there is hesitance, or confusion, give the students clues: “as you turned to your left, the light began to shine on the right side of the Moon ball,” etc. Once students have identified the Waxing Crescent, have them write the phase name above box #2 and glue the correct Phase Square in place. For each phase, show the corresponding phase illustration from Faces of the Moon so students can double-check their Phase Square choice. Continue this procedure until all eight Phase Squares are correctly glued in place and all of the phase names are labeled (see Figure 5). Figure 5 Stage 4 • Reviewing What We’ve Learned (run time: approximately 10 minutes) Students now test their Moon knowledge through a fun review exercise. Ask students to turn their Moon Phase Chart over, so they cannot see it. Draw a random Moon phase on the board or a piece of paper and ask if someone can identify the phase by name. Ask students if they can name the phases that would be seen before and after this phase. Once a phase has been correctly identified, ask if someone in the class can move the dial of the Orbit Spin Chart to show where in orbit this phase occurs. Continue quizzing the class with random phases until all of the phases and orbital positions have been correctly identified. Allow students to take home the charts to share. The back of Faces of the Moon includes Moon “Memo-Rhymes” which are great reinforcement phrases set in rhyme. Once learned, these Moon facts are rarely forgotten. Have fun! 8
  • 10. Copy this page on card stock (heavier paper). Cut out black spin dial and attach with paper fastener. attach dial with fastener here here fasten er ial k spin d t blac cut ou
  • 11. Moo n’s O it rb 5. UP 6. UP 5 4. UP 6 4 7. 3. UP WATCHING UP FROM 7 3 8. 2. UP UP 8 1. 2 UP 1 29 .5 it da ys rb to O com ’s plete M oon sunlight sunlight N a me : Sun
  • 12. Phase Squares – cut out strips of the eight Moon phases - one strip per student