This unit is a study of the structure
of the solar system, the characteristics of the members of that
system, and a more detailed look at the rotations and revolutions
of the Earth and the Moon
.
The grade 1 Core Unit Earth
and the grade 1 Optional Unit The
Sky deal with some of the characteristics of the Earth
and some of the planets which can be identified in the night
sky.
Exploring Space, a grade 6 Core Unit, further develops some of the themes of this unit, especially those on the descriptions of the planets.
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Put a small marker (a piece of modelling clay or masking tape) on the globe to locate St. John's, Newfoundland, your community, and Nanaimo, B.C. Ask the students which location gets sunlight first as the Earth rotates. Which location gets sunlight last? When the sunlight has just left St. John's, is it still light where you live? Extend this to European and Japanese cities compared to your community. Is there any way that there can be daylight in Paris and St. John's at the same time, or in Paris and your community, or in Tokyo and your community? Is there a noticeable difference between northern and southern Saskatchewan. This activity can lead to a discussion of time zones and differences of length of day in north and south.
Factors: A4, B3, B14, C6, C8, C10, C12, E4, E8, F3, F5
Objectives: 1.1, 1.2
Assessment Techniques: 1, 3, 5, 8
Common Essential Learnings: Critical and Creative Thinking. By observing the effect of light on the globe, students understand the phenomena of sunrise, and sunset. How the stationary Sun and rotating Earth can account for the observations we make every day is emphasized.
Part 1.
Now it is noon. They are back standing in the snowy field,
facing south again. How would they have to move their eyes
or
head to see the sun?
Finally it is almost supper time. They have come back to the
field one more time. The sun is setting. If they once more
stand facing south,how will they have to move their eyes or
turn their head to see the setting sun? How does that
direction compare with the morning, and at noon?
Ask the students to check this out at morning, noon, and
evening tomorrow.
Part 2.
Have one student stand on the cardboard facing the direction
of the south arrow and another student stand at the midpoint
of the left hand wall of the classroom holding a flashlight
shining toward the student on the cardboard. Turn off the
lights in the room and close the curtains, if possible.
Imagine that the cardboard (or chair) represents the Earth,
the arrow of tape points south, and the flashlight reflector
represents the Sun. Ask the student on the cardboard to
stand
with legs straddling the tape, looking straight ahead in the
direction the tape points, south. Daytime is when the sun
shines on the student's face. It is early in the morning and
the sun is not up yet. Slowly start to rotate the cardboard
counterclockwise on the floor. Have the student on the
cardboard indicate as soon as the flashlight reflector
becomes
visible using peripheral vision. The student's head should
not turn from looking the same direction as the arrow. Use
the
reference tape on the rug to determine in what direction the
Sun would first become visible.
Continue to rotate the cardboard and stop when the tape is
pointing towards the front wall of the classroom. From which
direction is the Sun visible now? Has the Sun moved? Has the
Earth rotated? Continue rotating the cardboard until the
tape
is pointing at the flashlight. At what time of day is the
Sun
in the south? Continue rotating the cardboard until the
flashlight has almost disappeared from the field of view of
the student on the cardboard. In what direction is the
flashlight from the cardboard? What does this represent?
What
fraction of a full rotation has the cardboard gone through
since the beginning? Continue turning the cardboard for
another quarter turn. What time is represented now?
Turn back to the beginning direction. This represents the
rotation of the Earth for one complete day. Stress that the
Earth has rotated but the Sun did not move. The Sun appeared
to move from east to west through the field of view of the
observer who was always facing south. Discuss the ancient
belief that it was the Sun which moved across the sky. Does
it
still seem like the Sun moves? You might want to mention the
legend of Apollo. Apollo was the Greek god whose job it was
to
drive the chariot of the Sun across the sky each day.
Factors: A2, B3, B14,
C6, C10, E4,
E8, F5,
G3
Objectives: 1.1, 1.2
Assessment Techniques: 1, 3, 5,
7c
Common Essential Learnings: Critical and Creative Thinking. This activity introduces students to the difficult
concept that how we perceive an event or situation depends
on
the preconceptions and assumptions that we have before we
begin to evaluate it. For instance, consider only two cars
and
nothing else. To an observer in car A, the situation with
car
A travelling at 110 km/h passing car B moving at 100 km/h
looks exactly the same as car B backing up at 10 km/h past a
stationary car A. The motion that one perceives depends on
the
frame of reference. Changing frames of reference can lead to
a totally different perception of the type of motion which
is
taking place.
When the person in the middle calls out "rotate" the people
in
the circle must spin slowly on the ball of one foot in a
counterclockwise direction. When the centre calls out
"revolve" the people in the circle walk slowly in a
counterclockwise direction. If "revolve and rotate" are
called
out, the circlers must both spin on the their feet and move
slowly in a counterclockwise direction. When "stop" is
called,
the circlers stop in exactly the direction they were facing
when the call went out. The centre will then call either
"time" or "season."
If "time" is called, each circler must determine the time of
day, based on the direction each is facing. If stop is
called
when one is facing directly away from the Sun, the time is
midnight. If facing toward the Sun, the time is noon.
Intermediate directions produce times between those. The 24
hour clock could be introduced to allow estimation of these
times, or the A.M. and P.M. designation could be used.
If "season" is called, each person must turn to see where
the
midsummer marker is, and figure out the season from
there.
After a suitable pause for reflection on the answer to the
call for time or season, the centre person should call the
name of one person in the circle, who will give the answer.
The rest of the circlers and the person in the centre can
evaluate that answer.
Factors: B3, B18, C10, C12, E8,
F3, F5,
G3
Objectives: 1.1, 1.2
Assessment Techniques: 1, 3, 5,
7c
Common Essential Learnings: Communication. This gives
students an opportunity to reinforce the meanings of the
terms
rotate and revolve in a situation where they can get visual
clues from other students and from the teacher, and relate
the
terms to a physical experience. It also gives them a chance
to
link the terms and their motions to the time of day and the
seasons.
The moonrise is a phenomenon similar to sunrise. When the
Earth rotates so that the Moon comes into view, the Moon
appears to rise. (Use the rug activity (#2) to illustrate
this. Hold a tennis ball in the back corner of the room
opposite the flashlight, or any other position along the
walls
for the phases. This can also be illustrated with a globe
and
a tennis ball for the Moon and a flashlight for the Sun. At
the grade three level, students are expected to understand
only the concepts of new moon and full moon.
A full moon occurs when the Moon is on the opposite side of
the Earth from the Sun. At full moon, the Moon appears to
rise
(comes into view) when the Sun sets. New moon occurs when
the
Moon is on the same side of the Earth as the sun. Since it
is
on the same side of the Earth as the Sun, the new moon rises
when the sun rises and is visible all day long, setting in
the
evening. Between new moon and full moon is called the waxing
crescent moon. After full moon comes the waning crescent
moon,
which lasts until new moon.
Factors: A2, A4, B3,
B14, C6,
C8, C10, C12, E4,
E8, F5,
G3
Objectives: 1.4, 1.5
Assessment Techniques: 1, 3, 5,
7c
Common Essential Learnings: Critical and Creative Thinking. Models are used to develop an understanding of the
Earth-Moon-Sun system.
Factors: A2, A5, B8,
C7, C12, E4, F5,
G3
Objectives: 1, 3, 5, 7c,
9
Common Essential Learnings: Numeracy. This gives a
visual link between the numerical data on the distances from
the Sun to each planet, and the relative distances between
planets. The activity places the planets at appropriate
positions on a number line.
Objectives: 2.1, 2.3
Assessment Techniques: 2, 3, 4,
5,
6, 9
Common Essential Learnings: Numeracy. Students will
develop a concept of the size of the Earth through concrete
representations. Independent Learning. Students will
understand that there is a great deal in this world to
investigate
and study.
Using the information they have obtained for each planet,
the
students could produce television or radio ads promoting
tourist travel to one of the planets, and present them to
the
class or to other classes. A science fair project could be
to
'simulate' a planet's environment, and then invite
'tourists'
to visit.
This is an excellent opportunity to work on resource
retrieval, including the use of periodical indexes. The unit
can be planned with the help of the teacher-librarian.
Factors: A2, A5, C6,
C12, E4,
G3
Objectives: 2.1, 2.2, 2.3
Assessment Techniques: 2, 3, 4,
5,
6, 9
Common Essential Learnings: Communication. From a
variety of textual, visual, and perhaps auditory resources,
students synthesize their concepts of the planets.
Discuss with the students where the various constellations
are
in the sky, and how to recognize them. Schedule one night
when
they can come with their parents to a good viewing site, and
together learn to identify planets and stars. Possibly some
parents or other resource persons will have some expertise
in
this area. An astronomer or an astronomy teacher could be
invited to talk to the group. Hot chocolate or some other
refreshments will help make this night class more
attractive.
If feasible, plan a field trip to an observatory in
conjunction with this activity.
Objectives: 2.5
Assessment Techniques: 1, 3, 4,
5,
9
Common Essential Learnings: Independent Learning.
This
activity is designed to spark an interest in observing the
sky. If the parents are involved in the activity, the
students
will understand that learning can take place at any age, and
that learning can be a cooperative activity.
This activity may be done in conjunction with the grade 3
Core Unit Animals.
Objectives: 2.4
Assessment Techniques: 2, 3, 4, 5,
9
Common Essential Learnings: Critical and Creative Thinking. In this activity the students must visualize a life
form which is compatible with both the characteristics of one
of the planets and with the requirements of life as we know
it.
Factors: A2, A4, A5,
B3, B8,
B14, C6,
C7, C8,
E8, F3
Objectives: 1.2, 1.3, 1.5
Assessment Techniques: 2, 3, 4, 5,
9
Common Essential Learnings: Numeracy. The concepts of
time and calendars, and quantification of an abstract
concept (time) are developed in this unit.
Ask the students to close their eyes and imagine that it is
very early in the morning, before sunrise. They are outside
standing in an snowy field. Christmas will be here soon and
the air is crisp and clean. They are facing south and
looking
straight ahead. After a minute or so, streaks of reddish
light
flood across the meadow. From what direction are the
sunbeams
coming? How would they have to move their head or their eyes
to see the rising sun?
On a piece of heavy corrugated cardboard at least 1 m by 1m,
make an arrow from masking tape, or with a felt-tip marker.
Label the arrow as pointing south. The other directions can
be
marked, too. Place the cardboard on the floor near the
centre
of the back wall of the classroom, and orient it so that the
south arrow points toward the right hand wall of the
classroom
as one looks toward the front. (A student might sit in a
rotating chair rather than stand on the cardboard. In this
case put the arrow on the seat or arm of the chair so that
it
faces the front edge.)
Planet
Mercury
Venus
Earth
Mars
Jupiter
Saturn
Uranus
Neptune
Pluto
Distance
6 cm
10 cm
14 cm
22 cm
74 cm
136 cm
280 cm
428 cm
562 cm