(1) PREDICTIONS: Fill out this part
first. If you don't know, GUESS - this is
not graded, but it is crucial for motivating your later investigations.
20 minutes.
A.) Describe the sun's path in Olympia,
today, in words.
Where did it rise? Where will it
set? how high will it get? E W N S
or something in between?
rise:
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set:
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height:
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B.) in Olympia: How would
you expect the sun's path to look in June?
Where on the horizon would you expect the sun to
rise and set? How high will it get in the sky?
Write down your predictions WITHOUT using your solar motion
detector. And in December?
in Olympia
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rise/set directions
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how high in the sky?
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June Sun
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December Sun
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C.) Now think about different
latitudes. How would the sun's path look at midsummer
from the North pole? From the equator?
Where on the horizon would you expect the sun to
rise and set? How high will it get in the sky?
midsummer Sun
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rise/set directions
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how high in the sky?
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from North Pole
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from Equator
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D.) Think about different latitudes
at mid-March. How would the sun's path look
at mid-March from the North pole? From Olympia?
From the equator? Where on the horizon
would you expect the sun to rise and set? How high
will it get in the sky?
Sun at mid-March
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rise/set directions |
how high in the sky? |
from North Pole
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from Olympia
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from Equator
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E.) Go back and think again
about how high the Sun gets at different latitudes at different
times of the year. Predict when the Sun will
reach its highest point from the North pole, from
Olympia, and from the equator. Will the Sun reach
the Zenith - the top of the sky - from each latitude?
If so, when? If not, how high will it
get?
Sun's highest point
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reaches Zenith?
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when? or how high?
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from North Pole
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from Olympia
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from Equator
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F) Zenith crossings.
How many times a year does the Sun
cross the Zenith from the Equator?
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At what latitude does the Sun cross
the Zenith only one day each year?
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Why?
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(2) In class: briefly
discuss your predictions with your team. Then
build your Solar Motion Detector,
following Zita's instructions. 15 min.
(3) Use your solar motion detector to answer
the questions in Part (1) above. Fill in your
answers with a different colored pen, so you can easily
compare.
(4) Then go back and compare your results to your
predictions.
Discuss your predictions and
investigations with your workshop team.
What do you agree on? What results differed
from your predictions? What can you conclude?
What are you still wondering about?
The MISMATCHES or SURPRISES are
the most interesting cases: these are where you
learn the most. Articulate as clearly as possible
the ways in which your observations DIFFERED from your predictions.
A.) Path of the sun
today in Olympia:
Agreements:
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Surprises:
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Conclusions:
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Questions:
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B.) Path of the sun in Olympia
in June:
Agreements:
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Surprises:
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Conclusions:
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Questions:
.
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C.) Different latitudes at
midsummer: (North pole and equator)
Agreements:
.
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Surprises:
.
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Conclusions:
.
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Questions:
.
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D.) Different latitudes at
mid-March. (North pole, Olympia, and equator)
Agreements:
.
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Surprises:
.
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Conclusions:
.
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Questions:
.
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E.) Different times
of the year. (North pole, Olympia, and equator)
Agreements:
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Surprises:
.
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Conclusions:
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Questions:
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F.) Zenith crossings.
Agreements:
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Surprises:
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Conclusions:
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Questions:
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(5) 20 minutes: Discuss cultural
significance: As a team, think about
how you could keep track of the Sun's path, without
special equipment.
What solar positions and dates are remarkable?
Why?
What significance did (or could)
these dates have to other cultures? Why?
How would you find when the Sun is
at those positions?
How could you mark when the Sun will
be at the same position next year?
How did (or might) other cultures
mark these positions and times?
Suppose you are an ancient astronomer-priest
and your life depends on predicting the day of celestial
events exactly. Which day would be easier to
predict exactly, solstice or equinox, using the scheme
you developed above? What occasion would
you assign to this day, to demonstrate your power
and your queen's divinity?
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