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Name ________________
Sun's Impact on Earth's Temperature
Student Instruction and Answer Sheet
| Materials
Needed
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Useful On-line
Resources
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Part I - Observing the Planets
Consider the weather and
cloud patterns visible on Venus, Earth, and Mars. Which planet has more
chaotic weather patterns? Propose several possible hypotheses.
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Venus
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Earth animatedGIF
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Mars QuickTimeMovie
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TemperatureRange850
to 900 FRotationalPeriod248 days
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TemperatureRange-70
to 140 FRotationalPeriod24 hours
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TemperatureRange-200
to 40 FRotationalPeriod24 hours
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Part
II - Computer Models
The last time a class conducted
the assessment in the section above, they concluded that Venus has more
dynamic weather patterns than Earth, which, in turn, has more dynamic weather
patterns than Mars. Similarly, they noted that Venus has little variation
in temperature, while Earth has a moderate variation in temperature, and
Mars has a widely varying temperature. The class settled on three competing
hypotheses. Your task is to use the computer
models from the Solar System Collaboratory (URL)
to evaluate which hypothesis seems to be the most correct or to propose
your own.
| Pat's
Hypothesis |
The
farther away a planet is from the Sun, the colder it is. |
| Chris's Hypothesis |
A planet far from the Sun
can be hot if it has a high albedo. |
| Aaron's Hypothesis |
A planet far from the Sun
can be hot if it has a high greenhouse effect. |
INSTRUCTIONS
ON HOW TO USE THE SOLAR SYSTEM COLLABORATORY COMPUTER MODELS.
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Access
the Solar System Collaboratory Computer Model (image
and real-time
access)
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Notice that the model contains
an imaginary planet, Planet X. Wherever you click the mouse, Planet X will
move to that point. Try moving it around and see what happens to
the temperature gauge on the right side of the screen.
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Read the temperature gauge as
accurately as you can and CONVERT the Kelven temperature to Fahrenheit
by entering a number in the KELVIN BOX and clicking in the FAHRENHEIT BOX.
It is useful to remember that 300 K is about room temperature, 70 F.
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Change the characteristics of
Planet X above the temperature converter. You can:
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observe the planet's temperature
as it relates to distance;
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change the planet's albedo (reflectivity)
of the atmosphere in a range of values from 0 to 1;
- change the planet's atmospheric
composition, called the GREENHOUSE EFFECTIVENESS) in the range of
0 to 1000. To learn more about the Greenhouse Effectiveness,
you might want to check out this
on-line resource.
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To get a feel for the numbers,
start by putting Planet X at the same distance Earth is from the Sun and
start changing the variables of albedo and greenhouse effectivenss to see
what happens to the temperature. Can you make Earth have a temperature
of 75 F?
EVALUATING THE
HYPOTHESES
Consider each of the hypothese
proposed below and test each one using the Collaboratory
Computer Model. Analyze the strengths and weaknesses of each
proposal and decide which is the most correct. Or better yet, propose
your own hypothesis and provide data to support your proposal.
| Pat's
Hypothesis |
The
farther away a planet is from the Sun, the colder it is. |
| Chris's Hypothesis |
A planet far from the Sun
can be hot if it has a high albedo. |
| Aaron's Hypothesis |
A planet far from the Sun
can be hot if it has a high greenhouse effect. |
| Your Hypothesis |
Your Hypothesis
Your Hypothesis
Your Hypothesis
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Part
III - Asking More Questions of the Computer Models
- How does varying the planet's
distance from the Sun change the temperature? If you double the
distance, does it halve the temperature? If you triple the distance,
does the temperature drop to 3-2 (that is,one ninth) its
original value?
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How good is the model?
Can you replicate the listed temperature on Mercury, Venus, Earth, and
Mars?
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How does changing the albedo
change a planet's temperature? Why does this occur?
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How close do you need to move
Mars in order for it to sustain life? How far away do you need to
put Venus? Can you make these planets sustain life?
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FFS - Facts for Students
The sun is the major source
of energy for phenomena on the earth's surface, such as growth of plants,
winds, ocean currents, and the water cycle. Seasons result from variations
in the amount of the sun's energy hitting the surface, due to the tilt
of the earth's rotation on its axis and the length of the day. |
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