Teacher's Guide for:

Planet Search

OBJECTIVES:

This show conforms to the following state science standards:  12.F.1a, 12.F.1b, 12.F.2a, 12.F.2b, 12.F.2c, 12.F.3b, 12.D.5b, 12.F.2a

BRIEF SHOW DESCRIPTION: PRE-VISIT ACTIVITIES/TOPICS FOR DISCUSSION:
  1. What is a "planet?" How can you tell the difference between stars and planets in the sky?
  2. Where can you find the planets in the sky? 
  3. What makes our Earth a special planet? What does it have that no other planet has? [liquid water]
  4. If you were to build a space ship, what other planet would you want to visit? Why?
POST-VISIT ACTIVITIES/TOPICS FOR DISCUSSION:
  1. Construct a simple model illustrating the distance between the Earth and the Moon. Most classrooms or libraries are equipped with a globe of the Earth. If this globe is roughly 12 inches in diameter then the Moon's relative size would be the size of a baseball. Have students note that the Moon's diameter is a bit smaller than the width of the United States. Now the Moon must be placed at the correct distance from the Earth, which is about 30 feet on this scale. Discuss how long it took our Apollo astronauts to travel this distance. 
  2. The tremendous distances in our solar system may be visualized in the classroom by constructing a model from simple home items. In order to fit the model within a room we have divided the actual distances by a factor of 450.
     
    Object  Diameter  Scale Object  Scale Distance
    Sun  864,000 miles 38-inch circle
    Mercury  3,100 miles  brass BB  3-1/8 inches
    Venus  7,550 miles  marble  6-3/4 inches
    Earth  7,927 miles  marble  9-1/4 inches
    Mars  4,200 miles  1/4" bead  14-1/8 inches
    Jupiter  88,900 miles  softball  48-1/2 inches
    Saturn  75,200 miles  baseball  89-1/4 inches
    Uranus  29,200 miles  golf ball  177-3/4 inches
    Neptune  28,000 miles  ping pong ball 279-3/4 inches
    Pluto  1,500 miles  grain of sand  367 inches
    Oort 
    Cloud
    7-1/3 miles 
    Alpha Centauri 
    (nearest star)
    39-1/2miles 

    After completing the model, you may discuss the following issues: 

    1. The elliptical orbit of Pluto brings it inside the orbit of Neptune for 20 years of Pluto's 248 year orbit about the Sun. Where is Pluto now? Which is the farther planet? 
    2. Given these distances illustrate where the Voyager 2 spacecraft is at present after passing Neptune in August of 1989, discuss the distance it has covered since its launch in 1977. 
    3. Introduce the laws of Kepler and Newton. Discuss the fact that the closer a planet is to the Sun, the shorter time it takes for that planet to make a complete revolution. 
  3. Discuss the school year for the mythical schools on the planet Uranus. Remember that with the extreme tilt of the axis of the planet, summers and winters are both 20 years in length. How would the school year be structured? How long would it take to graduate?
  4. The amount of gravity a planet possesses depends on its mass. A person's weight depends not only on the amount of mass the person has but also on the amount of gravity. Therefore a person will weigh less on a planet that is smaller than the Earth and weigh more on a planet that is larger than the Earth. This can be illustrated by using a simple can of soda pop. On Earth this 16-ounce can weighs 386 grams. Take several other empty soda cans and fill them with material (lead pellets, marbles, rock, etc.) until they weigh the following amounts for each planet. This is how much a full can would weigh if you were to take it to the planet:
    Body grams
    Sun  10,808 
    Mercury  150 
    Venus  339 
    Earth  386 
    Mars  147 
    Jupiter  903 
    Saturn  357 
    Uranus  307 
    Neptune  434 
    Pluto  170 
VOCABULARY LIST:
 
 
Accretion  Meteorite  Asteroid  Moon 
Comet  Orbit  Ecliptic  Planet 
Meteor  Prominence  Revolution  Rotation 
Star  Sunspot 

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