Universe Cycle - Solar System (4)
 Lab 

   
OBJECTIVES:
  • Observing craters on the surface of planets and moons.
  • Speculating on the origin of craters in the Solar System.
VOCABULARY:
  • craters
  • mare
  • rays
  • rills
  • satellite photograph
MATERIALS:

Students make craters.

BACKGROUND:

The surfaces of the terrestrial planets are covered with impact craters, except for the Earth. Many of the Solar System’s moons also have many craters. Impact craters form when a meteroite strikes the surface. The impact hits with so much force that it compresses the rock it strikes, forming the crater. The impact also vaporizes the impacting object. This impact plus the rebound of the compressed rock ejects material out of the crater. This material may spread up to thousands of kilometers away, depending on how much energy is released. The shape of the crater may change if its walls begin to slump inward, partially filling it up as shown in the figure to the left.

Craters may also be destroyed by surface processes, such as weathering, and flows of water, wind, and ice. This is why craters are rare on Earth. Old craters have been destroyed.

Our understanding of the origin of craters was limited until pictures and samples were returned from our own Moon's surface. We now have good photographic evidence for craters from the other terrestrial planets, especially Mars and Venus. Craters on these planets are difficult to interpret; some scientists think that some of them may be volcanic in origin.

On the Moon, the floor of a typical crater is below the average level of the surface. The crater is surrounded by a raised rim. Ejected material appears as piles of rubble or loose rock in a zone around the crater, or from larger craters, as a system of rays. Some craters are cut by rills, which are cracks in the surface. Rills may be faults, possibly caused by ancient tectonic activity or cooling processes.

Some very large lunar impact craters are filled by volcanic rock very similar to the terrestrial igneous rock basalt. These filled craters are usually called mare, from the Latin word for ocean. Scientists suggest that after a large impact, molten rock leaked up from the interior of the Moon along cracks, partially filling the crater.

In this activity the students first make their own craters, and then observe real craters using pictures from the lunar surface.

PROCEDURE:
  1. Explain how craters form to the students. You may wish to draw the diagrams shown in the background information to help. Explain the probable origin of lunar mare to the class. Again, you may wish to draw the diagram above on the board. Tell the student that they are going to make craters, and then look for real craters on the Moon.
     
  2. Have the students work in groups. Have the students follow the directions on the lab sheet, or if you prefer, assemble the cratering materials in advance. Pour flour into each pan and level it into a layer at least 4-5 cm thick. Have the students work outside or spread newspapers on the classroom floor. Have each student stand on a chair and drop a spoonful of flour into the pan from a height of about a meter. This will form mini-craters in the flour that have the same raised rims and sloping sides as real craters.

    If you have corn meal, you may want to mix that in with the flour. It gives the crater a more defined rim.
     

  3. Alternatively, you may want to make several craters with a few students, and have the rest of the class observe and record the craters on their lab sheets.
     
  4. You can also experiment by changing the angle of impact, by throwing the flour into the pan at an angle. This is how most "real" craters form; rarely if ever does an object strike exactly perpendicular to the Earth’s surface. Be careful, angled impacts can be messy! You should see, that unless the impact angle is very shallow, a circular crater is created. You may want to discuss with students that impacting objects do not hit the Earth straight on.
     
  5. Divide the students into groups of four. Give each group a packet of Moon photographs. Make sure that they return the material to the same packet. Give each student a magnifier. Have them look at each of the four pictures to try and determine which ones show craters and which ones do not. Have them count the number of craters on each photo, and record the information on their lab sheets.

    Have the students try to detect the difference between a mare and an impact crater. This is actually hard to see. You may wish to hint that the very large craters are usually mare. Instruct the students to look at the shadow. They may be able to tell the difference between a hill and a depression. But this is difficult also. It is good for the students to see the difficulty in this interpretation. Facing ambiguity is an important part of doing science.

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