Target Level: Middle School
Timetable: Two 40-minute class periods
Vocabulary: crosscutting relationships, crust, geologic unit, mid-ocean ridge, plate tectonics, relative age, seafloor spreading, subduction zone, terrain
Materials: Each student will need two copies of C3 "Wedges" image, (with one printed on card stock), colored pencils, scissors.
Europa is a moon of Jupiter. Although its surface is frozen water, liquid water could exist beneath the ice. Spacecraft pictures show areas of the surface where large plates of ice have broken apart and moved away from each other. Some have even twisted and rotated. The easiest way for these movements to occur is if the plates were floating on water, just like ice floes in the polar seas on Earth. If the plates can be fit back together like a jigsaw puzzle, with their edges matching up neatly, it provides evidence that the material beneath them was once liquid, or at least a warm, slushy ice. Let's try it and see!
Part A: Geologic Mapping
Look at Figure 1. Differences in surface texture, color or shading show us that particular regions are made of different materials, formed in unique ways, or created at different times. Making a geologic map is an easy way to show these differences. Using a copy of the "Wedges" image (Figure 1), identify three large areas of similar texture or shading. For now, avoid the small, narrow ridges. Lightly color each of the three surface types using a different color, even if they are not touching on the map (for example, color all smooth bright areas light green). When you are done, each color represents a different geologic unit.
Part B: Determining Relative Age
Using the colored image, can you figure out which unit is oldest and which is youngest? One way to determine relative age is to look for crosscutting relationships. Like a cake that is sliced, the surface can be broken by fractures. The unit (or slice) which cuts through the rock (or cake) is always younger than the rock itself. In other words, you can't cut something unless it's already there! Using the color as the name for each unit, arrange them in order of their relative age in the space below.
Look again at the relative age of each geologic unit on the "time line" above. Carefully remove those pieces that belong to the youngest unit. This will leave empty space behind. Can you fill the empty space by shifting together the remaining units? What kinds of "motion" did you have to use to do this? (e.g. transform = sliding past; divergent = moving apart; convergent = moving together; or rotation) Do any features or ridges match up now that were once separated by the youngest unit? The surface you have created represents Europa at some time in the past.
Remove the pieces for the next youngest unit and shift the remaining pieces to fill the gaps. What types of motion were required this time? Do any features or ridges match up again? Compare this "original landscape" to an uncut C3 "Wedges" image.
As a final step, reverse the process and "rebuild" the surface of Europa one unit at a time. This should give you an idea of the geologic history responsible for shaping Europa's icy surface.
This activity was adapted from:
Tufts, B.R., Greenberg, R., Sullivan, R., and Pappalardo, R., 1997, Reconstruction of Europan terrain in the Galileo C3 "Wedges" image and its geological implications, Lunar and Planetary Science Conference XXVIII Houston, Lunar and Planetary Institute, p. 1455-1456.