
Craters are all around us! We can find them on both the Earth and the moon. They can either be created by impacts from meteors or volcano tops blowing off. This lab focuses on Impactor Craters.

SOME KEY TERMS:
floor: bowl shaped or flat, characteristically below surrounding ground level unless filled in with lava.
ejecta: blandet of material surrounding the crater that was excavated during the impact event. Ejecta becomes thinner away from the crater.
raised rim: rock thrown out of the crater and deposited as a ring-shaped pile of debris at the crater's edge during the explosion and excavation of an impact event.
walls: characteristically steep and may have giant stairs called terraces.
rays: bright streaks staring from a crater and extending away for great distances. See Copernicus crater for another example.
central uplifts:mountains formed because of the huge increase and rapid decrease in pressure during the impact event. They occur only in the center of craters that are larger than 40 km diameter.
GUIDING QUESTION:
What are the factors that affect the appearance of impact craters? How do scientists use craters to tell the relative age of them?
HYPOTHESIS:
I think that the younger the crater is, the rougher it will be, because it might erode over time. Factors that might affect the appearance of impact craters is the speed the meteor is coming at, the heat of it, the mass of the meteor, and the size of the meteor.
MATERIALS:
safety goggles, tray, flour, notebook, spoon, small and large marbles, meter stick, ruler, excel and word.
PROCEDURE:
1. Put on goggles and apron. Fill the pan with 2.5 cm of flour.
2. Drop a small marble into the flour. What did you observe? Drop another marble again. What happens when they overlap?
The marble creates a small impact. You can hear it and it sends waves throughout the whole tub. The ejecta goes a little farther than the marble all the way around. When they overlap, they overlap on debris and create a small mound. In real life, this could be extremely disastrous. It also creates a bigger crater in a stranger shape.
3. Drop the larger marble into the flour. What did you observe? Drop another marble again. What happens when they overlap?
When you drop the larger marble, it creates a much larger impact and the ejecta flies everywhere. When they overlap, they create a half-moon type shape.
4. Think about the guiding question. What does affect the appearance of an impact crater?
Just from dropping the two different-sized marbles, I can see that the size of the meteor definitely affects what the crater looks like. The larger the marble, the bigger the crater, and the deeper the impact is.
5. Decide on which materials you will use and collect them all to take to your station. You will make a model to test the guiding question.
6. You will need to collect some qualitative (using your senses to make observations) and quantitative-numerical data (Height of drop, mass of the object, diameter of crater, depth of the crater, length of ejecta - if possible to measure, etc...)
7. Make a data table (below)
8. Run your lab according to the method provided.
9. You may wish to take pictures of each impact to use later in a blog post, or you may sketch the results in your notebook.
10. Collect the data needed and enter it into the table.
| Trial | Height of Drop | Diameter | Length of Ejecta | Depth of Crater |
| 1 | 30 | 1.9 cm | 0.1 cm | 0.7 cm |
| 2 | 30 | 2 cm | 0.3 cm | 0.4 cm |
| 3 | 30 | 1.7 cm | 0.3 cm | 0.7 cm |
| average | 30 | 1.87 cm | 0.23 cm | 0.6 cm |
| Trial | Height of Drop | Diameter | Length of Ejecta | Depth of Crater |
| 1 | 60 | 3 cm | 0.7 cm | 4 cm |
| 2 | 60 | 2 cm | 0.6 cm | 1.8 cm |
| 3 | 60 | 2 cm | 0.7 cm | 2.4 cm |
| average | 60 | 2.34 cm | 0.67 cm | 2.73 cm |
| Trial | Height of Drop | Diameter | Length of Ejecta | Depth of Crater |
| 1 | 90 | 2.5 cm | 1 cm | 2.7 cm |
| 2 | 90 | 2 cm | 0.5 cm | 2 cm |
| 3 | 90 | 2.3 cm | 0.7 cm | 2.3 cm |
| average | 90 | 2.27 cm | 0.73 cm | 2.34 cm |
| Trial | Height of Drop | Diameter | Length of Ejecta | Depth of Crater |
| 1 | 200 | 2.1 cm | 1.2 cm | 3 cm |
| 2 | 200 | 2.4 cm | 0.9 cm | 2.7 cm |
| 3 | 200 | 2.8 cm | 1 cm | 2.8 cm |
| average | 200 | 2.43 cm | 1.03 cm | 2.83 cm |
DATA ANALYSIS:
1. Is your hypothesis about what affects the appearance and size of craters supported by test data? Explain why or why not.
I think that my hypothesis covers most of the factors in the appearance of craters, just the one that I didn’t mention that I realized during this lab was when two craters overlap and create a different-shaped crater.
2. What does the data reveal about the relationship between crater size and velocity of impactor?
Well, we didn’t necessarily test the impactor velocity, but the farther away from the tub the impactor starts, the more speed it gains. This works well with our data, because the further away we dropped the impactor, the deeper the crater was, and it tended to have a bigger diameter too.
3. What does the data reveal about the relationship between ejecta (ray) length and velocity of impactor?
The same thing applies to this – the greater the velocity is that the impactor is coming at, the greater effect it’s going to have on the surface. In this case, it creates a lot of ejecta.
4. If the impactor were dropped from 6 meters, would the crater be larger or smaller? How much larger or smaller? Explain your answer.
It would be a lot bigger. This is because it has time to gain speed as it falls, because it is a greater distance than 90 cm, for example. Then, when it hits the surface, it creates a deep and big crater, with lots of debris (ejecta) coming from it.
CONCLUSION:
My hypothesis was relatively correct. The appearance of impact craters is affected by the velocity of the impactor, the mass, size, and weight of the impactor, where the impact crater is, and whether the crater overlaps. The last factor is one that I just learned this lab. It’s true that most craters look like circles – we can see that when we look at the moon. However, when two impactor craters overlap, they create a unique half-moon type shape. My original hypothesis was that scientists detect how old craters are by whether they have eroded a lot or not, but the overlapping of two impactor craters is another more fool-proof way that scientists figure out how old they are.
FURTHER INQUIRY:
Unfortunately, for this lab I think we had a couple of errors in the data. Measuring the depth of the crater and the ejecta was difficult, because we had to make sure that we weren’t going to mess up the crater. However, just by looking at the experiments we were doing, we were able to tell what would happen in a real life situation when a meteor comes hurtling at the earth. Some craters are larger than others because the meteor that comes is either larger than normal, or is coming at a much greater speed. Another thing that might happen is two craters overlap, creating a very large ‘double crater’. It also has to do with the mass. Basically, anything that will make the meteor larger or heavier will cause a bigger crater. You could test this by dropping the impactors not only at different heights, but also just throwing it hard, making it faster. Or you could test this by comparing two different impactors, which we did at the beginning of this lab, with the smaller marble and the larger marble. The surface that the meteor hits could also have something to do with the appearance of the crater – if it’s very impressionable ground, the meteor will undoubtedly have a greater effect on it than if its solid rock.
