Teacher’s notes
Using models to understand how craters are formed
Rationale
Do craters only form from volcanoes or can they also be formed as the
result of an impact? Students will investigate different crater types
and critically consider the results of their investigations. These results
will be developed to construct a system to identify the features of
each type of crater.
Activity
Curriculum level 4-6
Planet Earth and beyond Topic
Space
Type of investigation
Modelling
What you need
- A variety of pictures showing crater-like holes caused by:
- volcanic activity (for example, Lake Taupo)
- impact (for example, craters on Mars, the Moon, and on Earth in
Siberia, Arizona and Tapanui (NZ)).
- For modelling impact craters:
- flour or other light-coloured material to represent layers. (If
only white sand is available to represent bedrock, use a dark powder
for the layers, such as flour mixed with cocoa or paint powder.)
- a bag of dark-coloured sand (to represent bedrock)
- newspaper
- a shallow box
- a knife or spoon for levelling
- a sieve
- two chairs
- various-sized objects, such as marbles and golf balls (to act
as meteorites).
- Optional:
- Making Better Sense of Planet Earth and Beyond
- Volcanoes, Building Science Concepts, Book 12.
Note: Supporting activity resources are provided
below.
Focus
- Where do we see craters in New Zealand?
- How do we recognise craters in the landscape?
- How do craters get formed?
- Can craters change over time?
- What would you like to know about craters?
Exploration
- Show students the crater pictures and discuss what the pictures have
in common, and ways in which the pictures differ from each other.
- Ask:
- How do you think the various craters formed?
- Do you think it is possible to tell the volcanic craters from the
impact craters? If so, how?
- Then:
- Carry out the following activity to model the effect of an impact.
- Place newspaper over the working area of the floor.
- Put the box in the centre of the working area.
- Fill the box with dark-coloured sand (bedrock) to a depth of 4 centimetres.
Lightly compact it and smooth with the levelling tool.
- Use the sieve to sprinkle a thin layer of the surface material over
the bedrock material.
- Choose one student to stand on a chair and drop a ‘meteorite’
on to the landscape.
- Ask:
- What pattern is made by the flying debris?
- Can you see layers of bedrock and surface material in the crater walls?
- Get the students to investigate the effects of the meteorites hitting
various multi-layered surfaces at different speeds and angles.
- Then:
- Have the students look again at the pictures of craters.
- Ask:
- What similarities do you notice between the craters you have made
and the ones in the pictures?
- What new questions do you have about craters?
- Challenge students to make a list of the features of the two crater
types – volcanic and impact.
Extension
- Use your model to find out the effect of many meteorites hitting a
similar area. Does the pattern of the flying debris give you an idea
of the order of the different impacts? How could this help scientists
determine the relative age of impacts on the Moon?
- How can the features of the two crater types be used to decide the
order of events that shaped the surface of a planet or the Moon?
Reflection
- How can modelling activities help scientists test their theories?
- Scientists used to think that the Moon’s craters were volcanic. What
helped them change their theories?
- What did you learn about craters from the modelling activity? What
new questions did you develop?
- How can your list of features help sort the impact craters from the
volcanic ones?
- How does the different ways craters form contribute to the differences
in their observable features?