Experimenting with Craters

Impact craters form whenever an asteroid or comet crashes into the solid surface of another body. Craters can form on planets, moons, and even asteroids. The process of cratering is responsible for shaping the surfaces of most objects in the Solar System.

Wind and rain on Earth slowly erase craters, so only recent craters or the very largest craters remain visible as time passes. For example, Meteor Crater, in northern Arizona, is about 10,000 years old, a blink of the eye in the history of our planet. On bodies like the Moon or Mercury that have no air or water, craters can last millions or billions of years, preserving a record of the pummelling they've received.

Impacts occur at phenomenal speeds - 5000 times faster than a dropping rock. The force of the impact is enough to pulverize rock. But using some basic ingredients, you can study how craters are formed.

The materials for the crater activity are:

Instructions:
An important observation to make for each crater is the way the flour is distributed around the crater on the cocoa. Long streaks are known as rays and can be seen in many images of craters, especially Kepler, Copernicus, and Tycho craters on the Moon.

Pictures of craters are available on various sites on the web:
This page shows a variety of craters on the Moon, Mars, Venus, and Earth
This page is an atlas of images of the Moon (lots of images, so be patient)
This picture shows several craters with rays on the Moon
This picture is a sharp image of the Full Moon
This picture is a sharp image of the Far Side of the Moon (the side always pointing away from Earth)


Questions/comments? Contact us at astro.info@asu.edu