Physics coursework
To investigate the factors affecting the sizes of impact craters
Aim
My main aim was to find out if the crater occurred on the planet Earth. Before I started to do this experiment, I did some research to do with crater.
An impact may also be surrounded by an ejector blanket. This is a layer of material thrown out the formation of a crater. For example, the Ries crater in southern Germany is surrounded by a blanket of material up to 100 meters thick. Simple crater formation tends to be bowl shaped, like the Barringer Meteor crater and Wolf Creek. The ratio of width to dept is usually in the area of 5:1.
These uplifts are believed to be formed by a rebound in the Earth's crust after extremely compression by impact forces. As the crust rebounds back it find itself under significantly less pressure because the impact has removed millions of tonnes of material from the surface. Because the crust is now effectively overcompensating, this causes rock from below the crater bottom to break through to the surface and overshoot to form an up lift. The 13 Henbury craters in Australia were discovered in May 1931. The crater lies in an elliptical pattern covering a total area of about 1.25 square kilometres.
To investigate the factors affecting the sizes of impact craters
Aim
My main aim was to find out if the crater occurred on the planet Earth. Before I started to do this experiment, I did some research to do with crater.
An impact may also be surrounded by an ejector blanket. This is a layer of material thrown out the formation of a crater. For example, the Ries crater in southern Germany is surrounded by a blanket of material up to 100 meters thick. Simple crater formation tends to be bowl shaped, like the Barringer Meteor crater and Wolf Creek. The ratio of width to dept is usually in the area of 5:1.
These uplifts are believed to be formed by a rebound in the Earth's crust after extremely compression by impact forces. As the crust rebounds back it find itself under significantly less pressure because the impact has removed millions of tonnes of material from the surface. Because the crust is now effectively overcompensating, this causes rock from below the crater bottom to break through to the surface and overshoot to form an up lift. The 13 Henbury craters in Australia were discovered in May 1931. The crater lies in an elliptical pattern covering a total area of about 1.25 square kilometres.