Crater Counting

Introduction

Impact craters are the dominate landforms on most of the solid
surfaces in our solar system. These impact craters have formed on the
surfaces over the 4.6 billion years of our solar system. The number
of craters on a surface increases with the length of time that surface
has been exposed to space. These rather simple ideas are the basis
for a very powerful tool, called **crater counting**, that
planetary scientists use to unravel the history of a planetary
surface. The basic idea is that an old surface will have more impact
craters than a younger surface.

By counting the number of craters in some defined area on a world
(determining its **crater density**) and comparing it to the number
of craters on a same-sized area on another part of that world, you can
determine the **relative ages** of the two surfaces (*e.g.*
one area is twice as old as another).

If you want to find out the **absolute age** of the surface you are
studying, you need a sample from that surface. Fortunately for us,
the Apollo mission brought back lots of rocks from six sites on the
Moon. By measuring the ages of rocks from these six sites, and
measuring the crater density at these sites, we can determine how the
crater density is related to the absolute age at these sites. Now, at
least for the Moon, if we can measure the crater density of any part
of the Moon, we can compare it to the crater density at the Apollo
sites to determine their relative ages. Since we now know the
absolute ages of the rocks at the Apollo sites, we can determine the
absolute age of any part of the Moon.

In this class, we make the assumption that the cratering rate measured
by Apollo on the Moon is typical of the cratering rate in the inner
solar system. (**N.B.** This is a **very** important
assumption! You know you will be asked about it on the midterm). We
can now extend our measurements of the crater density on the Moon to
estimate the ages of various regions on the surface of Mars.

Data

The materials we will use for this lab are images taken by the Viking 1 and 2 orbiters.

The Viking project consisted of launches of two separate spacecraft to Mars. Viking 1, launched on 20 August 1975, and Viking 2 launched on 9 September 1975. Each spacecraft consisted of an orbiter and a lander. After orbiting Mars and returning images used for landing site selection, the orbiter and lander detached. The lander entered the Martian atmosphere and soft-landed at the selected site in the summer of 1976 . The orbiters continued imaging and conducting other scientific operations from orbit, while the landers deployed instruments on the surface. The Viking 1 orbiter was turned off on 17 August 1980, after returning more than 30,000 images in 1485 orbits around Mars. The Viking 2 orbiter was turned off on 25 July 1978, after returning almost 16,000 images in 706 orbits around Mars.

Procedure

- Download and print the data table and questions for this lab. Bring these to section. (This PDF is also in your course pack).
- Determine the crater density. Use the scale bar on the bottom of
the printed sheets of the two surfaces to determine how many craters
are in each size range (it helps if you transfer the scale bar to the
edge of a piece of paper). You may not be able to use all the
different size ranges. There may be no craters in some of the larger
ranges or too many craters in the smallest ranges. Try to fill in as
many of the size ranges as you can. Record the numbers in
the
*Crater Density Data Table*. - The data for the crater density of the Apollo sites was
determined over 1,000,000 km
^{2}. The total area of the images you used are shown at the bottom of the image. Using your numbers from the table and the formula below, determine how many craters of each size range are found in 1,000,000 km^{2}. Record this number in the table. - Plot your data points from the table on the Crater Density Graph. Put your points on the graph in the middle of your size range. For example, if you had 200 craters in the 0-8 km size range, you should put your point at the intersection of 200 on the y-axis, and 6 on the x-axis. (Note: the y-axis of this graph has a logarithmic scale. If you are unfamiliar with how to plot points on a logarithmic scale ask your TA).
- Determine the age of your surface. Once you have your points plotted, fit a straight line through the points, or as close to them as you can. Your line should be roughly parallel to the age lines on the graph. The line you have drawn represents the average age of the cratered surface you have been examining. Estimate the age by interpolating the location of the line you have drawn with the age lines already on the graph.
- Answer the questions on the back of the data table and questions handout.

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Last modified: Mon Jun 29 08:06:34 PDT 2009

Last modified: Mon Jun 29 08:06:34 PDT 2009