# astr 110 astrophysics i – question the chart above is a crater countage graph whi

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The chart above is a crater count-age graph which you will use through this laboratory. You use it as follows:

2. Use the ruler to make a rough measurement of the size of one of these craters (in km).

3. Find the number nearest that size on the x-axis of the graph above. For example, if you find a crater with size ~15.5 km, look for 16 km in the graph. We’ll call this size the “target size.”

4. Count all the craters in the region with sizes between the small tick above the target size (20 km for a target size of 16 km) and the tick below the target size (14 km for the case of a target size of 16 km). This is the observed number of craters Nobs.

8. Repeat the experiment for another target size in the same region in order to obtain a second estimate of the age (not for Mars. Only once for Mars). Compare the two ages for consistency.

1. Age of the Lunar Maria

The age of the Lunar maria were measured by radioisotope dating and serves as the basis for the

crater count experiments. In this section, we will measure the age of the maria using crater

counts. We will use imaging data from Google Earth Pro

maps of the moon. To do this, start

a web browser, go to https://www.google.com/earth/versions/#earth-pro, and install the software.

If you are having difficulty downloading the software yourself, you can remote into UBC

Okanagan’s lab computers by following the instructions found at: link. Any of the computers in

SCI 126 will have the software.

Use the switch button ( ) in the top tool bar to navigate to the surface of the moon. Select moon

and find the maria which are the very dark regions on the moon. Zoom in on an area in the maria

and find a region with some craters. You will need to use the ruler ( ) in the top tool bar to

measure the sizes of objects (in km).

Q1: Using the method described in the introduction, measure the age of the maria using crater

counts.

The Apollo button shows where the moon landings occurred. Note that all of the landings were

on the maria and so all our sampling is from this area.

2. Age of the Lunar Highlands

The next area for exploration is the Lunar Highlands which are primarily on the far side of the

moon. They are the light colored regions near the equator of the moon, opposite the maria.

These regions have only been observed by satellite so the ages are only from crater counts.

These regions are reportedly the oldest surface areas of the moon. Does your crater counting

bear that out?

2/3

Lab 4 – Crater Counts and Surface Ages

Q2: Use the crater counting method to estimate the age of the lunar highlands. The same hints as

before apply.

Q3: The crater counting chart has a lot of information encoded in it. Based off your reading in

the textbook and class notes, answer the following questions: (1) Why do the “age lines” slope

from upper left to lower right? (2) Why are the age lines for older ages above the lines for

younger ages?

3. Concluding Investigation:

We can also use the crater counting chart above to estimate the ages of other surfaces in the Solar

system. The approximation is rather rough but relies on assuming (1) that the number of

impactors of a given size is uniform for a given period in the Solar System’s history and (2) that

the speed of impact is dominated by the orbital motion of the impactor and not the gravity of the

planet.

Q4: There are several images from the surface of Mars on Canvas. Select one image and use the

techniques you have developed above, estimate the age for this area. Submit the image showing

the measurement of the size of the craters.

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