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The Winter 2010 issue of The Earth Scientist includes a variety of educational resources, ranging from astronomy to glaciers. Check out the other publications and classroom materials in our online store.
The two basic types of regions on the Moon: a smooth, dark mare on the left and a heavily-cratered, light-colored highland region on the upper right.

Lunar Geology

Looking up at the Moon, you can see that there are dark regions and light regions. With binoculars, you can even see that the dark regions are smooth compared to the light regions which have many craters.

Dark areas on the Moon are called maria, which means "seas" in latin. Astronauts discovered that these regions are smooth and shallow. Maria have few craters and are covered with a type of rock (called basalts) which are similar to lava rocks formed by volcanoes here on Earth. Tests showed that these lunar rocks are between 3.1 and 3.8 billion years old.

Light-colored areas are more hilly and covered with lots of craters. This is the "land", or terrae on the Moon. The color of these areas comes from a type of light-colored rock called anorthosite. This type of rock is found only in the oldest mountain ranges on the Earth. Geologists have found that these lunar rocks are over 4 billion years old. That's nearly as old as the solar system itself!

Once it was known that the light areas were old and the dark maria younger, scientists could piece together the Moon's history.

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Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part by the National Science Foundation and NASA, our Founding Partners (the American Geophysical Union and American Geosciences Institute) as well as through Institutional, Contributing, and Affiliate Partners, individual memberships and generous donors. Thank you for your support! NASA AGU AGI NSF