The Moon, Earth's only natural satellite, is easily observed with the naked eye. Over the course of one month, you can observe its full range of appearances and its pattern of movement in the sky. The phases of the Moon (new, crescent, quarter, gibbous, and full) are a result not of a change in the actual shape of the Moon, but of the relative positions of the Sun, Moon, and Earth. That is, the apparent changes in the Moon's shape are simply changes in the portion of the lit side of the Moon that you can see from Earth.
However, misconceptions regarding the Moon's apparent change in shape still abound. Some believe that clouds or some other object cover up the Moon, blocking our view of part of it. This may happen, but it is not the mechanism behind the lunar cycle. Others believe that the shadow of Earth or some other object falls on the Moon's surface, causing the phases of the Moon. While the Moon does occasionally cross Earth's shadow, resulting in a lunar eclipse, shadows cast by Earth are not what cause lunar phases.
In this lesson, students learn about the Moon's changing appearance and its pattern of movement. Through class discussion, activities, and multimedia resources, students explore the phases of the Moon and are introduced to the concept of orbital motion.
When discussing the phases of the Moon, it is important to refer to the changing appearance of the Moon rather than the changing shape .
Two to three class periods, separated by days and weeks
Arrange to begin the lesson when the Moon is in first quarter (it will be visible during the afternoon). Set up and try the model demonstration to make sure that the lighting in the classroom will be effective. The light source should be placed in a central location with room for students to move around it.
1. Ask students to share their ideas about the Moon. Encourage them to talk about what they have already observed and any conceptions that they may have. Ask:
2. Explain that the class is going to study the Moon based on their own observations. Ask:
3. Show the first minute of the Galileo: Discovering Jupiter's Moons, which discusses some of Galileo's observations of the Moon.
4. (Optional) Discuss what the Moon looks like up close. Remind students that humans have actually been on the Moon and have taken pictures and brought back samples of Moon rocks. Work though the Explore the Moon as a class.
5. As a class, look at the Phases of the Moon to see examples of how the Moon can appear from Earth. Discuss each screen as you go through the interactive.
6. Explain that the class will be making daily observations of the Moon and recording them in a Moon Journal. Their journal entries will include sketches of how the Moon looks each day (when visible), as well as the date, time, location of the Moon in the sky (direction and height above the horizon), weather conditions, and the name of the phase.
7. Distribute the notebooks for the Moon Journals. Have students make their first journal entry as a class. If the Moon is in first quarter, it should be visible during the afternoon. Go outside as a class and help students locate the Moon. Note: Remind students never to look directly at the Sun.
8. Assign students to continue to make daily observations of the Moon in their journals.
9. After a few days of observations, have students look at their journal entries. Ask:
10. After a couple of weeks of observations (past the full phase), have students look at their journal entries again. Ask:
11. Explain that the Moon does not give off any light of its own -- it only reflects sunlight. Because the Moon revolves around Earth, it looks different to us from day to day as it changes position in its orbit. For more information about how the Moon orbits Earth, show the Why Doesn't the Moon Fall Down?. Note: Even though Earth is sometimes positioned between the Sun and the Moon (such as at full moon), it is much smaller than the Sun, so it doesn't usually block the Sun's rays from reaching the Moon. However, occasionally, the three bodies line up just right so that Earth does block sunlight from reaching the Moon, causing a lunar eclipse.
12. Distribute the balls and have students work in pairs to model the Earth-Moon-Sun system. The light source, representing the Sun, should be placed in a central area with the students surrounding it. Each student represents Earth, and the ball (held at arm's length) represents the Moon. Half of the ball should be illuminated, and as the student rotates in place, the visible portion of the illuminated part will mimic the phases of the Moon. Have students explore this model for a few minutes. Note: To an observer on Earth, the curved side of the lit part of the Moon always faces the Sun (notice how it changes side before and after the new moon phase).
13. Review the phases of the Moon: new, crescent, quarter, gibbous, and full. Write the names of the phases on the board and also have students draw an illustration on the board of each phase.
14. Choose a phase and point to its illustration. Ask students to position their Moons so that they look like the picture. For example, if you ask for a full moon, the students need to manipulate their positions to simulate the full moon phase (i.e., the lamp is behind them and the fully lit side of the Moon is facing them). Have students explain the following:
15. Have students challenge their partners with the model -- one student acts as the model while the other asks for specific phases. Make sure each student has a chance to be both the model and the challenger. Then ask:
16. (Optional) Show The Origin of the Moon. This video segment from NOVA follows the Apollo 15 astronauts as they collect samples of ancient rock from the Moon's crust. The discovery of this ancient rock helps lead to a radical new theory about the Moon's origin. Note that this video segment is intended for middle school and high school students.
Have students discuss the following:
The Digital Library for Earth System Education (www.dlese.org) offers access to additional resources on this topic.