Essential Question: How does the position of the sun, earth, and moon affect each other? S6E2a. Demonstrate the phases of the moon by showing the alignment.

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Presentation transcript:

Essential Question: How does the position of the sun, earth, and moon affect each other? S6E2a. Demonstrate the phases of the moon by showing the alignment of the earth, moon, and sun. S6E2b. Explain the alignment of the earth, moon, and sun during solar and lunar eclipses. Instructional Approach(s): The teacher should introduce the essential question and the standards aligned to the essential question.

Eclipses

What is an eclipse? Why do we not have an eclipse every month? Activating Strategy: What is an eclipse? Why do we not have an eclipse every month? Instructional Approach(s): The teacher should pose the questions to the class. The teacher may opt to have students discuss the questions with a partner. An eclipse is the total or partial blocking of light of one object by another object. We do not have solar and lunar eclipses every month because the Earth’s orbit around the sun is not in the same plane as the moon’s orbit around the Earth. Do not spend more than 2-3 minutes on the activating strategy. If students are struggling with the answers, let them know that by the end of the lesson, they should have a better understanding of eclipses and move into the lesson.

Instructional Approach(s): The teacher should use the diagrams to demonstrate that the Earth’s orbit plane is different from the moon’s orbit plane; therefore, the moon is not always in the position to cause eclipses.

Use the Eclipse Notes Instructional Approach(s): The teacher should give each student an Eclipse Notes sheet and instruct the students to use the Notes sheet to record important information throughout the lesson.

There are two types of Eclipses: Solar Eclipse Lunar Eclipse Instructional Approach(s): The teacher should start off by reading the statement “there are two types of eclipses”. Ask the class or call on students to identify the two types of eclipses. Once students have responded, click to reveal the two eclipses.

Solar Eclipse When its orbit around Earth takes the Moon directly between Earth and the Sun, the Moon blocks our view of the Sun in what we call a solar eclipse. *In short, the moon passes between the Earth and Sun causing the Earth to pass through the Moon’s shadow. Depending on where you are on Earth, you may experience a total eclipse or a partial eclipse. Instructional Approach(s): The teacher should present the characteristics of a solar eclipse on the slide while the students describe a solar eclipse on their notes.

Solar Eclipse Penumbra Umbra The Moon's faint outer shadow. Partial solar eclipses are visible from within the penumbral shadow. Umbra The Moon's dark inner shadow. Total solar eclipses are visible from within the umbral shadow. http://www.mreclipse.com/Special/SEprimer.html Instructional Approach(s): The teacher should present the characteristics of a solar eclipse on the slide while the students describe a solar eclipse on their notes.

Solar Eclipse Occur two to four times a year Instructional Approach(s): The teacher should present the characteristics of a solar eclipse on the slide while the students describe a solar eclipse on their notes.

Diagrams of a Solar Eclipse Instructional Approach(s): The teacher should use the diagrams to illustrate the position of the Earth, Sun, and Moon during a solar eclipse. Be sure to discuss how and why only parts of the Earth experience the total and partial solar eclipse.

Animations of a Solar Eclipse http://ww2.valdosta.edu/~cbarnbau/astro_demos/frameset_moon.html http://www.classzone.com/books/earth_science/terc/content/visualizations/es2505/es2505page01.cfm?chapter_no=visualization Instructional Approach(s): The teacher should show the animations of a solar eclipse to reinforce the concept.

In the space provided on your notes, draw a simple diagram showing the position of the Sun, Moon, and Earth during a solar eclipse. Instructional Approach(s): Give the students a few minutes (no more than 2 minutes) to draw a simple diagram showing the position of the Sun, Moon, and Earth during a solar eclipse. The students may start out with just the positions shown. After a few minutes, click to show the simple diagram on the slide. You may want students to go back and illustrate the shadow part too.

Lunar Eclipse

Lunar Eclipse *A Lunar Eclipse occurs when the moon passes through the Earth’s shadow. Depending on where the moon crosses Earth’s shadow, the top or bottom will appear darker. The reddish color is from sunlight refracted by Earth’s atmosphere onto the moon. Instructional Approach(s): The teacher should present the characteristics of a lunar eclipse on the slide while the students describe a lunar eclipse on their notes.

Lunar Eclipse Penumbral Lunar Eclipse (click for photo example) The Moon passes through Earth's penumbral shadow. These events are of only academic interest because they are subtle and hard to observe. (click for photo example) Partial Lunar Eclipse A portion of the Moon passes through Earth's umbral shadow. These events are easy to see, even with the unaided eye. Total Lunar Eclipse The entire Moon passes through Earth's umbral shadow. These events are quite striking due to the Moon's vibrant red color during the total phase (totality). Instructional Approach(s): The teacher should present the characteristics of a lunar eclipse on the slide while the students describe a lunar eclipse on their notes.

Lunar Eclipse Occur two to four times a year Instructional Approach(s): The teacher should present the characteristics of a solar eclipse on the slide while the students describe a solar eclipse on their notes.

Lunar Eclipse Instructional Approach(s): The teacher should use the diagrams to illustrate the position of the Earth, Sun, and Moon during a lunar eclipse. Be sure to discuss how and why only parts of the Earth experience the total and partial lunar eclipse.

Video Clips and Animations of a Lunar Eclipse http://www.neok12.com/video/Eclipse/zX027e52507b754877644063.htm http://ww2.valdosta.edu/~cbarnbau/astro_demos/frameset_moon.html Instructional Approach(s): The teacher should show the animations of a lunar eclipse to reinforce the concept. http://ww2.valdosta.edu/~cbarnbau/astro_demos/frameset_moon.html

In the space provided on your notes, draw a simple diagram showing the position of the Sun, Moon, and Earth during a solar eclipse. Instructional Approach(s): Give the students a few minutes (no more than 2 minutes) to draw a simple diagram showing the position of the Sun, Moon, and Earth during a lunar eclipse. The students may start out with just the positions shown. After a few minutes, click to show the simple diagram on the slide. You may want students to go back and illustrate the shadow part too. http://www.mreclipse.com/Special/LEprimer.html

Distributed Summarizing With an elbow partner, describe the difference between a solar eclipse and a lunar eclipse. Instructional Approach(s): The students should answer the distributed summarizing question with a partner. Partners can be determined by the students or the teacher can provide more specific directions such as turn to the person directly in front/behind you or to the right/left of you, etc. It may be necessary to have a group of three if you have an uneven number of students. Do not allow more than 1 minute of discussion time. The teacher should be walking around listening and redirecting discussions as needed. Once students have been given 2 minutes or less to discuss solar and lunar eclipses, click to the next slide.

Lunar Eclipses happen when the Moon passes through Earth’s shadow, whereas solar eclipses happen when Earth passes through the Moon’s shadow. Instructional Approach(s): The teacher should use the slide to review the differences between a solar eclipse and a lunar eclipse.

Summarizing Strategy [see resources] Instructional Approach(s): Each student should complete the summarizing strategy. The teacher should review each summarizer to determine the level of student mastery to determine if differentiation is needed.