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In the Moon Time |
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| Summary: By observing and recording information about the moon's
phase and position in the sky over a 5 week period, students can begin the
study of astronomy as it was anciently studied before the invention of telescopes.
They will then use models to explain their observations. You can also relate
the moon phases to the tides of the ocean and how they affect life in the
oceans.
Category: Learning cycle Learning Objectives:
Materials:
Sequence and duration of each part of lesson: This module is intended as an introduction. Students will individually observe and record information about the Moon's phase and position in the sky at different times of night over a 5 week period. They will work in teams to compile this data and develop a model to demonstrate the apparent motion and change of phase of the Moon. They should be able to design their own data table and schedule their own observations. This same data could be obtained from almanacs or calendars that show moon phases or from computer programs. A shareware program called Skyglobe allows you to set dates and times and watch the moon move across the sky. But these sources would best be used as supplements to the students' observations. There is no substitute for direct observation. Exploration Phase: Assign students to record data on the appearance of the Moon and its position in the sky at different times of the night. Allow students to determine how they will record data. Note that the moon sometimes rises very late. Some observations can be made early in the morning or even during daylight. If the moon was not up when students went to bed, it will probably still be up when they leave for school. After about 3 days of observations, allow class time for discussion and comparison of the data charts in use. Students may benefit from comparing charts and data in teams of 3 or 4. Ask whether other students have recorded data that seems significant that they didn't think to record. Possible data include time of moon rise, height above the horizon at a fixed time, constellation the moon is near, phase, and which edge of a crescent moon is lighted. Within their teams, students may want to arrange taking turns making observations and getting together later to compile data. (Optional) After at least 1 week of observations, Introduce the Skyglobe program and make copies available to those who can use it on their computer. This program shows the position of sun, moon, stars, and planets at any date as seen from many locations. The view can be rotated and set to move ahead in steps. Special Computer Management Consideration: Take precautions against introducing viruses to your system when making copies of Skyglobe shareware. Copy to new or cleared disks. Mention the project frequently over the next month. Invention Phase : (At end of 5 weeks)
Challenge each team to set up a demonstration of the relative motion of the Earth, moon, and sun that will fit their observations and can be used to demonstrate the answer to several of the questions above. [Note that their model does not have to agree with current astronomic theory.] Expansion Phase Discuss the following:
Bring the exercise to closure by making sure all students can explain current theory using their model. Evaluation: will be based on individual data charts and on team models and final explanations. On data charts look for a complete and well organized table of observations. Note any unique observations other students do not have. On the model look for clarity of the explanation and participation of all team members. Related Resources: One source for Skyglobe shareware that is guaranteed virus free is the Software Lab, 1-800-359-9998. |
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