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Transcript
mOON cHART tEACHER GUIDE Curriculum linked to ‘A Curriculum for Excellence’ Science - Planet Earth - Space Suitable for S2-S6 pupils. By charting the motion of the Moon pupils will enhance their understanding of the relative motion within our solar system. In particular, pupils will investigate the motion of the Moon across the sky along with why we observe different phases of the Moon. Discussion Questions Things to consider • Several factors must remain constant: location, time and frame of reference. • The Moon may not be observable every evening when observing the night sky at the same time each day. • • The calendar shows dates when the Moon is visible from Glasgow between 6pm and 10pm. Starting the activity on one of these dates will ensure that as pupils begin the activity they will be able (weather permitting) to observe the Moon at their chosen time (between 6pm and 10pm). To guarantee that a full cycle of the Moon is observed, the experiment should run for a minimum of 30 days. • Pupils may require more than one worksheet or sheet of paper to complete their diagram. For younger pupils it may be helpful to suggest they start by drawing their first sketch of the Moon on the right hand side of their paper. • Depending upon the age/ability of the class, the ‘other things to try’ section of the pupil worksheet may be useful. Use our ‘Star Maps’ activity (available on Glasgow Science Centre’s website) to help pupils identify specific constellations. www.glasgowsciencecentre.org/moonchart.aspx example Can you explain why the Moon appears to change shape? Can you track the Moon for the whole month? Does the Moon follow a path or does it appear to wander around the sky? Does the Moon sometimes appear larger or smaller in the sky? Does the Moon only appear at night? Why? What is a Lunar Eclipse? Is that the same as a Solar Eclipse? Does it happen every month? Why? The Moon orbits around the Earth but does the Moon rotate on its axis? What evidence do you have to support your answer? useful information Path of the moon Like the Sun, the Moon rises and sets every day. It too rises in the East and sets in the West. However, the Moon may appear in the sky at night, or during the day. We often don’t think of the Moon as being in the sky during the day since it’s difficult to see because the Sun is so much brighter. Moon Phases A common misconception is that the phases of the Moon are created by the shadow of the Earth. In fact, it is the relative positions of the Sun, Moon and Earth that creates the appearance of changes in the shape of the Moon. Lunar Eclipses As the Moon orbits the Earth, it occasionally passes through the Earth’s shadow. It doesn’t happen every month but it does happen a few times each year. This event is known as a Lunar Eclipse. During a lunar eclipse, the Moon may appear to change colour - anything from grey to a bright red colour may be observed. No two lunar eclipses are the same. A Solar Eclipse, on the other hand, occurs when the Moon blocks sunlight from reaching the Earth. The apparent path of the Sun around the sky is known as the ecliptic. The Moon follows the general path of the ecliptic but spends half it’s journey around the Earth above the ecliptic and half below. It takes the Moon 29.5 days to complete its orbit around the Earth (known as a synodic period) but 27.3 days between full moons (known as a sidereal period). That means that a full moon doesn’t appear in the same location every time. It also takes the Moon 27.3 days to spin on its axis which creates synchronous rotation; meaning that the same side of the Moon always faces the Earth. Copyright © 2008 Glasgow Science Centre