APS 1030 Laboratory 1 Motions of the Sun MOTIONS OF THE SUN SYNOPSIS: The objective of this lab is to become familiar with the apparent motions of the Sun in the Boulder sky. EQUIPMENT: A globe of the Earth, a light box. Part I. Daily Motion of the Sun The daily motion of the Sun is caused by the Earth’s rotation rather than the Sun actually moving across the sky. (A subtle point! It took civilization thousands of years to figure this out!) The diagram below show an overhead view of the Earth and Sun: We will now follow a person (the stick figure) as the Earth rotates. At point ‘A’ our viewer is rotated into view of the Sun, and the Sun appears to rise (i.e. sunrise!) Noon is defined as the time when the viewer is located at point ‘B.’ This is the point where the Sun will be at its highest point in the sky. At point ‘C’ our viewer is being rotated out of view of the Sun, and he or she sees sunset. Midnight is defined as point ‘D’; the point opposite Noon. The Sun at points ‘A’, ‘B’ and ‘C’ as seen on Earth are shown below: APS 1030 Laboratory 2 Motions of the Sun In the next part you will use the globe and light box: I.1 Put the globe at one end of the table. At the other far end position the light box such that it is illuminating the globe; the light box will simulate the Sun. Find Boulder on the globe; and position the globe such that Boulder (latitude 40°, longitude 105°) is facing the light box (at position ‘B’, i.e. Noon.) Orient the globe such that the Earth’s axis is pointing 90° (in either direction) away from the light box. In a moment you will see that this orientation represents the equinoxes; on these days the Northern and Southern hemispheres each receive 12 hours of sunlight. What fraction of the Earth is illuminated? I.2 At the time Boulder is at Noon: • What major cities are experiencing sunrise and sunset? (pick one for each.) • What country is at the same latitude as Boulder but on the other side of the globe? • What time is it there? • What are the people of Tibet doing right now? • Are the Honda Corporation offices in Tokyo likely to be open at this moment? I.3 Rotate the globe such that Boulder is now at sunset. How much of the Earth is illuminated now? What time is it now for the country on the other side of the globe? Part II. The Annual Motion of the Sun The position of the Sun in the sky also changes as the Earth orbits around the Sun. This motion is not to be confused with the daily motion of the Sun described above! The Earth’s axis is tilted 23.5° with respect to the perpendicular of its orbital plane (see diagram below). As a consequence different parts of the Earth receive different amounts of sunlight depending on where the Earth is in its orbit. Note: the orbit is circular, but it is shown here in projection: Due to the Earth’s tilt the northern hemisphere receives more light during the summer months; and less light during the winter. The Sun also rises higher in the sky during the summer; and this direct sunlight is more warming. These two effects cause the summer to be warmer than the winter. The summer is not warmer than the winter because the Earth is closer to the Sun; in fact, the Earth is slightly closer to the Sun during the Northern hemisphere's winter! The Sun’s path across the summer and winter sky is shown on the next page. Note that the winter Sun does not rise as high; nor is it up for as long: APS 1030 Laboratory 3 Motions of the Sun If you were to measure the position of the Sun every day at Noon over the span of a year, you would notice that it slowly moves up and down with the seasons. For example, on June 21st the Sun at Noon is at its highest, northernmost position, while on December 22nd the Sun is at its lowest, southernmost position. These days are called the summer and winter solstices respectively. Solstice literally means “Sun stop”; on those two days the Sun appears to stop moving and change directions (e.g. on the Summer solstice the Sun stops moving to the North and starts to descend to the South.) The illustration above shows the Earth at the summer solstice. Position your globe such that Boulder is at Noon and it is the Summer solstice. From the globe and the illustration above answer the following questions: II.1 What direction do the stars rotate around Polaris, the “North Star”, as seen from the Northern hemisphere. Do they go around clockwise or counter-clockwise? II.2 Go to the country at the same latitude as Boulder but on the other side of the globe. What country is this? What season is this part of the world in? II.3 Now go back to Boulder. Follow the 105° meridian south to a latitude of 40° south. What is there? You should find Easter Island just to the north. (Did you notice South America is much farther east than the U.S.?) What season is this part of the world in? APS 1030 Laboratory 4 Motions of the Sun II.4 Finally, find the antipode to Boulder - the point directly opposite on the globe, through the center of the Earth. (Hint: It is not China!) II.5 The Tropic of Cancer marks the northernmost points where the Sun can be seen at the zenith (i.e. directly overhead) respectively. On the summer solstice anyone standing on the Tropic of Cancer will see the Sun overhead at Noon. Is there anywhere in the United States where you could see the Sun at the zenith? II.6 The Arctic Circle marks the northern region of the Earth where the Sun is sometimes, always (or never!) visible. Find the town of Barrow, Alaska. On the summer solstice at what times will the Sun rise and set here? Part. III: The Southern Hemisphere Without changing the orientation of the globe study what is happening “down under” in Australia. III.1 On the Northern hemisphere's Summer solstice is the Sun to the North or South? What season is Australia experiencing? Would this be a good time to ski the Snowy Mtns. in New South Wales? III.2 The Tropic of Capricorn marks the southernmost point at which the Sun can be seen at zenith. Look at the town of Alice Springs in the center of Australia. Is the sun ever directly overhead in Alice Springs? If so, when? III.3 The Antarctic Circle is the southern equivalent of the Arctic Circle. On our summer solstice what time does the Sun rise at the South Pole? III.4 In Australia, do the stars rise in the east and set in the west? Which way do the stars revolve around the south celestial pole? Part IV: Thought Question Everybody knows it's colder in December than in July (a tleast in the northern hemisphere!), but why? Is it because of a change in the number of daylight hours? The height of the Sun above the horizon? The "intensity" of the sunlight? Or are we simply closer to the Sun in the summer than in winter? IV.1 How might you figure out the reason for seasons? What observations might you make over a year at the north pole, south pole, and equator? Medieval Noon mark from Bedos de Celles, La Gnomonique pratique (Paris, 1790), a book on the use of sundials. If you look carefully at the shadows you may notice that the artist has made a mistake.
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