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International Shadow Trackers This investigation funded in part through an IDEAS grant from the Space Science Telescope Institute with funding from NASA
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More Information About Solstices and EquinoxesBecause the Earth is tipped compared to the Sun, the Northern and Southern hemispheres of the Earth alternately tip toward and away from the Sun. This causes the Sun, Moon, and planets and stars as observed at noon or midnight (i.e. halfway between rising and setting) to look like they move North and South during the year. Then, twice each year, they stop and reverse direction in repeating cycles. These apparent motions of the Sun and full Moon are caused because the tipped Earth is moving (revolving) around the Sun. The length of one year is determined by the time it takes the Earth to move around the Sun once. Astronomers have invented names to describe the position of the Sun (and also Full Moon) during this annual cycle. Solstices are the times when the Sun (and full Moon) appears furthest North or South and Equinoxes are times when the Sun (and full Moon) appears halfway between the North and South. Solstice gets its name from the apparent movement of the Sun and essentially means “the Sun is standing still.” The solstices are when the Sun appears to stop and change directions. They usually happen on June 20 or 21 and December 21 or 22 of each year. In the North, Summer Solstice (the beginning of summer) is in June and Winter Solstice (the beginning of winter) is in December. In the South, Summer Solstice is in December and Winter Solstice is in June. These are times when the Earth has both the longest and shortest days. When people living in the Northern Hemisphere have the shortest day, and thus the beginning of winter, the people in the Southern Hemisphere have the longest day and thus the beginning of summer. Equinox means “equal nights.” Every place on the Earth has equal times of night and day during an equinox. This is the time that the Sun (and full Moon) is half way through its apparent movement between furthest South and furthest North. The Vernal Equinox is the beginning of spring in the North or fall in the South and usually happens on March 20 or 21 when the Sun appears to be moving slightly northward each day. The Autumnal Equinox, also the beginning of spring or fall, usually happens on September 22 or 23 when the Sun appears to be moving southward. An interesting aspect of a equinox is that the sun is rising at one of the Earth’s poles and setting at the other pole – and the poles begin a 6-month long period of day or night. The time of the Vernal Equinox in March is especially important because this is the astronomical beginning of a new year and the basis for determining the length of a year. To really understand these motions, the changes we observe, and the cause of the seasons, we need to make observations over at least one year.
Reference Websites
Learning StandardsThe following are some examples of some learning standards that support this investigation: Earth and Space Science: Arizona Grade 5:
Arizona Grade 7:
Ohio Grade 5:
Ohio Grade 8:
Scientific Inquiry and/or Scientific Ways of Knowing: Arizona Grade 5:
Arizona Grade 7:
Ohio Grade 5:
Ohio Grade 8:
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