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Space Today Script Version 6/19/2017 12:00:00 PM Media Script Space Today Logo ----(After music is over, step on foot pedal to zoom in camera and brighten lights.) Good afternoon. This is Space Today, XXXXX reporting. Opening Title and Music ----- Today we are going to talk about Archaeoastronomy. Archaeoastronomy is: • The investigation of the astronomical knowledge of prehistoric cultures. • Archaeoastronomy is the study of how people in the past “have understood the phenomena in the sky, how they used these phenomena and what role the sky played in their cultures.” Archaeoastronomy Title Today astronomers use sophisticated instruments and observatories to study and measure the Sun, planets, stars and much, much more. Ancient peoples watched the skies as well, building observatories such as Stonehenge and recording movements of planets and stars for hundreds of years. Observatory photo Archaeoastronomy definition Stonehenge P 1 of 8 p2 of 8 Script Today we are going to learn about the astronomical observations made by the Maya and the tools they used to make these observations, such as this observatory at Chichen Itza (Cheechin-eat-Za). The Maya of the Classic Period lived in Mesoamerica in the countries of Mexico, Honduras, Guatemala, and Belize. The Classic Period lasted from 250 – 900 AD and during this time the Maya made many important astronomical observations. Their observations were important for their calendar, agricultural planting cycles, ceremonial and religious festivals and planning dates for battles. One important star for the Maya was the sun. The Sun was very important to the ancient Maya. The Maya Sun God was Kinich Ahau (Kin-eesh Ahhow). They tracked the movements of the sun over hundreds of years and were able to make predictions, all without the aid of modern technology. How exactly did the Maya make such accurate measurements without telescopes? Media El Caracol Observatory at Chichen Itza Mesoamerica Map Sun and Glyph p3 of 8 Script Let’s travel to the site of Caracol (Cara-cole) in Belize. This group of buildings is called the “E-group” by archaeologists. E groups were designed to map the movement of the sun at the equinoxes and solstices. By tracking the movement of the sun as it would rise the Maya were able to determine things such as the cardinal directions (North, South, East and West) as well as the solstices and the equinoxes. The Maya had glyphs for each of the cardinal directions and the determination of these directions was important for ceremonial and religious purposes. Media E- Group at Caracol E- group diagram with all 3 sun locations Cardinal Direction Glyphs p4 of 8 Script The solstices are the days with the most time between sunrise and sunset or with the least time between the two. The summer solstice is the day with the most time between sunrise and set. And the winter solstice is the day with the least. A Maya observer watching from the same location over many years would have noticed that the sun does not rise in the same location every day. The sun always rises in the east and on the summer solstice it rises in its most northeast position. We used our Sundial Exploration Station to create this birds-eye view of the sun rise on the summer solstice as the Maya people at Caracol (Cara-cole) would see it. These white buildings represent the buildings of the E-Group. The orange pole is our Maya observer. Notice the southwest direction of the shadow being cast by the sun of our observer. The winter solstice is the day of the year with the least amount of time between sunrise and sunset. On the winter solstice, the sun rises in its most southeast position. Media Graphic of sunrise at E-group on summer solstice Sundial image of summer solstice Graphic of sunrise at E-group on winter solstice p5 of 8 Script From our birds-eye view we can see that the sun is now casting the observer’s shadow in a northwest direction. On the two equinoxes day and night are of equal length; around 12 hours. Twice a year on the equinoxes the sun rises directly in the east. Again from our birds-eye view we can see that the sun is casting the observer’s shadow directly west. The tropics are the band around the equator where the sun will pass directly overhead. We call the position in the sky directly overhead the Zenith. This occurs from 23.5° north of the equator to 23.5° south of the equator. The location of the Maya in the tropics allowed them to make very accurate measurements of solar cycles because the sun passes directly overhead at high noon twice a year. Media Sundial image of winter solstice Graphic of sunrise at E-group on winter solstice Sundial image of winter solstice Tropic latitude graphic p6 of 8 Script The accomplishments of these early astronomers seem incredible, but what they lacked in sophisticated technology, they made up by patient observing over long periods of time and simple instruments such as the zenith tube. By observing the sun through the zenith tube on the two occasions a year that it passes directly overhead, very accurate timing could be achieved. On the left is a vertical zenith sighting tube from the site of Xochicalco (Show-she-cal-co) in Mexico. On the right is the structure that allows access to its other end underground. Careful observation would have set the sun-transit time to a minute or so. Returning to our birds-eye view, we can see that on the summer solstice and winter solstice the sun would cast a shadow down the zenith tube at high noon. Twice a year at high noon the sun would be directly overhead, shining down with no shadow on the zenith tube. These two events would be equal spaced in time around the summer solstice. Media Zenith tube image Sundial image Xenith Solstices Sundial image Xenith Equinox p7 of 8 Script The Maya were able to make incredibly accurate measurements of astronomical cycles just with these simple techniques. By comparing the records of the Maya against our modern calculations we notice that Maya calculations are extremely accurate. Note that they knew the year to within 2 seconds of its actual time. You too can observe the sun, moon and other objects in the sky in your own backyard without a telescope or other equipment. Stand in the same place every day at sunrise for a few weeks and record your observations of where the sun rises. Remember; never look directly into the sun. Explore our Sundial Exploration Station to learn more about the movements of the sun and what you can observe in your own backyard. Don’t forget to check out our current temporary exhibition, Maya: Hidden Worlds Revealed while you are here to learn more about the Classic Period Maya. In the exhibit you can see over 250 spectacular artifacts, print your birthdate in Maya glyphs, build a corbeled arch, and much more. Media Maya observations of sun, lunar and Venus cycles vs. modern calculations Sunrise over city Sundial Exploration Station Maya exhibit slide p8 of 8 Script And that’s this episode of Space Today! Media Credits