General Astronomy: Lecture 2 - The Ancient Views of the Heavens

Spahn's Science Lectures
1 Jun 201726:24

Summary

TLDRThis astronomy lecture explores the evolution of human understanding of the cosmos, from ancient civilizations' practical uses of astronomy for timekeeping and navigation to the development of the geocentric model by ancient Greeks. It highlights how observations led to the realization that Earth is a planet in a vast universe and discusses the contributions of figures like Pythagoras, Plato, Aristotle, and Ptolemy in shaping early astronomical theories.

Takeaways

  • 🌌 Astronomy is one of the oldest sciences, with roots stretching back to antiquity.
  • 🌍 Ancient civilizations had practical reasons for studying astronomy, such as timekeeping, seasonal changes, and navigation.
  • 🌜 People in central Africa could predict rainfall patterns by observing the orientation of the waxing crescent moon.
  • πŸ“… Our modern measurements of time, like the day, month, and year, are based on astronomical observations.
  • 🌞 The seven days of the week were named after the seven planets of ancient times, including the Sun and the Moon.
  • πŸ•°οΈ Ancient cultures used simple tools like Sun dials and obelisks to tell time by observing the Sun's path.
  • πŸ—Ώ Structures like Stonehenge and the Templo Mayor were built to mark astronomical events and align with celestial bodies.
  • 🌐 The geocentric model, which placed Earth at the center of the universe, was developed by Greek philosophers over several centuries.
  • πŸ“‰ The Ptolemaic model, a geocentric system, was able to predict planetary positions with reasonable accuracy and was used for over 1500 years.
  • πŸš€ The transition from the geocentric to the heliocentric model marks a significant shift in our understanding of the universe, moving towards modern science.

Q & A

  • What is the significance of ancient astronomy in understanding the cosmos?

    -Ancient astronomy is significant because it represents the earliest systematic observations of the sky and the development of the first scientific models to explain celestial phenomena. It laid the foundation for modern astronomy and our understanding of the universe.

  • How did ancient cultures use astronomy for practical benefits?

    -Ancient cultures used astronomy for practical benefits such as timekeeping, tracking seasonal changes, and navigation. For example, people in central Africa predicted rainfall patterns by observing the moon's orientation.

  • What is the origin of the seven-day week in relation to astronomy?

    -The seven-day week originates from the seven planets of ancient times, which included the Sun, the Moon, and the five planets visible to the naked eye: Mercury, Venus, Mars, Jupiter, and Saturn. Each day was named after one of these celestial bodies.

  • How did the ancient Egyptians use the Sun to tell time?

    -The ancient Egyptians used the Sun's path across the sky to tell time. They likely used simple Sun dials based on the shadows cast by sticks and built obelisks that may have served as large, accurate timekeeping devices.

  • What is the significance of Stonehenge in the context of ancient astronomy?

    -Stonehenge is significant because it was used as an astronomical device to mark the seasons and as a social and religious gathering place. It has alignments that correspond to the Sun's position on the summer solstice.

  • How did the Aztecs use astronomy in their Templo Mayor?

    -The Aztecs used the Templo Mayor, with its twin temples on a pyramid, to align with the Sun's position on the equinoxes. From a royal observer's vantage point, the Sun would rise through the notch between the temples on the fall and spring equinoxes.

  • What is the major lunar standstill and how was it observed at the Sun Dagger site?

    -The major lunar standstill is an 18.6-year cycle where the full moon reaches its most southerly point along the eastern horizon. At the Sun Dagger site, this event was marked by the shadow of the full moon passing through slabs of rock to light the edge of a spiral.

  • What was the geocentric model of the universe, and why was it significant?

    -The geocentric model placed the Earth at the center of the universe, with all celestial bodies moving around it. It was significant because it was the dominant model in Western thought for almost two thousand years and was the culmination of many Greek philosophers' and astronomers' observations and theories.

  • Who was Claudius Ptolemy and what was his contribution to the geocentric model?

    -Claudius Ptolemy was a Greek astronomer whose geocentric model, known as the Ptolemaic system, adapted and synthesized earlier ideas into a single system that agreed well with astronomical observations at the time. His model could predict planetary positions with reasonable accuracy and was used for over 1500 years.

  • What was the role of Aristotle in the development of the geocentric model?

    -Aristotle contributed to the geocentric model by arguing that gravity pulled heavy things toward the center of the universe, forming a spherical Earth. He also believed in celestial spheres responsible for the motion of celestial bodies, reinforcing the idea of an Earth-centered universe.

Outlines

00:00

🌌 Introduction to General Astronomy

The paragraph introduces the viewer to general astronomy, highlighting the ancient views of the cosmos and how our understanding has evolved. It emphasizes the Earth's status as a planet orbiting an ordinary star within a vast universe. The lecture aims to explore how we've learned about the universe through careful observation, which has been ongoing for thousands of years. Ancient civilizations had practical uses for astronomy, such as timekeeping, seasonal tracking, and navigation. An example is given of how people in central Africa predicted rainfall patterns by observing the moon's orientation. The paragraph also discusses how the length of our day, month, and year are derived from astronomical observations, and how the seven days of the week are named after the seven planets known to ancient civilizations.

05:00

πŸ•°οΈ Ancient Timekeeping and Astronomy

This section delves into how ancient cultures used astronomy for timekeeping, with the origins of our modern clock traced back to ancient Egypt. The Egyptians divided the day and night into twelve equal parts, leading to our AM and PM system. The paragraph discusses various ancient structures like Stonehenge and the Aztec Templo Mayor, which were used to mark the seasons and perform astronomical observations. It also mentions how many cultures aligned their buildings with cardinal directions to track the Sun's movement. The Sun Dagger, a feature created by ancestral Pueblo people in New Mexico, is highlighted as an example of a structure used to mark the Sun's positions on special dates like the solstices.

10:03

πŸ”­ The Accuracy of Ancient Observations

Paragraph 3 discusses the importance of accurate, repeatable observations in ancient astronomy and how they laid the groundwork for modern science. It explains how structures like Stonehenge or the Templo Mayor required meticulous observation to be built with such precision. The paragraph also touches on the rise of ancient Greek civilization and its contributions to science, including the development of the geocentric model of the universe. A timeline of important figures in the development of the geocentric model is provided, emphasizing the gradual refinement of astronomical understanding over centuries.

15:05

🌐 The Development of the Geocentric Model

This paragraph traces the development of the geocentric model of the universe, which placed Earth at the center. It starts with the philosopher Thales, who first proposed a non-supernatural explanation for the universe's composition, and continues through the contributions of Anaximander, Pythagoras, Plato, Eudoxus, Aristotle, and finally Ptolemy. Each figure built upon the ideas of the previous, refining the model to better match observations. The paragraph explains how the geocentric model, despite being incorrect, was a significant step forward in scientific understanding because it was based on observations and could predict planetary positions with reasonable accuracy.

20:06

πŸ’« Retrograde Motion and the Ptolemaic System

The paragraph discusses the challenge of retrograde motion, where planets appear to move backward in the sky, and how it was explained within the geocentric model. It introduces the concept of 'epicycles' and 'deferents' used by Apollonius to explain these motions. The paragraph also details how Ptolemy synthesized earlier ideas into the Ptolemaic model, which could predict planetary positions with remarkable accuracy for its time. This model, despite being based on the incorrect assumption that Earth was the center of the universe, remained in use for over a millennium.

25:11

🌞 Transition to the Heliocentric Model

The final paragraph sets the stage for the next lecture, which will discuss the Copernican revolution that shifted the model of the universe from the geocentric to the heliocentric system, with the Sun at the center. It reflects on the durability of the geocentric model and the challenge of scientific paradigm shifts, emphasizing the importance of questioning established beliefs and continually seeking to align our understanding with observations.

Mindmap

Keywords

πŸ’‘Astronomy

Astronomy is the scientific study of celestial objects, space, and the physical universe as a whole. In the context of the video, astronomy is portrayed as the oldest of the sciences, with roots stretching back to antiquity. It is highlighted by the careful observations of the sky that have been ongoing for thousands of years, indicating its significance in understanding the cosmos and our place within it.

πŸ’‘Celestial Sphere

The celestial sphere is an ancient concept that refers to an imaginary sphere with the Earth at its center, upon which all celestial bodies are thought to be attached. Anaximander is credited with inventing this idea. In the video, the celestial sphere is mentioned as a key development in early astronomical models, showing how ancient civilizations began to understand the relative positions of celestial bodies.

πŸ’‘Geocentric Model

The geocentric model is a now-disproven description of the universe with Earth at the center and all celestial bodies, including the Sun, Moon, and stars, orbiting around it. The video discusses how this model developed gradually over several centuries and was a dominant view until the Copernican heliocentric model was proposed. It illustrates the progression of human understanding of our place in the universe.

πŸ’‘Retrograde Motion

Retrograde motion refers to the apparent backward movement of a planet against the backdrop of other stars, as viewed from Earth. This phenomenon was a challenge to the early geocentric model and is explained in the video as a reason for the development of more complex models, such as the Ptolemaic system, which used epicycles to account for these observations.

πŸ’‘Epicycles

Epicycles are small circles in which celestial bodies were thought to move while those circles themselves revolved around a larger circle (deferent). This concept was developed by Apollonius and is discussed in the video as a method to explain the retrograde motion of planets within the geocentric model.

πŸ’‘Copernicus

Copernicus is mentioned in the video as a pivotal figure in the shift from the geocentric to the heliocentric model of the solar system. His work is a stepping stone towards modern astronomy and represents a significant shift in understanding the structure of the solar system.

πŸ’‘Ptolemy

Ptolemy was a Greek astronomer whose geocentric model, known as the Ptolemaic system, was widely accepted for over a thousand years. The video describes his model as a significant accomplishment in synthesizing earlier ideas into a system that could predict planetary positions with reasonable accuracy.

πŸ’‘Stonehenge

Stonehenge is a prehistoric monument known for its alignment with the movements of the sun. In the video, it is used as an example of how ancient cultures used astronomical observations for practical purposes, such as marking the seasons and serving as a gathering place.

πŸ’‘Aztec

The Aztec civilization is mentioned in relation to the Templo Mayor, a structure aligned with celestial events. This example from the video highlights how ancient cultures used astronomy for religious and ceremonial purposes, indicating the widespread significance of astronomy across different civilizations.

πŸ’‘Precession

Precession, specifically the precession of the moon's orbit, is a concept touched upon in the video. It refers to the slow westward shift of the moon's nodes, which takes approximately 18.6 years to complete a cycle. The Sun Dagger, a petroglyph created by the ancestral Pueblo people, is mentioned as a structure that may have marked this lunar cycle.

πŸ’‘Observational Science

Observational science is emphasized in the video as the foundation of astronomy. It involves making careful, repeatable observations of the sky to gather data and understand celestial phenomena. This approach is highlighted as a precursor to modern scientific methods, showing the video's theme of the evolution of scientific thought.

Highlights

Astronomy is considered the oldest of the sciences with roots stretching deep into antiquity.

Ancient civilizations practiced astronomy for practical benefits such as timekeeping, seasonal changes, and navigation.

People in central Africa predicted rainfall patterns by observing the orientation of the waxing crescent moon.

The length of our day, month, and year, as well as the seven days of the week, have astronomical roots.

Ancient cultures used the Sun's path and shadows to tell time, like the ancient Egyptians with obelisks.

Stonehenge was used as an astronomical device and a social and religious gathering place.

The Aztec city featured the Templo Mayor, where the Sun rose through the notch between the temples on the equinoxes.

Many cultures aligned their buildings and streets with the cardinal directions to track the Sun's positions.

The Sun Dagger in New Mexico marked the sun's positions on special dates like the winter or summer solstice.

Ancient observations led to the development of modern science, with elements present in many early human cultures.

Greek philosophers developed a tradition of understanding nature without relying on supernatural explanations.

The Greeks used mathematics to give precision to their ideas about the universe.

Aristotle's geocentric model dominated Western thought for almost two thousand years.

Ptolemy's model could predict planetary positions within a few degrees of arc, keeping it in use for the next 1500 years.

The geocentric model, although incorrect, was a way of explaining observations and a part of scientific progress.

The next lecture will discuss the Copernican revolution, moving from the geocentric to the heliocentric system.

Transcripts

play00:00

hello and welcome to general astronomy

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lecture to the ancient views of the

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heavens today we know that the earth is

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a planet orbiting a rather ordinary star

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and a galaxy more than 100 billion stars

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that is in an incredibly vast universe

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we know that the earth along with the

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entire cosmos is in constant motion we

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also know that on the scale of cosmic

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time human civilization has existed for

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only the briefest moment how do we come

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to learn these things so that's what

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we'll look at today careful observations

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of the sky have been going on for many

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thousands of years astronomy has been

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called the oldest of the sciences

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because its roots stretch deepest into

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antiquity ancient civilizations did not

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always practice astronomy in the same

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way or for the same reasons that we

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study it today but nonetheless had some

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amazing achievements understanding this

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ancient astronomy can give us a greater

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appreciation of how and why science

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developed through time interest in

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astronomy likely stems due to parts of

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our fundamental curiosity but ancient

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cultures also had discovered that

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astronomy had practical benefits for

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timekeeping keeping track of seasonal

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changes and navigation one amazing

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example comes from the people of central

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Africa although we do not know exactly

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when they developed this skill people in

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some regions learned to predict rainfall

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patterns by making careful observations

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of the moon the orientation of the horns

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of a waxing crescent moon which is the

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moon that you see in this chart relative

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to the horizon varies over the course of

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the year primarily because the angle at

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which the sun's path through the sky

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intersects the horizon that changes

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throughout the year this orientation

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also depends on latitude in tropical

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regions in which there are distinct rain

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and dry seasons rather than the four

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familiar seasons at temperate latitudes

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where we live the orientation of the

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crescent moon can be used to predict how

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much rainfall should be expected over

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coming days and weeks so you can see on

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this chart here how

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dry season is typically from October to

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February and rainy season is from March

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to September and based on that relative

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to the orientation of the moon so how

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much it's angled to the luster to the

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right they were able to use that to

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predict when the rain and dry seasons

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would be so a pretty remarkable

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achievement way back then the impact of

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ancient astronomical observations is

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still with us in our modern measurements

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of time the length of our day is the

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time it takes for the Sun to complete

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one full circuit of the sky because

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there are throat eighths in 24 hours the

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length of a month comes from the moon's

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cycle of phases so the moon cycle of

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phases takes about 29 and a half days so

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that's where a month comes from the year

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is based on the cycle of the seasons in

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other words how long it takes us to

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revolve not rotate around the Sun the

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seven days of the week were named after

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the seven planets of ancient times we

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didn't know of all the planets we know

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of now background so the seven planets

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of Asian times which were the Sun the

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moon and the five planets that are

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easily visible to the naked eye Mercury

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Venus Mars Jupiter and Saturn the

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ancient definition of planets which

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comes from a Greek word meaning wanderer

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applied to any object that appeared to

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wander among the fixed stars that is why

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the Sun in the moon were on the list

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while the earth was not because we do

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not see our own planet moving in the sky

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so back then they just considered any

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wandering object a planet so that

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wouldn't explain why the Sun and the

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moon are on there because they appear to

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be moving through the sky several of the

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English names come for dramatic come

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from with Germanic gods which you can

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see here in this table for example our

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day Tuesday comes from the Germanic God

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- Wednesday comes from voting Thursday

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from Thor and Friday from free on so you

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can kind of see where some of these

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things are coming from though

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in the daytime ancient peoples could

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tell time by observing sun's path

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throughout the sky many cultures likely

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use sticks and the shadows they cast as

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simple Sun dials the ancient Egyptians

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in fact Duty built huge obelisks often

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decorated in homage to the Sun which

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were likely served as simple clocks as

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well this ancient Egyptian obelisk that

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you see in the image which stands 83

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feet tall and weighs 331 tons resides in

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st. Peter's Square at the Vatican in

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Rome it is one of twenty one surviving

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obelisks from ancient Egypt much of what

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most of which are now scattered

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throughout the world shadows cast by the

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obelisk may have been used to tell time

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[Music]

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we can trace the origins of our modern

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clock to ancient Egypt some four

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thousand years ago the Egyptians debated

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divided daytime and nighttime into

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twelve equal parts which is how we got

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our twelve hours of each AM and PM the

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abbreviations for a.m. and p.m. stand

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for the Latin terms and meridiem and

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post meridiem respectively which means

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before the middle of the day and effort

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the middle of the day so you're starting

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to see that everything has these

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astronomical roots many ancient cultures

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built structures to help mark the

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seasons Stonehenge is a well-known

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example that served both as an

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astronomical device and as a social and

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religious gathering place the sketch on

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the right shows the archaeologists or

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how archaeologists believe that

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Stonehenge looked upon its completion at

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about 1550 BC several astronomical

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alignments are shown as they appear from

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the center for example the Sun rises

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directly over the heel stone on the

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summer solstice so the first day of

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summer so Stonehenge is actually much

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larger than what we typically see in

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photos most of it has been deteriorated

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over time but you can see for example

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that on the first day of summer the Sun

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will aligned directly over this heel

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stone and there's lots of other

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alignments as well

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so it's amazing that even way back then

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they are able to determine these things

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in the Americas one of the most

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spectacular structures was the templo

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mayor and the Aztec city of I always say

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this wrong tenor I can't say it I'm

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sorry this is going to happen a few

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times but it's modern-day Mexico City so

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pardon me for not being able to

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pronounce on these words it features

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twin temples on a flat-topped pyramid

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from the vantage point of a royal

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observer with watching from the opposite

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side of the plaza the Sun rose through

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the knotch between the temples on the

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equinoxes so that would be the fall and

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the spring equinox before conquistadors

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destroyed it Spanish visitors reported

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elaborate rituals at the templo mayor

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sometimes including human sacrifices

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that were held at times determined by

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astronomical observations so happy

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thoughts this actually happens quite a

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lot in the class we'll have a lot of

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these happy thought moments but we'll

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get through many cultures aligned their

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buildings and streets with the cardinal

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directions north south east and west

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which made it easier to keep track of

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the changing rise and set positions of

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the Sun over the course of the year this

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type of alignment is found at such

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diverse sites as the Egyptian pyramids

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the Forbidden City in China on the right

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image and among the ceremonial Kiva's

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built by the ancient ancestral Pueblo

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people of the American Southwest

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believes that ones in New Mexico they're

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in the center this large structure more

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than 20 meters in diameter is a Kiva in

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Chaco Canyon New Mexico got ahead of

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myself it was built by the ancestral

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Pueblo people approximately 1,000 years

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ago and its main axis which you see kind

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of pointing from the top left to the

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bottom right is aligned almost precisely

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north-south

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[Music]

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other structures were used to mark the

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sun's positions on special dates such as

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the winter or summer solstice many sub

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structures can be found around the world

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but one of the most amazing is the Sun

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dagger made by the ancestral Pueblo

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people in New Mexico these large slabs

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of rock lie in front of a carved spiral

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which you see there on the left and the

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right in such a way that they produce

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special patterns of light and shadow at

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different times throughout the year for

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example a single dagger of sunlight

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pierces the center of the spiral only at

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noon on the summer solstice while two

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daggers of light will bracket the spiral

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at the winter solstice so here you see

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that summer solstice where the lights at

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noon will pierce the center of the

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circle only on the summer solstice the

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first day of summer and then here on the

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right on the winter solstice you see the

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two lines of light bracketing that

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spiral only on that day the Sun Dagger

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may have also been used to mark a

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special cycle of the moon that had

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ritual significance to the end ancestral

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Pueblo people the rise in set positions

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of the full moon vary in an eighteen

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point six year cycle that's the cycle of

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precession of the moon's orbit that

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we'll get into later so the full moon

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rises at its most southerly point along

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the eastern horizon only once every

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eighteen point six years at this time

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known as a major luminal lunar

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standstill the shadow of the full moon

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passes through the slabs of rock to

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light tangent to the edge of the spiral

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in the Sun Dagger then nine point three

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years later half of that time the lunar

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shadow cuts through the center of the

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spiral the major lunar stance though can

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also be observed with structures nearby

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at chimney rock and in cliff dwellings

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at the Colorado Mesa Verde National Park

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so it's incredible already that they can

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use this to mark the first thing as

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somewhere in winter but we believe that

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it could also be used

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could have also been used to predict the

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moon's motions over a 20-year span

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almost it's incredible

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unfortunately however within just twelve

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years of the site's discovery in 1977

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the rocks had shifted so that the effect

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no longer occurs and we believe that

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these shifts were due to erosion of the

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trails below the rocks because of a

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large number of visitors so we we pretty

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much destroyed it but still at least we

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know what it is and we have visual

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evidence of what it looks like so it's a

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really remarkable feature before a

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structure such as Stonehenge or the

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temple mayor could be built careful

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observations had to be made and repeated

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over and over to ensure their accuracy

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otherwise how would they know to build

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them in that perfect way careful

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repeatable observations also underline

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the modern or underlie modern science

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elements of modern science were

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therefore present in many early human

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cultures the past that led to modern

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science emerged from the ancient

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civilizations of the Mediterranean and

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the Middle East especially from ancient

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Greece Greece gradually rose to power in

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the Middle East beginning around 800 BC

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and was well established by about 500 BC

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Greek philosophers developed at least

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three major innovations that helped pave

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the way for modern science first they

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developed a traditional I'm sorry they

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developed a tradition of trying to

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understand nature without relying on

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supernatural explanations and of working

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communally to the baits and challenge

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each other's idea so this is a really

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big turning point up until those points

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I mean almost everything was believed to

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be supernatural but now they take away

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that supernatural influence and they

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debate and they talk to one another so

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this was really the the birth of modern

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scientific community second the Greeks

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used mathematics to give precision to

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their ideas which allowed them to

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explore the implications of new ideas in

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much greater depth than whatever

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otherwise been possible so now they're

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adding math into the equation

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third while much of their philosophy

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actively consisted of subtle debates

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grounded only in thought and was not

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scientific in the modern sense the

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Greeks also saw the power of reasoning

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from observations they understood that

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an explanation could not be right if it

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disagreed with observational facts and

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so this is very important all three of

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these I mean the community the use of

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math and then the reliance and

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observation this is really the beginning

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to of the birth of modern science so I'm

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taking this now and taking a look at

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what the Greeks came up with to describe

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the universe we start here with our own

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solar system they had a way to describe

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our solar system that we call the

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geocentric model the Greek geocentric

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model of the cosmos so named because it

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placed a spherical earth at the center

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of the universe develops gradually over

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a period of several centuries because

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this model is so important in the

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history of science let's briefly trace

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its developments so we're going to spend

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the rest of this lecture really taking

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ourselves from nothing to this model how

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do we get to this point is basically

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what we're looking at so this geocentric

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model places the earth at the center of

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the universe

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hence geocentric and it's comparable to

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a Mary ground as you see on the left so

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you could consider the earth to be the

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center the axis of that rotating Mary

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ground and then perhaps the children on

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the rides as the planets are moving

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around that Center so the first thing

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I'm going to show you now is actually a

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timeline it's two slides because it

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couldn't fit it on one slide this is a

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timeline of all the important people

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that led us to that geocentric model now

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I'm not going to sit here and just list

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them all off we will go through most of

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the important people in the coming

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slides so I put this in here simply for

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you to reference it's a great resource

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so here's the other half of it it's a

play14:49

great place to look if you just wanted

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some quick information about who did

play14:53

this or when did this person do that but

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we will go into detail of some of these

play14:57

people know so these slides do serve as

play14:59

a reference

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so you go back a slide so we're going to

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begin at the top left we're going to

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begin with salaries we generally trace

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the origin of Greek signs to the

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philosopher Follies valleys was the

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first person known to have addressed the

play15:17

question what is the universe made of

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without resorting to any supernatural

play15:22

explanation his own guess that the

play15:26

universe fundamentally consisted of

play15:28

water and that the earth is a flat disc

play15:30

floating in an infinite ocean was not

play15:34

widely accepted even in his own time

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nevertheless just by asking the question

play15:38

he suggested that the world is

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inherently understandable and thereby

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inspired others to come up with better

play15:45

models for the structure of the universe

play15:48

so even though he was very incorrect as

play15:51

we know today and not many people

play15:53

believed him it was still a big turning

play15:55

point in story and astronomy next is

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Anaximander a more sophisticated idea

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followed soon after proposed by a

play16:04

student of the Hollies named Anaximander

play16:07

he suggested that earth floats in empty

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space so we're making progress

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surrounded by a sphere of stars and two

play16:14

separate rings along which the Sun and

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Moon travel we therefore credit him with

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inventing the idea of what we will call

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the celestial sphere you hear me talk

play16:24

about that a lot once we get through

play16:25

this history lesson interestingly

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Anaximander imagined earth itself to be

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cylindrical rather than spherical in

play16:33

shape now that sounds odd but think

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about this he probably chose this shape

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because he knew earth had to be curved

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in a north-south direction to explain

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changes in the constellations with

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latitude because the visible

play16:48

constellations do not change with

play16:49

longitude he no he saw no need for

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curvature in the east-west direction

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right so as you travel north to south

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along the globe what you see in the sky

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in terms of constellations changes but

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if you travel say from Durant Oklahoma

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straight east or west you will see the

play17:08

exact same constellations so it's kind

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of reasonable that he thought curvature

play17:13

was only along one direction

play17:14

so that assumed the earth was

play17:15

cylindrical even though seen as weird is

play17:18

actually not too inaccurate to think

play17:20

about back then all right next we have

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Pythagoras we do not know precisely when

play17:28

the Greeks first began to think that

play17:30

earth was round but this idea was taught

play17:32

as early as about 500 BC by the famous

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mathematician Pythagoras he and his

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followers envisioned earth as a sphere

play17:40

floating at the center of the celestial

play17:42

sphere much of their motivation for

play17:45

adopting a spherical earth was full

play17:46

philosophical the pythagoreans had a

play17:51

mystical interest in mathematical

play17:54

perfection and they considered a sphere

play17:57

to be geometrically perfect so they

play18:00

believed that we were the center of

play18:01

everything we were perfect and all that

play18:03

so they thought that the earth was

play18:05

spherical not because it was an

play18:08

observational fact at the time but

play18:10

because that was perfection and that's

play18:12

the way they viewed it and so it's

play18:15

pretty amazing that it could be so

play18:17

simple next is Plato the Pythagorean

play18:23

interest and heavenly perfection became

play18:25

deeply ingrained in most Greek

play18:27

philosophers so that idea really really

play18:30

held on for a long time as you'll see as

play18:32

we go on it took on even more

play18:35

significance after Plato asserted that

play18:37

all heavenly objects move in perfect

play18:39

circles and at constant speeds and

play18:41

therefore must reside on huge fears

play18:44

encircling the earth so not only now do

play18:46

we think the earth is a perfect sphere

play18:47

at the center of everything well we

play18:49

believe everything else moves in perfect

play18:51

spheres at perfect speeds around us the

play18:55

Platonic belief and perfection

play18:56

influenced astronomical models for the

play18:58

next 2,000 years of course those Greeks

play19:03

who made observations found plato's

play19:05

models to be problematic the apparent

play19:08

retrograde motion of the planets which

play19:10

we'll talk about in a second the

play19:11

backward motion of planets in the sky

play19:13

already well known by that time clearly

play19:16

show that the plans do not move at

play19:18

constant speeds around earth so there

play19:20

was already some issue with this idea

play19:23

an ingenious solution came from plato's

play19:27

colleague Eudoxus

play19:28

who created a model in which the Sun the

play19:31

moon and the planets each had their own

play19:33

spheres nested within several other

play19:35

spheres individually the nested spheres

play19:39

turned into perfect circles by carefully

play19:43

choosing the sizes rotational axes and

play19:45

rotation speeds for the invisible

play19:47

spheres Eudoxus was able to make them

play19:50

work together in a way that reproduced

play19:52

many of the observed motions of the Sun

play19:55

the moon and the planets in our sky

play19:58

other Greek models refined the model by

play20:01

comparing its predictions to

play20:02

observations and adding more spheres to

play20:05

improve the agree agreement so here in

play20:08

the top you see what we call that

play20:10

retrograde motion so in the sky this is

play20:14

for example the path of Mars at the

play20:16

beginning of January starts over here

play20:18

and moves from west to east throughout

play20:20

the months but then for a little while

play20:22

it moves

play20:23

apparently backwards through the sky

play20:25

that's that retrograde motion I

play20:26

mentioned and then it continues its path

play20:28

from west to east so that was a

play20:31

challenge to this perfect circle idea so

play20:35

you DOCSIS came along and started to

play20:37

come up with some ideas of these nested

play20:38

spheres which we'll get into more in

play20:40

just a moment following Eudoxus is

play20:45

Aristotle whether you DOCSIS and his

play20:49

followers thought of the nested spheres

play20:50

as real physical objects is not clear

play20:53

but Aristotle certainly did an

play20:55

Aristotle's model all the sphere is

play20:58

responsible for celestial motion were

play21:00

transparent and interconnected like the

play21:03

gears of a giant machine Earth's

play21:05

position at the center was explained as

play21:08

a natural consequence of gravity

play21:11

Aristotle argued that gravity pulled

play21:13

heavy things toward the center of the

play21:14

universe and allowed the lighter things

play21:16

to float toward the heavens thereby

play21:18

causing all of the dirt rock and water

play21:20

of the universe to collect at the center

play21:22

and form the spherical earth I guess not

play21:25

a terrible idea back then

play21:28

we now know that Aristotle was wrong

play21:30

about both gravity and Earth's location

play21:32

however largely because of his

play21:34

persuasive arguments for an

play21:35

earth-centered universe this geocentric

play21:38

view dominated Western thought for

play21:40

almost two thousand years to explain the

play21:46

apparent retrograde motion of the

play21:47

planets

play21:48

Apollonia suggested that each planet

play21:50

moved around earth on a small circle

play21:52

that turned upon a larger circle the

play21:55

small circle sometimes referred to as an

play21:57

epi cycle and the large circle is often

play22:00

called a defferent or deferment so two

play22:03

important terms a planet following this

play22:06

circle upon circle motion that you can

play22:08

see in the schematic on the right would

play22:10

trace a loop as seen from Earth with the

play22:14

backwards portion of the loop mimicking

play22:15

the apparent retrograde motion so that

play22:18

graph that I showed you a moment ago

play22:20

with that retrograde motion this could

play22:22

explain it so this idea of a circle upon

play22:24

circles so the idea is that the planet

play22:27

itself moves in a little circle but as

play22:29

it's moving in that little circle that

play22:31

circle as a whole is moving around a

play22:33

larger circle so if you were to trace

play22:35

this out it would form this little bit

play22:37

of a backward motion for some time

play22:39

before returning back to that

play22:40

west-to-east motion so right there you

play22:43

could explain the retrograde motion

play22:45

because of this idea among his many

play22:51

accomplishments a park is developed the

play22:53

circle upon circle idea of Apollonius

play22:55

into a model that could predict

play22:57

planetary positions so this is the first

play23:00

time now that we are taking something

play23:01

that we see and using it to predict

play23:04

future positions to do this

play23:07

the park is had to add several features

play23:09

to the basic idea for example he

play23:12

included even smaller circles that moved

play23:14

upon the original set of small circles

play23:15

and he positioned the large circle

play23:18

slightly off centered from Earth so now

play23:20

not only are we starting to predict

play23:22

things but we're also slightly starting

play23:26

to move away from this idea of

play23:27

perfection by placing them off centered

play23:30

from the earth so we're getting there

play23:33

but the culmination of it all if this

play23:36

geocentric model comes from : a Greek

play23:40

modeling of the cosmos culminated in the

play23:42

work of Claudius Ptolemy Toula mais

play23:44

model still placed earth at the center

play23:46

of the universe but it differed in

play23:49

significant ways from the nested sphere

play23:51

ideas of Eudoxus and Aristotle we refer

play23:55

to Ptolemies geocentric model as the

play23:57

Ptolemaic model to distinguish it from

play23:59

the earlier models so he has his own

play24:02

name now for this model the Ptolemaic

play24:04

model tolas great accomplishment was to

play24:08

adapt and synthesize earlier ideas into

play24:10

a single system that agree quite well

play24:12

with the astronomical observations made

play24:14

at the time so even though it was still

play24:17

wrong what he put together agreed to

play24:22

reasonable extent with the observations

play24:24

that were being made at that time so he

play24:26

basically took everything and put into

play24:28

one nice package in the end he created

play24:31

and published a model that could

play24:32

correctly forecast future planetary

play24:34

positions within a few degrees of Arc

play24:37

which means an arc a degree of Arc is a

play24:42

sixtieth of a degree which we'll get

play24:44

into later as well oh I can explain it

play24:48

too I mean it's also about the angular

play24:51

size of your hand held at arm's length

play24:53

against the sky so right now you can

play24:56

hold your arm out all the way extend it

play24:58

with your hand sticking up and he could

play25:01

predict planetary positions within a few

play25:03

degrees of Arc which is the width of

play25:05

your hand so that gives you an idea this

play25:10

was sufficiently accurate at the time to

play25:12

keep the model in use for the next 1500

play25:15

years so this geocentric model came

play25:19

together pretty quickly relatively

play25:21

speaking through all these different

play25:22

people and until my Tola may put it into

play25:25

one nice package where the earth is at

play25:27

the center of the universe and

play25:28

everything moved around us even though

play25:31

it was incorrect it was a way of

play25:33

explaining what they saw so it was still

play25:36

great that they were using science to

play25:38

agree with the observations they were

play25:40

making and that's a part of what makes

play25:43

science so tough sometimes I mean for

play25:45

thousands of years

play25:46

they believe this was correct and it did

play25:48

agree with observation so I mean who

play25:51

knows even today we could be sure about

play25:53

something and then a thousand years are

play25:54

going to find out that we were totally

play25:56

wrong and so we know that the earth is

play25:58

not the center the universe so in our

play26:01

next lecture we're going to talk about

play26:03

the Copernican revolution that takes us

play26:05

away from ancient the ancient Greeks

play26:07

model of the earth centered system and

play26:09

it takes us to the heliocentric system

play26:11

where the Sun is the center of our solar

play26:13

system which is in fact correct so now

play26:16

we're going to start getting closer and

play26:17

closer to modern science so as always

play26:20

thanks for watching and I'll see you in

play26:21

the next lecture

play26:22

[Music]

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