Lecture 6 – History of Astronomy, Part 1/2
Summary / Checklist of the Main Concepts to Understand and Remember
Astronomy in the Classical Period – 4th Century BC to 2nd Century AD | ||
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What is the difference between a geocentric and a heliocentric model of the universe (or the solar system)? | |
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What is planet retrograde motion? (How do planets move on the Celestial Sphere, normally and during retrograde motion?) | |
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What is parallax in general, and what is stellar parallax? | |
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What does stellar parallax have to do with understanding the Solar System? | |
• | What were the main points of Aristotle's theory about how objects move? | |
• | What were some of Aristotle's arguments in support of the idea that the Earth did not move through space? | |
• | Why is Ptolemy important in the history of astronomy? Around what time (what century) did he live? | |
• | How did Ptolemy explain the retrograde motion of planets? | |
• | What is an epicycle? | |
Topics from the lecture page and textbook not listed above [or between square brackets]
were not covered in class;
Underlined words indicate that I will expect students to remember a number or a name related to that topic.
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