| Spring 2010 | Astronomy 110 | MWF 9:30 &mdash 10:20 |
We begin with a brief overview of the universe and the distances, ages, and sizes of various astronomical objects. We will then focus on our home planet and its motion, which plays a critical role in our observations the universe.
| 1.1 | Our Modern View of the Universe • What is our place in the universe • How did we come to be? • How can we know what the universe was like? • Can we see the entire universe? |
| 1.2 | The Scale of the Universe • How big is Earth compared to our solar system? • How far away are the stars? • How big is the Milky Way Galaxy? • How big is the universe? • How do our lifetimes compare to the age of the universe? |
| 1.3 | Spaceship Earth • How is the Earth moving in our solar system? (skim rest if you wish; we'll come back to it) |
| 2.1 | Patterns in the Night Sky • What does the universe look like from Earth? (through p. 28, and "The Local Sky") • Why do stars rise and set? • Why do the constellations we see depend on latitude and time of year? |
| 2.2 | The Reason for Seasons • What causes the seasons? • How do we mark the progression of the seasons? |
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Joshua
E. Barnes
(barnes at ifa.hawaii.edu)
Updated:
16 January 2010
http://www.ifa.hawaii.edu/~barnes/ast110_10/orientation.html |
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