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From red shift to telescopes to the Big Bang theory

Have you ever wondered what those bright twinkly blobs in the night sky actually are? Oh sure, your science teacher says they're stars, but you've always secretly suspected there's more to it than that. (Otherwise why would Jiminy Cricket be so obsessed with them?) Well you're right—there is more to it than that. It's called astronomy, and it lets you in on the secret lives of stars, planets, and everything in between.

Here you'll learn where stars go to die, ponder the possibility of time travel, learn about red shift, and contemplate the likelihood that some alien version of you is contemplating exactly the same thing billions of light years away (i.e. get cozy with the Drake Equation). You'll also learn what a light year actually is, why you don't need to worry about a rogue planet slamming into Earth and ending life as we know it, and what you should be worried about.

In this course, we'll cover:

  • the history of astronomy
  • our solar system (love you, Milky Way!)
  • everything you'd ever want to know about stars
  • tools of the trade (telescopes, parallax, mapping)
  • cosmology and the history of the universe
  • the big questions in astronomy
  • how to become an astronomer

Astronomy's one science where you can actually indulge your secret Star Trek fantasies—warp drive, time travel, and alien life are all legitimate fields of study here. So suit up, Shmoop up, and prepare to boldly go. Find out where the stars can take you, and what they can teach us.

Course Breakdown

Unit 1. There's No Place Like Home

This unit covers the basics of astronomy: what astronomy is, a brief history of astronomy, what astronomists study, and major astronomical bodies we'd find in our solar system.

Unit 2. Goodness Gracious, Great Balls of Fire

This unit is all about stars. What are they? What are they made of? We learn about the life cycle of stars, and then study deep space phenomena like nebulae, black holes, and other star systems. Finally, we'll examine real data from the Kepler telescope and websites like Galaxy Zoo to get some hands-on astronomy experience.

Unit 3. Tools of the Trade

This unit studies the tools astronomers use to do astronomy, including one of the most important: the telescope. After reviewing the history of the telescope and how it revolutionized our understanding of the sky, we'll learn the basics of modern telescopes and make our very own 'scope. Finally, we'll learn about a few other "tools," like parallax, ascension, declination, and learn about how the Earth's tilt affects our planet.

Unit 4. Cosmology, the Universe, and Math

In this unit we really bit into some meaty cosmological topics: Kepler's Laws of Planetary Motion, the Cosmic Distance Ladder, the Big Bang Theory, and the history of the universe. Ever wondered what Olbers' Paradox is? Find out here.

Unit 5. The Big Questions in Modern Astronomy

We cap off the course by investigating some of the big remaining questions in modern astronomy, including SETI, the search for extra-terrestrial intelligence. We'll get cozy with the Fermi Paradox, the Drake Equation, and close out the course by exploring career opportunities in astronomy.

Sample Lesson - Introduction

Lesson 3: Welcome to Our Solar System

[insert inappropriate gas cloud joke here]

Not to put too much pressure on it, but we can't really discuss astronomy without discussing the beginning of our solar system. After all, if there were no solar system, there would be no astronomy, and no human beings to talk about it. One event triggered all the necessary ingredients to create the cosmos and life itself. That's a lot to riding on the shoulders of one event. We hope it's been working its delts.

While we don't know exactly how the solar system formed, we do have an educated guess. We think that about 5 billion years ago a gas and dust cloud called a nebula collapsed. Why? Here are some theories:

  • A giant star exploded and the shockwave of energy from it caused the collapse. So we are made up of star dust. (Take that, everybody who said you wouldn't make it in Hollywood.)
  • At the middle of the cloud, a magnetic field created a wave of energy that caused the collapse.
  • Waves of radiation from supergiant stars caused the collapse.

Any way you slice it, the cloud started to spin, and its middle got very hot. Let's journey inside the universe when it was in a hot, dense state. First stop: Gas Cloud.

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  • Course Length: 1 weeks
  • Grade Levels: 10, 11, 12
  • Course Type: Elective
  • Category:
    • Science
  • Prerequisites:
    Algebra I—Semester A
    Algebra I—Semester B

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