High School Earth Science—Semester A

The pale blue dot, Shmoop style.

  • Credit Recovery Enabled
  • Course Length: 18 weeks
  • Course Type: Basic
  • Category:
    • Science
    • High School

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Welcome to Earth Science, Shmoop-style. Come on in, make yourself at home. After all, this course is all about the giant blue marble we all call home. That's right, we're talking about the ins and outs of our favorite planet: the sunEarth. It's like the king of planets! This course will take you on a tour of everything our little planet has to offer, from giant tectonic plates surfing on waves of magma to a transparent blanket of molecules that keeps us cozy (sometimes a little too cozy, but we'll talk global warming later).

We'll also cover Earth's life story, from its adorable baby years as a barren, oxygenless rock, to the awkward teen years (you thought acne was bad, try having volcanoes on your face), to the present day, where it's just trying its best to keep us all alive. And since we're not total narcissists, we'll also venture out a bit into space, to see what's been going on since that whole Big Bang thing. After all, the Earth is pretty cool, but it's not the center of the universe.

Once you're done with Semester A of this course, you can expect to be a rock star in the following:

  • what the study of earth science actually covers, because "being on Earth" just isn't enough;
  • the Big Bang and all the stuff that spewed out of it;
  • our solar system, what holds it together, and why it doesn't all freeze while flying through space;
  • identifying rocks and minerals and how they were born;
  • how we know anything about the Earth's origins when there were no cameras around to capture all of the action;
  • Earth's very long life story;
  • what's on the inside of the Earth, and what that means for the surface.

Shmoop has a solid lineup of activities, quizzes, and projects for your Earth-gazing needs. So, let's get to it. Earth might stick around for a couple more billion years, but we sure won't. Time's a-wastin'.

Oh, and before we forget: High School Earth Science is a two-semester course, and you're staring Semester A in the face. You can stare at Semester B's face right over here.

Technology Requirements

From a technology standpoint, all you need for this course is a web browser-capable computer and a reliable internet connection. A tablet works, too, if you don't mind typing on it. Additionally, access to a scanner or digital camera, or a cellphone with a camera, or jeez, even a webcam, will come in handy, since you'll occasionally need to upload images of diagrams you draw. That's it.

Required Skills

Knowledge of Algebra concepts


Unit Breakdown

1 High School Earth Science—Semester A - Introduction to Earth Science

To learn all you can about Earth, you'll first need to know about science. It's right there in the name of the course, so this can't be too surprising for you. This first unit will make sure everyone is up to speed on the scientific method; how to collect, graph, and analyze good data; and some basic physics and chemistry we'll be using throughout the course. Once everyone's down with the physical processes and chemical reactions that provide the basic building blocks for Earth, we'll be ready to look at how it actually was built in Unit 2.

2 High School Earth Science—Semester A - The Universe

The universe is kind of a big deal. The biggest, really, since it includes, well, everything ever. We're going to focus on just some of its more interesting features—where it came from (a super hot, dense mass of space-time), how we know that (science!), the formation of galaxies and stars (gravity helps pull it all together), how stars create different elements (gravity gets to working overtime here), and black holes (uh, you can stop now, gravity). By understanding how the universe was formed, we can understand how our solar system and our planet (the "Earth" in "Earth Science" were formed too.)

3 High School Earth Science—Semester A - Our Solar System

After our whirlwind tour of the entire universe, we zoom in and take a closer look at our own neighborhood—the solar system. Our local space is full of planets, moons, comets, asteroids, meteors, and more. As you might expect after last unit, gravity plays a key role in keeping all this clutter close by. We'll also explore out how the Day Star at the center of our solar system makes Earth such a cuddly, livable place for us.

4 High School Earth Science—Semester A - Rocks and Minerals

After a couple units drifting among the stars, we'll finally start digging into the dirt of this course. Technically, we'll be digging into rocks and minerals in this unit, since they're not dirt. We'll learn how to classify, identify, and indemnify them, as well of how they are formed in the first place. That includes taking a tour of the Rock Cycle, Earth's slowest-moving recycling program.

5 High School Earth Science—Semester A - Evidence for Earth's History

How do you know that? might just be the most important question ever asked. That's because answering it stands at the core of science—it's all about the evidence, baby. In this unit, we're going to look at how we can know anything about Earth's ancient history. We weren't there way back when, but the past has left its smudged fingerprints all over the present. We'll use both radioactive dating and the positions of Earth's layers to pin down a timeline.

6 High School Earth Science—Semester A - Geologic Time Scale

Now that we're certified time detectives, we'll deep-dive into the details of Earth's history. All 4.54 billion years of it. If your jaw isn't on the floor thinking about how large a single billion is, much less four and a half of them, then we humbly suggest you haven't thought about it enough. Don't worry, we'll help you properly put that amount of time into perspective before we explore the main eras of the past. We'll also take a look at one of the most important pieces of evidence about what the world was like in the distant past—fossils. Maybe if we're lucky, one day our preserved remains will teach scientists of the future about the present day.

7 High School Earth Science—Semester A - Earth's Innards

Now we're really going to start digging deep. The semester ends with us drilling down through 4,000 miles of Earth's rocky insides. The thing about it is that the inside of Earth isn't sitting still—it's constantly (but very slowly) moving matter and energy around through its various layers. Knowing what those layers are up to is key to understanding all kinds of important processes on the planet's surface. We'll check out how earthquakes, volcanoes, mountains, and even the shapes of the continents all tie into Earth's innards.


Recommended prerequisites:

  • Algebra I—Semester A
  • Algebra I—Semester B

  • Sample Lesson - Introduction

    Lesson 7.04: Plate Tectonics

    We've always had a love-hate relationship with puzzles.

    Puzzles are both mentally stimulating and totally mindless, which means that after six hours spent sitting on the couch leaning over the coffee table, we can feel like we've really accomplished something. It's super satisfying to put that last piece in its spot and see all 1,000 little shapes come together to make a big picture.

    At the same time, it's pretty frustrating to spend six hours sitting on the couch leaning over the coffee table and have nothing real to show for it but an achy back. It's exhausting to spend all night working on a puzzle and still not be finished. And it's absolutely infuriating to get to the end and realize that we were missing a piece all along.



    Puzzle with one piece missing.
    Gah! If only we'd known before we put the other 999 pieces in place.
    (Source)

    In this lesson, we're going to look at the biggest puzzle on the planet. This puzzle only has a few dozen pieces, but since one piece covers more than 40 million square miles, it isn't a puzzle we can piece together on our coffee table.

    Together, these puzzle pieces, or plates, cover Earth's surface, and we'll look at what they are, why they exist, and how they shape our planet. This is important stuff because the movement and position of the plates determine our planet's geography, climate, and biology. In short, they determine whether this is a place we can live. It's a good thing this puzzle isn't missing any pieces.


    Sample Lesson - Reading

    Reading 7.7.04: Earth's Puzzle Pieces

    In the last few lessons, we've discussed how the earth is made up of layers. The top 60 miles or so—the lithosphere—is compact rock that includes both the crust we walk on and the upper, solid portion of the mantle. While it may look pretty solid to us, the lithosphere is not one connected sheet of rock, like the peel of an orange or the skin of an onion.

    Instead, imagine taking a hard-boiled egg and rolling it gently under your hand until the shell cracks. The shell still covers the egg, but now it's cracked and broken into small sections. The lithosphere is likewise broken up into numerous tectonic plates (sometimes called lithospheric plates), which sit on top of the semi-solid asthenosphere. There are seven major plates, ten minor plates, and numerous smaller plates that fill in the gaps.

    Map of the major tectonic plates.
    (Source)

    Keep in mind that although there are also seven continents, these landmasses don't perfectly match up with the major plates. As we can see on the map above, Europe and Asia mostly share one giant plate, but parts of those continents, like India, are on entirely different plates. The two don't always neatly match, but what's happening below the surface is the main factor in what, geographically, is happening above.

    Between a Rock and a Hard Place

    While the plates are important, the real interesting stuff occurs at the places where they meet, because that's where the movement happens. The edges of tectonic plates are called plate boundaries, and there are three main types: divergent boundaries, convergent boundaries, and transform faults.

    At divergent boundaries, two plates move away from one another at fissures in the earth. Powered by convection currents in the mantle, the crust is stretched and cracked. This allows magma to flow upward, causing the plates to move apart from one another as new plate material is created to fill in the gaps.

    Divergent boundaries almost always occur where two similar plates meet. When two oceanic plates move apart, new ocean floor is created. The Mid-Atlantic Ridge is a great example of this, while the East African Rift is a good example of a divergent boundary between two continental plates.

    At convergent boundaries, two plates move toward one another, but what happens when they collide depends on what kinds of crust the plates are. There are three different kinds of convergent plate boundaries.

    Take a quick visit to the U.S. Geological Survey's website to learn about the differences between the three types of convergent boundaries. Make sure to take note of what geologic features exist as a result of the collision and why they occur. Also pay attention to the explanation of subduction zones and how different types of crust subduct based on how dense they are.

    Transform faults are different from the other two because they don't involve the creation or destruction of new crust. Instead, they occur where the edges of two plates slide sideways past one another—although "slide" isn't really the right word when we're talking about huge pieces of rock 60 miles deep.

    Instead, as the plates move past each other, they grind and scrape together like two giant pieces of sandpaper, building up huge amounts of energy that get released in the form of huge earthquakes. After an earthquake at a transform boundary, like the San Andreas fault in California, we might wake up to find our rosebushes are now in our neighbor's' yard.

    Recap

    Feeling like plate tectonics theory is a bit of a puzzle itself? Let's quickly look through the pieces:

    • Tectonic plates are pieces of Earth's solid lithosphere that move on top of the semi-solid asthenosphere. They move as a result of convection currents in the mantle.
    • At divergent boundaries, plates move away from one another and new plate material is created in the space left behind.
    • At convergent boundaries, plates collide into one another. What happens next depends on whether the plates are oceanic or continental crust.
      • If a continental plate converges with an oceanic plate, then the denser oceanic plate will subduct, or sink, below the continental plate. This leads to the formation of magma, plus a convenient channel for it to find its way to the surface.
      • If two oceanic plates converge, then the older, denser plate will subduct.
      • Continental plates won't subduct. They'll just smash into each other to form mountain ranges.
    • At transform faults, plates grind sideways past each other.
    • These different boundaries result in different geologic features like volcanoes and earthquakes. Since we're afraid of both of these things, we can plan our next vacation by avoiding them.

    Sample Lesson - Activity

    Activity 7.04a: Where in the World?

    Remember maps? We're not talking Google Maps here. We mean good old-fashioned paper maps that you had to read and interpret yourself.

    These maps could be a pain to read if you didn’t know what you were doing, though. These days, you can just ask Siri for directions, and she'll tell you exactly how to get there, how long the trip will take, and if there are any In-N-Outs along the way. That's pretty cool—at least until the battery runs out. Know who’s got your back then? Old-school maps.

    So, it's still be helpful to understand maps. You don't want to be one of those drivers who follows their GPS right into a lake, do you?

    While we can't guarantee you won't end up swimming for the shore, we can at least help you steer clear of some other natural features. In this lesson, you'll be mapping volcanoes, earthquakes, and a few other things.

    There are two parts to this activity. First, we'll work with a paper map. Then, the real fun begins, because you'll build some 3D models for some of the features you'll map out in the first part.

    Materials

    • A way of printing out the world map linked below
    • Colored pencils or markers
    • Scratch paper
    • Some clay or Play-Doh; if you want to make your own, here's Shmoop's quick and easy recipe for two-ingredient dough (you can pick up the ingredients at the dollar store)
      • Mix 1 cup of hair conditioner, body lotion, or shaving cream with 2 cups of corn starch.
      • Mix together until you have a moldable dough.
      • Optional: add food coloring to make it pretty.

    Part I

    Step One: Download and print out this handy-dandy world map.

    Step Two: Hop on the internet. You'll need to look for the locations of major volcanoes around the world. Once you've found them, plot them on the map. You can choose whatever symbol you want, like little triangles or circles, but make sure you let us know what it is by drawing a legend.

    Step Three: Now, find the locations of major earthquakes and do the same thing. Plot the earthquakes on your map using a symbol you choose, and identify that symbol on your map legend.

    Step Four: Looking at your map, make a 3–4 sentence hypothesis about plate boundaries. Where would you expect to see transform faults? How about convergent boundaries? (Be sure to identify which type of convergent boundary you're talking about, like oceanic-oceanic.) Why? Write your hypothesis out on a separate sheet of paper, or better yet, type it up in a doc.

    Step Five: Search online for the locations of the tectonic plates (or look at the map from this lesson's Reading). Draw them on your map, too. You don't need to do all the minor plates, but you should include at least the 10–12 biggest ones.

    Step Six: Take a look at your map. What do you notice? Write a paragraph or two (5–10 sentences) below your hypothesis describing your observations. Be sure to explain why different features occur where they do. Also, be as specific as possible when talking about the different types of plate boundaries.

    Part II

    Now that you've got a good understanding of where plate boundaries are and what happens when different plates meet, let's build some models and play around with some clay or Play-Doh. You'll also be answering some questions along the way, so you might want a notebook or some scratch paper to write in.

    Step One: Make six "plates" out of your dough. They don't have to be in the shape of the real tectonic plates, but that would win extra cool points. How big you make them will depend on how much material you have.

    Step Two: Grab a couple of your plates and place them next to each other. Then, push them together until you have a mountain range. With some small pieces of paper, label the two plates (are they continental or oceanic?), the type of boundary formed, and the direction in which each plate is moving.

    Where on your map from Part I would you expect to find mountains like the ones you've just created? What can we say about the densities of these two plates?

    Step Three: Take a couple more plates and place them next to each other. Their edges should touch, but don't push them together. Rather, try to slide them past each other. Yeah, there will be some "damage" to the plates, but that's life, and we're modeling real stuff here. With some small pieces of paper, label the two plates (continental or oceanic), the type of boundary, and the direction in which each plate is moving.

    Where on your map from Part I would you find a plate boundary like this? Was new crust created during this interaction? Why or why not?

    Step Four: After placing the last two plates next to each other, push them together so that one plate subducts under the other. With some small pieces of paper, label the two plates (continental or oceanic), the type of boundary, and the direction in which each plate is moving.

    Where on your map from Part I would you find a plate boundary like this? Was there a noticeable difference between the size of the plate that subducted and the other that floated on top?

    Step Five: Snap some clear pictures of your models. Make sure that the labels are legible.

    When you're all done cleaning up, collect all of your notes and answers to our questions. Here's a list of everything you'll be turning in for this activity:

    • Your filled-in, labeled map (from Part I, Steps One through Five).
    • The page with your 3–4 sentence hypothesis (from Part I, Step Four) and 5–10 sentence observations (from Part I, Step Five).
    • The pictures of your 3D models (from Part II, Step Five).
    • Your model observations (from Part II, Steps Two through Four).

    Stick all of those in some documents and upload them using the button below. Then put a copy of everything in your car, just in case Siri tries to lead you into a transform fault or something.


    Sample Lesson - Activity

    1. Susie wakes up and realizes that she is surrounded by huge mountains. She is pretty sure they are volcanoes, and she also sees a sign warning about earthquakes. What type of plate boundary is Susie likely near?

    2. Which of the following describes what occurs at a transform plate boundary?

    3. Why do volcanoes typically occur at subduction zones?

    4. When continental and oceanic crust converge, which of them will subduct?

    5. Which of the following statements about plate tectonics is true?