High School Earth Science—Semester B

Shmooping the land, sea, and air.

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

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Captain Kirk said that space is the final frontier, but we think that exploring Earth has its own charms. In Shmoop's Earth Science course, you'll boldly study what makes our planet tick. If you want to know what makes it tock, consider taking a clock-making class instead.

This is Semester B of the aforementioned course, which gets down in the dirt with the following topics:

  • the forces that shape Earth's surface—because even planets like getting a makeover every couple centuries;
  • what's happening up in the atmosphere above our heads (besides Lucy and her diamonds dive-bombing 747s for fun);
  • the difference between weather and climate, and why you should care;
  • how crucial compounds like carbon, water, nitrogen, and phosphorus cycle between living things (like us) and the environment;
  • how Earth's processes have impacted human societies, and how we in turn have impacted the Earth;
  • the Ghosts of Climate Change—Past, Present, and Future.

Through it all, we have enough activities, quizzes, and projects to buckle a tectonic plate.

Oh, and a friendly reminder: High School Earth Science is a two-semester course, and this is Semester B. If you yearn for Semester A, click-click here to find it.

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

8 High School Earth Science—Semester B - Shaping Earth's Surface

Beauty is only skin deep, and Earth is gorgeous. So, we'll spend a unit poring over the surface of the planet to soak in the view. Well, and to learn about the forces that shape it. Earth's surface isn't static, whether we're looking on land or at sea. The oceans are constantly churning, and the ground is constantly under assault by wind and water. While plate tectonics spends eons building Earth's surface up, erosion and deposition are wearing it down. They're the perfect tools for touching up the planet's appearance before a big night out in the solar system.

9 High School Earth Science—Semester B - Earth's Atmosphere and Weather

Look—up in the sky! It's a cloud! A low-pressure air mass! It's...the weather! Okay, maybe all of those exclamation points were overkill, but still—it's okay to get excited about the weather. In this unit, we tackle the basics of what causes it to rain, sleet, and snow (and all the other fun atmospheric conditions that try to stop the postal service from doing its job). And we'll also talk about why weatherpeople can be wrong so often and still keep their jobs. The short version? Their reputation is worse than their bite, and predicting the weather is hard.

10 High School Earth Science—Semester B - Seasons and Climate

We just finished talking about what makes the weather tick, so it's natural to follow up with a discussion of climate. They're two different, but related, things. While the weather is all about the day-to-day business of what the atmosphere is up to, the climate takes the long view of things. We're not talking about the weekly forecast, but patterns that can only be noticed when looking at events over 10s, 100s, 1000s, or even 1,000,000s of years. In this unit, after a quick look at what causes the seasons each year, we'll cover what Earth's climate has been like in years (and decades, centuries, millennia) past.

11 High School Earth Science—Semester B - Biogeochemical Cycles

Carbon...oxygen...water...nitrogen...phosphorus. By their powers combined, we get the biogeochemical cycles. They're no Captain Planet, but they'll do in a pinch. That's because they determine how some very basic, very important compounds and nutrients are distributed. They get passed back and forth between living things and the environment, they are chemicals, and they are always on the move—that covers the "bio," "geo," "chemical," and "cycle" parts of the term.

12 High School Earth Science—Semester B - Human History on Earth

Despite how awesome human beings are (and we are pretty awesome), at the end of the day we're still a bunch of hairless apes. That means we're just as reliant on the environment around us as any other living thing. In this unit, we explore how our basic biological needs, natural disasters, disease, climate, and the distribution of resources have all affected human societies throughout the ages. The next time you're feeling all high and mighty, stop and think about how much you owe Mother Nature.

13 High School Earth Science—Semester B - Human Impact on Earth

So, we just got done saying that humans aren't that big of a deal. That's not 100% true, though. We can have huge effects on the world around us. It turns out that feeding, clothing, and entertaining over seven billion of us uses up a lot of resources. In this unit, we explore the impact that human activity has had on the planet's land, water, and atmosphere, how we can minimize the harm we cause, and we'll evaluate possible future-tech solutions to our current pollution woes.

14 High School Earth Science—Semester B - Climate Change

In the final unit of this course, we tackle the biggest topic in all of Earth Science—the future of our planet. While we wish this unit was called Ice Cream Volcanos and Free Trips to Disneyland, the reality is a little bleaker than that. In a way, this unit is a culmination of stuff we've been talking about throughout the rest of the course. To know the future, we need to know the past, so we'll go into more detail about the Ghost of Climates Past, particularly the positive feedback loops that help drive climatic shifts. Then we'll take a closer look at the present, examining the meteorological and biological evidence that we're in the middle of a shift in climate—and how we've caused it. Then our eyes look to the future to predict the impacts climate change will have on the planet, as well as what we can do to help minimize those effects. Hopefully, we can squeeze a rocky road ice cream cone and a Disney trip in there somewhere.


Recommended prerequisites:

  • Algebra I—Semester A
  • Algebra I—Semester B
  • High School Earth Science—Semester A

  • Sample Lesson - Introduction

    Lesson 14.03: Climate Feedback



    A term paper with teacher comments in red ink
    Think this feedback is harsh? Wait to see what Earth can do.
    (Source)

    When we hear the term "feedback," most of us probably think about the feedback we get from teachers when we have to write essays or do other big projects. So in other words, "feedback" means critiques and criticisms, oftentimes harsh criticisms.

    When it comes to climate, Earth has its own way of providing feedback. No, it doesn't involve a red pen, and no Earth doesn't shout things like "lack of evidence," "comma splice," and "where's the negative?" That doesn't mean Earth's feedback isn't harsh, though.

    In fact, we'll learn in this lesson that positive feedback is a big reason Earth's climate changes as much as it does between glacial and interglacial periods. We could almost say that Earth's feedback makes the climate over react. We can all relate to that, though, right?

    After all who hasn't gotten frightened by all those red marks on a paper and overcompensated on the next paper?


    Sample Lesson - Reading

    Reading 14.14.03: How About Some Positive Feedback

    In the previous lesson, we learned about how Earth has gone back and forth between glacial and interglacial periods about every 100,000 years, in what scientists call Milankovitch Cycles.

    As we learned, these cycles are triggered by the eccentricity of Earth's orbit, the wobble in Earth's rotation, and the cycle of equinoxes. Notice that we said "triggered" here. It turns out that there are other things happening on Earth that factor into Earth's climate, too.

    After all, it's not like Earth is just a blank slate for the Sun's radiation to play with. Earth has a whole slew of systems already in place that help regulate our climate.

    In general, our atmosphere, oceans, and even our magnetic field help maintain our climate at a cozy temperature. In particular, the greenhouse effect, or how gasses in our atmosphere trap infrared heat, keeps Earth from getting too cold and undergoing massive temperature fluctuations.

    However, there are several of Earth's systems that create positive feedback when it comes to climate change, meaning that they amplify the effect of Milankovitch Cycles. The three main positive feedbacks we'll take a look at are 1) atmospheric water vapor, 2) the ice-albedo effect, and 3) greenhouse gasses.

    Without these three feedbacks, all the stuff going on with our orbit around the sun would result in a drastically different climate scenario for all of us here on Earth.

    It's Not the Heat, it's the Humidity

    About 70% of Earth is covered with water, so it's probably not surprising that the water cycle plays a huge role in our climate.

    As Earth goes through a Milkanovitch Cycle and starts to warm up, more water evaporates into the atmosphere. While we normally think of water vapor as pretty harmless, it turns out that it's actually a greenhouse gas.

    That means water vapor traps heat in our atmosphere, which in turn causes more water to evaporate from our oceans, which then means more heat is trapped in our atmosphere, which in turn means…well, we can all see where this is going.

    This positive feedback loop amplifies the warming effect as Earth enters interglacial periods. The opposite is also true as Earth goes into glacial periods. As the Earth starts to cool as a natural result of the Milkanovitch Cycle, less water is evaporated, meaning less heat is trapped in the atmosphere.

    Whichever way we're going—heating or cooling—water vapor in the atmosphere is a positive feedback. In fact, scientists believe that water vapor is the biggest positive feedback affecting Earth's natural climate change.

    Grab them Sunglasses

    Ever been skiing or snowboarding on a sunny day? It turns out that snow and ice are pretty glary. This doesn't only result in gnarly sunburns for unwary skiers. It also has a profound effect on our climate.

    Whereas most surfaces on Earth absorb sunlight and heat the planet up, Earth's polar icecaps and glaciers act like a mirror. They reflect sunlight right back out into space, which prevents Earth from absorbing that energy. This is called the ice-albedo effect.

    When Earth has colder winters, the polar ice caps and other glaciers grow larger, which means the Earth reflects more sunlight back out into space, resulting in an even colder climate. That, in turn, leads to larger ice caps, which leads to more sunlight reflected into space.

    Once again, we have positive feedback.

    On the flip side, ocean waters are dark and absorb a good amount of the energy from sunlight. That means when the climate warms, not only is there less snow and ice to reflect sunlight back into space, there's water there to suck all that sunlight up.

    So just like with water vapor in the atmosphere, the ice-albedo effect creates positive feedback both when the climate is cooling and warming.

    A Warm Earth is a Gassy Earth

    Ready to not be shocked? Greenhouse gasses in the atmosphere are another form of positive feedback, both when the climate is warming and when it is cooling. In that respect, it's exactly the same as water vapor and the ice-albedo effect. The mechanism is a bit more complex, though.

    The general trend is that warm climates release greenhouse gasses from carbon sinks, which in turn amplifies the greenhouse effect in the atmosphere. This, of course, leads to increased warming.

    On the flipside, cold climates trap greenhouse gasses in carbon sinks, which reduces the greenhouse effect. This leads to increased cooling.

    To understand why a warming Earth releases more greenhouse gasses, we need to take a gander at a couple of Earth's carbon sinks.

    The first is Earth's oceans. When water is colder, it can dissolve more CO2. When water is warmer, more CO2 gets released into the atmosphere. It's the same principle that makes warm sodas more fizzy than cold sodas. The only difference is that Earth's oceans are a soda pop that cover 70% of Earth's surface.

    The second carbon sink is the surface of land, particularly land that is permafrost, or "permanently" frozen during cold periods. When permafrost thaws out, all the dead plants and other organic materials that were trapped in the ice begin to decay. This releases both carbon dioxide and methane.

    Similarly, glaciers and permafrost can cover other natural pockets of methane that suddenly get released when that ice melts.

    Whichever of these carbon sinks we're looking at, the result is the same: greenhouse gasses are released when the climate warms, and trapped when the climate cools.

    The Carbon Heartbeat

    While Milankovitch Cycles are the driving force behind glacial and interglacial periods, the three positive feedback loops we just discussed causes Earth's climate to shift rather quickly.


    (Source)

    As the lower part of graph above shows, the changes between glacial and interglacial periods are abrupt. If it wasn't for the climate feedback loops, we'd probably expect to see the fluctuations be gradual and less severe.

    The other important fact to take note of in the graph above is how accurately atmospheric carbon (the top curve) correlates with global temperature (the bottom curve). The two are essentially mirror images of each other, going up and down like a heartbeat in a regular pattern.

    Understanding this sort of data about Earth's climate history allows us to analyze our current climate and make predictions about the future. To that end, we need to take note of one last important part of the graph above.

    Looking at carbon dioxide levels, we can see that it has had a natural fluctuation between 180 and 300 parts per million for the last 800,000 years. This is the natural fluctuation of carbon dioxide caused by Milankovitch Cycles and Earth's positive feedback loops.

    According to NASA, the concentration of carbon dioxide in our atmosphere reached 400 parts per million in 2013 and has continued to rise steadily, ever since. This abnormal increase is caused by human activity and is higher than it's been in the entirety of human history. No wonder scientists are alarmed.

    Recap

    In this reading, we learned that it's not all about the Sun and Earth's orbit when it comes Earth's climate over the last million or so years. Several positive feedback loops come into play, which make sudden climate change…well, much more sudden, and probably more severe, too.

    The positive feedback mechanisms include

    • Atmospheric water vapor.
    • The ice-albedo effect.
    • Greenhouse gasses.

    We also learned that CO2 has fluctuated between 180 and 300 parts per million for the last 800,000 years, but is currently above 400 parts per million.


    Sample Lesson - Activity

    Activity 14.03a: A Comic Tragedy

    We read a whole lot about feedback in this lesson. Well, here's some feedback that students have been hollering at teachers for decades: "Diagrams and pictures are worth a thousand words."

    Shmoop agrees. That's why we're asking you to draw a comic strip for this activity. Your goal is to create a comic strip that shows the before-and-after result of the three positive feedback mechanism that help climate change happen.

    You don't need to show a full warming and cooling cycle; simply showing how the feedback mechanisms either help the world heat up or how they help the world cool down will do the trick. You're welcome to be as creative and artsy as you want to be with your comic strip. Just make sure it includes the following elements:

    • At least one panel that shows the initial trigger of climate change: Milankovitch Cycles.
    • At least one before-and-after panel for each positive feedback mechanism, although you might find it helpful to have more than two panels for each of them.
    • Include captions, dialogue, or labels to help explain what's going on in each panel.
    • Give your comic a title.

    So to recap, your comic should include a minimum of 7 panels and clearly show how all three feedback mechanisms work. When you're all done, scan or take a pic of your comic and upload it below.


    Sample Lesson - Activity

    1. Which of the following is not a positive feedback mechanism affecting climate change?

    2. Positive feedback mechanisms cause climate change to happen more gradually: True/False?

    3. Which part of the carbon cycle is not a positive feedback for climate change?

    4. Water vapor acts as a greenhouse gas: True/False?

    5. Based on what we know about the ice-albedo effect, would we expect the widespread presence or absence of clouds to have any impact on climate change?