Earth & Space Science

Earth & Space Science

  • About This Project
    • Preface/About
    • Author/Contributors
    • For Investors/Donors
    • Teaching Guide
  • Ch 1 – Our Place in the Universe
    • Chapter Introduction
    • 1.1 Our Cosmic Address
    • 1.1.1 Overview
    • 1.1.2 What do we mean when we say “Earth is a planet”?
    • 1.1.3 What is our solar system?
    • 1.1.4 What is a galaxy?
    • 1.1.5 What is the universe?
    • 1.1 Review: Our Cosmic Address
    • 1.2 The Scale of Space
    • 1.2.1 Overview
    • 1.2.2 How Big is the Earth–Moon System?
    • 1.2.3 How Big is our Solar System?
    • 1.2.4 How far are the stars?
    • 1.2.5 How big is the Milky Way Galaxy?
    • 1.2.6 How big is the universe?
    • 1.2 Review: The Scale of the Universe
    • 1.3 Spaceship Earth
    • 1.3.1 How is Earth moving in our solar system?
    • 1.3.2 How is our solar system moving in the Milky Way Galaxy?
    • 1.3.3 How does our galaxy move relative to other galaxies in the universe?
    • 1.3 Review
  • Ch 2 – Understanding the Sky
    • Chapter Introduction
    • 2.1 Our Everyday View of the Universe
    • 2.1.1 What do we see in the local sky?
    • 2.1.2 What is the celestial sphere?
    • 2.1.3 Why do stars rise and set?
    • 2.1.4 Why do we see different constellations at different times of year?
    • 2.1 Review
    • 2.2 Seasons
    • 2.2.1 What causes the seasons?
    • 2.2.2 How do seasons differ around the world?
    • 2.2.3 Does the orientation of Earth’s axis ever change?
    • 2.2 Review
    • 2.3 Viewing the Moon: Phases and Eclipses
    • 2.3.1 Why do we see phases of the Moon?
    • 2.3.2 When do we see different phases of the Moon in our sky?
    • 2.3.3 Why do we always see the same face of the Moon?
    • 2.3.4 What are eclipses?
    • 2.3 Review
    • 2.4 Planets in the Night Sky
    • 2.4.1 How do we recognize planets in the sky?
    • 2.4.2 Why do the planets “wander”?
    • 2.4 Review
  • Ch 3 – How Science Discovered the Earth
    • Chapter Introduction
    • 3.1 The Ancient View of Earth
    • 3.1.1 How did the ancient Greeks learn that Earth is round?
    • 3.1.2 Why didn’t the ancient Greeks realize that Earth orbits the Sun?
    • 3.1 Review
    • 3.2 The Copernican Revolution
    • 3.2.1 How did the idea of Earth as a planet gain favor?
    • 3.2.2 How did Galileo seal the case for Earth as a planet?
    • 3.2 Review
    • 3.3 The Nature of Modern Science
    • 3.3.1 How does science work?
    • 3.3.2 What is a “theory” in science?
    • 3.3.3 What is the value of science?
    • 3.3 Review
    • 3.4 The Fact and Theory of Gravity
    • 3.4.1 What is gravity?
    • 3.4.2 How does gravity hold us to the ground and make objects fall?
    • 3.4.3 Why does gravity make planets round?
    • 3.4.4 How does gravity govern motion in the universe?
    • 3.4 Review
  • Chapter 4 – Planet Earth
    • Chapter Introduction
    • 4.1 A Planetary Overview
    • 4.1.1 What does Earth look like on the outside?
    • 4.1.2 What does Earth look like on the inside?
    • 4.1.3 How has Earth changed through time?
    • 4.1.4 How do we study the Earth?
    • 4.1 Review
    • 4.2 Earth System Science
    • 4.2.1 What are Earth’s four major systems?
    • 4.2.2 What drives Earth system changes?
    • 4.2.3 What IS energy and how do we measure it?
    • 4.2 Review
    • 4.3 Earth In the Context of Other Worlds
    • 4.3.1 How does Earth compare to other worlds of our solar system?
    • 4.3.2 Could there be life on other worlds?
  • Chapter 5 – Earth Through Time
    • Chapter Introduction
    • 5.1 Learning from Rocks and Fossils
    • 5.1.1 How do rocks form?
    • 5.1.2 What are fossils?
    • 5.1.3 How do we learn the ages of rocks and fossils?
    • 5.1 Review
    • 5.2 Shaping Earth’s Surface
    • 5.2.1 How do continents differ from oceans?
    • 5.2.2 What processes shape continents?
    • 5.2.3 What dangers do geological changes pose?
    • 5.2 Review
    • 5.3 Plate Tectonics — The Unifying Theory of Earth’s Geology
    • 5.3.1 What evidence led to the idea that continents move?
    • 5.3.2 How does the theory of plate tectonics explain Earth’s major features?
    • 5.3 Review
    • 5.4 A Brief Geological History of Earth
    • 5.4.1 What major changes mark Earth’s fossil record?
    • 5.4.2 What killed the dinosaurs?
    • 5.4.3 Have we humans started a new geological epoch?
    • 5.4 Review
  • Chapter 6 – Air and Water
    • Chapter Introduction
    • 6.1 Atmosphere and Hydrosphere
    • 6.1.1 What exactly is the atmosphere?
    • 6.1.2 How is water distributed on Earth?
    • 6.1.3 How does water cycle through the hydrosphere and atmosphere?
    • 6.1 Review
    • 6.2 Global Winds and Currents
    • 6.2.1 What drives global winds and currents?
    • 6.2.2 What is the general pattern of winds on Earth?
    • 6.2.3 What is the general pattern of ocean currents?
    • 6.2 Review
    • 6.3 Weather and Climate
    • 6.3.1 What is the difference between weather and climate?
    • 6.3.2 How and why does climate vary around the world?
    • 6.3.3 How do we measure and predict the weather?
  • Chapter 7 – Human Impact on the Climate
    • Chapter Introduction
    • 7.1 The Basic Science of Global Warming
    • 7.1.1 What is the greenhouse effect?
    • 7.1.2 How is human activity strengthening Earth’s greenhouse effect?
    • 7.1.3 How do we know that global warming is really happening and is human-caused?
    • 7.1.4 How does human-caused climate change compare to natural climate change?
    • 7.1 Review
    • 7.2 Consequences of Global Warming
    • 7.2.1 What are the major consequences of global warming?
    • 7.2.2 How do scientists predict future consequences of global warming?
    • 7.2.3 How will climate changes affect you and others around the world?
    • 7.2 Review
    • 7.3 Solutions to Global Warming
    • 7.3.1 What existing technologies could solve the problem of global warming?
    • 7.3.2 What future technologies might help even more?
    • 7.3.3 What does it take to implement a solution?
    • 7.3.4 What will your world look like AFTER we solve global warming?
    • 7.3 Review

I was wondering...

Why does the Coriolis effect create three sets of circulation cells, rather than some other number?

 
 
Great question! Remember that, without rotation, there would be just two large circulation cells, one for each hemisphere (see Figure 6.2.2–2). With rotation, the Coriolis effect comes into play, deflecting winds flowing toward the equator to the west. As you saw in Figure 6.2.2–3), this prevents wind from following a continuous path all the way from the poles to the equator, which is the reason that rotation forces each single circulation cell to split. But why does each of them split into three cells, rather than some other number of cells?

View Figure 6.2.2-2


View Figure 6.2.2-3

The answer has to do with the strength of the Coriolis effect. Figure 6.2.2–3 shows that, for Earth, if you start with winds from the poles, the Coriolis effect will have diverted these winds fully to the west by the time they get about 1/3 of the way to the equator (which means to about 60° latitude in each hemisphere). It is this 1/3 of the way that explains why the single large cell splits into three cells on Earth. In other words, the split into three cells is a consequence of the particular strength of the Coriolis effect on Earth.

This brings us to a follow-up question, which is: What determines the strength of the Coriolis effect? If you look back at the way the Coriolis effect works on a merry-go-round (see Figure 6.2.1–4), you’ll probably realize that one factor is the speed of rotation: the faster the rotation, the stronger the Coriolis effect. For planets, a second factor is the strength of gravity, with stronger gravity meaning a stronger Coriolis effect. To summarize: The strength of the Coriolis effect on a planet depends on the planet’s gravity and rotation rate.

View Figure 6.2.1-4

We can use this idea to explain how wind patterns on other planets compare to those of Earth. Let’s take two examples (photos below).

First, consider Venus. Venus has almost the same strength of gravity as Earth, but it rotates extremely slowly (taking about 243 days for a single rotation). As a result, Venus has such a weak Coriolis effect that it has a circulation pattern like that for a non-rotating planet, with just one large cell in each hemisphere. These cells carry heat from the equator to the poles so effectively that Venus has nearly the same temperature at all latitudes.

Next, consider Jupiter. Jupiter has much stronger gravity than Earth and it rotates very fast (one rotation takes less than 10 hours). This gives it a very strong Coriolis effect, which splits each hemisphere into many more than Earth’s three circulation cells. In fact, this is why Jupiter has a “striped” appearance. In essence, each stripe represents a different circulation cell. (The Great Red Spot is a giant storm, so it breaks up the general pattern.)

venus
Venus rotates very slowly, giving it such a weak Coriolis effect that it has the circulation pattern of a non-rotating planet. Credit: NASA/Pioneer Venus Orbiter.

Jupiter
Jupiter’s strong gravity and fast rotation give it a much stronger Coriolis effect than Earth, causing its circulation in each hemisphere to split into more than the three cells found on Earth. These many cells are the reason for Jupiter’s “striped” appearance. Credit: NASA/Hubble Space Telescope.

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Figure 6.2.2-2

Figure 6.2.2–2 – This diagram shows a model of what Earth’s global wind patterns would look like if Earth were not rotating. The atmosphere would have just two large circulation cells carrying heat from the equator toward the poles. Credit: Adapted from The Cosmic Perspective.

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Figure 6.2.2-3

Figure 6.2.2–3 – This figure shows how Earth’s rotation changes the flow of surface winds through the Coriolis effect. Notice that the winds can no longer flow straight from the poles all the way to the equator.Credit: Adapted from The Cosmic Perspective.

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Figure 6.2.1-4

coriolis merry go round demo
Figure 6.2.1–4 – The Coriolis effect explains why a ball rolled on a merry-go-round appears to follow a curved path. Credit: Adapted from The Cosmic Perspective.
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