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 do you say it will probably never be possible to predict weather more than a couple weeks out?

A century ago, we couldn’t predict the weather well even a day or two ahead of time. Today, weather forecasts are fairly reliable for several days in advance, and most weather web sites will give you a 10-day forecast (though these longer term forecasts often prove to be inaccurate). So you might guess that as our computer models improve in the future, we’ll be able to predict the weather much further into the future. However, there’s a limit to how far out we can expect weather predictions to be accurate, as a result of something that is sometimes called “the butterfly effect.” (Important note: As discussed below, this limitation applies to weather prediction, but not to climate prediction.)

The first step in understanding the butterfly effect is to understand a little bit about how scientists make predictions. In general terms, scientific prediction always requires knowing two things:

(1) the current state, or “initial conditions,” of a system

(2) the laws that govern how the system is changing.

Knowing both things is easy for a simple system, like that of a moving car. For example, if you know where a car is and how fast and in what direction it is traveling, you can predict where it will be a few minutes from now. But prediction is far more difficult for a complex system like weather, which is ultimately created by the motions of countless individual atoms and molecules.

Scientists therefore attempt to predict the weather by creating a “model world.” For example, suppose you overlay a globe of Earth with graph paper and specify the current temperature, pressure, cloud cover, and wind within each square; these are your initial conditions, which you can input into a computer along with a set of equations (physical laws) describing the processes that can change weather from one moment to the next. We’ll discuss such models further in the context of climate in Section 7.2.2, but you can get a quick overview by studying Figure 7.2.2–1, which is shown below.

Figure 7.2.2-1 – This illustration summarizes how a climate model works. (Weather models work essentially the same way.) A computer program represents Earth’s climate with a set of small elements (shaped roughly like cubes here). In each element, scientists start with data from some point in time to represent “initial conditions,” then “run” the model by using equations that represent the physical processes that can change the initial conditions. Click the image to open a zoomable graphic that illustrates the process for individual model elements. You may also wish to watch this video that discusses the idea. Credit: NOAA, Zofostro Science.

Once you’ve set up your initial conditions and created your model world, you can use your model to predict the weather for the next month in some particular location, such as New York City. The model might tell you that tomorrow will be warm and sunny, with cooling during the next week and a major storm passing through a month from now.

Now, suppose you run the model again, but you make one small change in the initial conditions, such as a small change in the wind speed somewhere over Brazil. This very slight change in a single initial condition will not affect the weather prediction for tomorrow in New York City at all, and it is unlikely to have any effect on the prediction for next week’s weather either. However, the laws governing weather can cause tiny changes in initial conditions to be greatly magnified over time. As a result, when you compare what your two model runs (your first one and the one with the small change in wind over Brazil) predict for New York’s weather a month from now, you may find the two predictions to be very different; for example, one model might predict cold and rain a month from now, while the other predicts warm and sunny.

The fact that tiny changes in initial conditions can lead to huge changes in predictions a month later explains why weather models can never be reliable more than a few weeks out. In essence, the problem is that we’ll never be able to know the initial conditions perfectly enough to make reliable predictions for, say, a month in the future. That is why the problem is called the “butterfly effect”: If initial conditions change by as much as the flap of a butterfly’s wings in one part of the world, the resulting long-term predictions may be very different even for far-away places in the world.

Keep in mind that the fact that weather predictions become unreliable does not mean that climate predictions will have the same problem. The reason is that even though the butterfly effect may make a prediction for a particular time and place (such as New York City in one month) unreliable, it will not affect predictions for the average weather that a region would experience over many years. That is why climate prediction is actually much easier and more reliable than weather prediction .

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