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

Take It To The Next Level

Mass-Energy (E = mc2)

In the process of discovering his special theory of relativity, Einstein also discovered that mass itself is a form of potential energy, often called mass-energy. The amount of potential energy contained in mass is described by Einstein’s famous equation

E = mc2
where E is the amount of mass-energy contained in the object, m is the mass of the object, and c is the speed of light.

Because the speed of light is very fast (300,000 kilometers per second, which is the same as 300,000,000 meters per second), the number c2 is a very large number. Therefore, Einstein’s equation tells us that a small amount of mass contains a huge amount of stored energy. For example, the energy released by a 1-megaton H-bomb comes from converting only about 0.1 kilogram of mass (about 3 ounces—a quarter of a can of soda) into energy.

The energy released by this H-bomb came from converting only about 0.1 kilogram of mass into energy.

However, even though mass contains an enormous amount of energy, only in relatively rare circumstances is this energy “useful” in the sense of causing movement, heating, or transformation into other forms of energy. The reason is that mass generally stays unchanged. In nature, the only major exceptions occur in:

  • Radioactive decay , in which an atomic nucleus undergoes changes that result in the conversion of a small amount of the nucleus’s mass into energy.
    Note that one form of radioactive decay is nuclear fission, in which a large atomic nucleus (such as uranium) is split apart into smaller nuclei. Humans have learned to induce fission, and it is the energy source used in nuclear bombs and also in all current nuclear power plants.
  • Nuclear fusion, which is the power source of stars: The fusion process combines (fuses together) small atomic nuclei to make larger ones, again with a small amount of the original mass being converted to energy in the process. Humans have learned to use fusion in hydrogen bombs (H-bombs), but have not yet developed it as a power source.

As we’ve discussed, radioactive decay is a source of heating for Earth’s interior, but other than that we can generally ignore mass-energy in Earth science.

Three More Notes

For those who really want to “take it to the next level,” here are three more notes you might find interesting about Einstein’s formula E = mc2.

Note 1: You can use the formula to calculate the mass-energy contained in any amount of mass. If you use standard units, then you should put the mass m in kilograms, the speed of light in meters per second (c = 3 108 m/s), and the calculation will then give the energy E in joules.

Example: Suppose that you could somehow convert a 1 kilogram rock completely into energy. How much energy would it release?

Solution: We simply apply the formula with m = 1 kg:

This is an enormous amount of energy; in fact, we’d need to burn about 7.5 billion liters of gasoline to generate the same amount of energy for cars, which is as much gasoline as used by all cars in the United States combined for about a week.

Note 2: As discussed above, radioactive decay, nuclear fission, and nuclear fusion all convert only a small fraction of the original mass into energy. So you might wonder: Are there any processes that can completely convert mass into energy? The answer is yes: There is one process that completely converts mass into energy, and it is called matter–antimatter annihilation. The term antimatter refers to subatomic particles that are sort of like mirror opposites of ordinary matter particles. For example, an antielectron (also called a positron), is just like an ordinary electron except it has a positive electrical charge instead of a negative electrical charge. When any particle of matter meets its corresponding particle of antimatter (such as an electron meeting an antielectron), the particles completely annihilate each other, converting all of the mass into energy.

This diagram illustrates how a collision between an electron and antielectron converts their masses completely into energy.

Note 3: Although we more commonly think of E = mc2 as telling us how much energy we can get from mass, the fact that it has an “=” sign tells us that mass and energy can be converted in either direction. In fact, if you can concentrate enough energy in a very small space, the energy can spontaneously turn into subatomic particles of mass. This is why physicists build the gigantic machines known as particle accelerators, such as the Large Hadron Collider in Europe: They accelerate known particles (such as electrons or protons) to extremely high speeds, so that collisions between them release highly concentrated bursts of energy. In the aftermath of these collisions, some of the released energy spontaneously turns into new particles, and sometimes these new particles are of a type that had never before been discovered.

The Large Hadron Collider (LHC) circulates subatomic particles around a 27-kilometer loop that is mostly underground. The aerial photo shows the underground path of the loop near Geneva, Switzerland. The inset illustrates one of the detectors that records what occurs in a particle collision; you can see its large size from the people shown for scale.

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