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...

How did gases get trapped in the interiors of Earth and other rocky worlds?

Perhaps you’ve noticed a couple of statements that might at first sound contradictory: We said that Earth and other rocky worlds were too small to pull in hydrogen gas as they formed, but we’ve also said that they had gas trapped in their interiors that formed atmospheres through outgassing. How can both be true?

The basic answer is that the “gas” trapped in their interiors was not hydrogen but heavier molecules (such as water and carbon dioxide), and these molecules were chemically attached to some of the rock that built these worlds. In other words, these “gases” joined the rocky worlds in the form of rock, which put them in the worlds’ interiors. The gases could then become separated from the rock by the effects of the internal heat within these worlds, and then released into atmospheres through volcanic outgassing.

However, this answer leads to another question that scientists still don’t fully know how to answer. According to models of solar system formation, it was too hot in the region where the rocky worlds formed for any gases to be chemically attached to rock. Therefore, scientists assume that all the trapped gases must have been brought in from cooler regions of the solar system, where it was possible for gas molecules to be attached to rock. This is a reasonable assumption, because models tell us that at least some particles from cooler regions of the solar system should have moved inward, where they could help form the rocky worlds. Moreover, we know that both asteroids and comets that formed farther from the Sun have such gases mixed with their rock (or rock/ice in the case of comets).

The question that scientists are still trying to answer is: Which region of the solar system did most of this material come from? That is, did the gases trapped in the rocky planets come primarily from the region of the asteroid belt or from the much more distant realm of the comets? The answer is not yet known, though recent evidence appears to be favoring the asteroid belt as the source of this gas.

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