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

Units of Mass and Weight

Mathematically, mass and weight are related as follows:

weight = mass x the acceleration of gravity

This means that mass and weight must have different units (because the units of weight are the units of mass times the units of acceleration). However, the metric system and the U.S. unit system handle these units a bit differently, so let’s look at each separately.

Metric Units of Mass and Weight
In the metric system, the standard unit of mass is the kilogram. In other words, if a scale (on Earth) says that you “weigh” 60 kilograms, it is really telling you that you have a mass of 60 kilograms. To calculate your weight, we must multiply by the acceleration of gravity, which for Earth we approximate as 10 m/s2:

The units of weight probably look pretty strange, and you would technically read them as “kilogram-meters per second squared.” Fortunately, this combination of units is given a special name: the “newton.” In other words, if you have a mass of 60 kilograms, your weight is about 600 newtons.

To summarize, when we put an object (on Earth) on a metric scale that reads kilograms, the scale is actually telling us the object’s mass, not its weight. To get its weight, we must multiply by the acceleration of gravity, which will give us a weight in newtons. (You might notice that this also means that metric scales that read kilograms give accurate masses only on Earth; if you wanted to take a metric scale to another planet, you would be better off with one that tells you weight in newtons.)

Example: Metric Mass and Weight on the Moon. Suppose that a scale on Earth tells you that you have a mass of 60 kilograms. What is your mass and your weight on the Moon? Recall from the earlier Do the Math box that the acceleration of gravity on the Moon is about 1/6 that on Earth.

Answer to Example

  • For mass: An object’s mass is the same everywhere, since it depends only how much matter it contains. Therefore, if you have a mass of 60 kilograms on Earth, you would have the same mass of 60 kilograms on the Moon.
  • For weight: Because weight is mass x the acceleration of gravity, and the acceleration of gravity on the Moon is about 1/6 that on Earth, your weight on the Moon would be about 1/6 of your weight on Earth. We’ve already found (above) that your weight on Earth is about 600 newtons. Therefore, your weight on the Moon is 1/6 of that, or about 100 newtons.

U.S. Units of Mass and Weight

In the United States, we commonly talk about pounds instead of kilograms. Technically, however, pounds are a unit of weight, not of mass. In other words, if you get on a scale and it reads 120 pounds, then you have a weight of 120 pounds. So what is your mass? To answer, we start with our earlier definition:

weight = mass x the acceleration of gravity

Finding mass therefore requires a little bit of algebra. First, we first reverse the left and right sides

mass x the acceleration of gravity = weight

Next, we divide both sides by the acceleration of gravity to find:

mass = weight/ the acceleration of gravity

In other words, if you know your weight in pounds, then you would find your mass by dividing by the acceleration of gravity, which in U.S. units is 32 ft/s2. The result would be your mass in units called “slugs.”

So we’ll stop here, because most people don’t like thinking of themselves in terms of slugs. You might also notice that this is yet one more reason why scientists always prefer to work with the metric system.

Show Teachers Notes

This optional box covers a subtlety about mass and weight that will be important when students go on to study physics in high school, which is that, as a result of the way the U.S. and metric systems of units developed, they handle mass and weight differently:

  • In the metric system, we commonly talk in terms of kilograms, which technically are a unit of mass, not weight.
  • In the U.S. system, we commonly talk in terms of pounds, which are a unit of weight, not mass.

As long as we only consider objects on Earth, we can generally ignore this subtlety. Indeed, that is exactly what we do when we use the standard conversion of 1 kilogram = 2.2. pounds. However, for scientific work – or for any situation that is not on the surface of Earth (such as in space or on the Moon) — the distinction becomes very important. As the box demonstrates, it’s easy to work with the distinction in the metric system, where masses in kilograms can be converted to weights in newtons. In contrast, the U.S. system would force you to use the ridiculous-sounding units of “slugs” — which is one more reason why virtually all scientific work is done in metric units.

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