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

“Triangulation”: Using Parallax to Measure Distance

Parallax has another important role in our lives: The fact that the amount of parallax we observe for an object gets smaller with increasing distance means that careful measurements of parallax allow us to calculate distances. This is very important in everyday life, because this technique — usually called “triangulation” — is used to measure distances for engineering and construction. And in astronomy, stellar parallax provides us with our only direct method for measuring distances to stars. Use this activity to help you understand how the method works.

Materials

  • Protractor
  • Graph paper
  • Ruler, meter stick or tape measure
  • Wire or twist tie
  • Tape
  • Pencil
Figure 3.3

Before starting, consider again Figure 3.3. In this activity, you will reproduce this type of observation at a much smaller scale, to measure distances within your classroom.

Step 1: Modify your protractor so that you can use it to measure angular position. Take your twist tie and bend one end into a slight ‘?’ shape, then use tape to attach the twist tie to the center of your protractor at a right angle, like so:

Step 2: Choose an object to which you will find the distance. Have you or your partner take a position as close to the object as possible and then pace out at least 10 steps straight away from it. You can take more than 10 steps, but you want to take at least 10 steps in order to be able to complete the experiment.

Step 3: Establish a baseline for observation. Looking back at Figure 1, notice how the two positions of the Earth in July and January represent points that are exactly opposite each other in the ‘circle’ of the Earth’s orbit. The distance between these two points is called the baseline, and it is from these two opposite positions that astronomers make their observations to measure the parallax of distant stars. You will need to set up a baseline from which to make your observations. Using a ruler or meter stick, measure out a 12-foot baseline, and mark the end positions A and B like the example shown here:

Orient your baseline so that it is perpendicular to the path that leads back to your object.

Step 4: Observe the position of the object and measure the angle from position A. Have partner 1 stand at point A of your baseline and hold the protractor at eye level. Keeping the edge of the protractor parallel to the baseline, have partner 1 move the protractor until the object appears aligned behind the twist tie, from the point of view of partner 1. Now have partner 2 move a pencil around the edge of the protractor until it aligns directly between the twist tie and the object, from the point of view of partner 1:

Partner 2 should note the angle on the protractor where the pencil aligns. Record this value as “angle A”.

Step 5: Observe the object and measure the angle from position B. Repeat step 4 from position B on the other end of the baseline. This time have partner 2 hold up the protractor and align the twist tie in front of the object. Have partner 1 move the pencil around the protractor as before, stopping when the twist tie, pencil and object are all aligned from the point of view of Partner 2. Record this value as angle B.

Step 6: Graph your data. On graph paper, draw a line to represent your baseline. Choose a scale where one square of graph paper equals one foot of real distance, so that the baseline you draw on your paper should be 12 squares long.

Place the protractor so that the flat edge is parallel to the baseline, with the center on point A. Make a mark for angle A that you measured at this position. Use a ruler to draw a straight line connecting point A on your baseline to the mark for angle A, and continue this straight line all the way to the top of the page.

Now place the protractor with the center on point B and mark angle B that you measured during the experiment. Use the ruler to draw a line connecting point B to the mark for angle B and continue this straight line all the way to the top of the page as well.

Step 7: Measure the distance. The point where the lines through angles A & B intersect represents the location of the object to which you were measuring the distance. Using your ruler, make a straight line connecting the point of intersection to the baseline. Count how many squares separate the point of intersection from the baseline and record this number as the distance. Since we chose a scale where one square of graph paper represents 1 foot of actual distance, the distance you measured on the graph paper equals the distance to your object in feet.

Now check your answer by using the measuring stick to measure the real distance – it should be very close to the distance you measured on the graph paper. Notice that you did not have to extend any sort of measuring device to the object to learn its distance – how cool that this is how astronomers can measure the distances to stars without having to actually travel to them!

Show Teachers Notes

The topic of parallax and distance goes beyond the NGSS for middle school, but it offers an excellent opportunity to connect with the mathematics and many applications of the distance measurement method more commonly called “triangulation.” In essence, this process simply requires measuring the apparent shift in angular position of an object due to parallax. This is how astronomers measure the distances to distant stars using parallax, and how surveyors measure distances to objects here on Earth. This activity helps students understand this method, formally called trigonometric parallax. Students will choose an object in the classroom and measure the distance to it by observing the position of an object and recording their viewing (or, parallax) angle as they observe the object from two different view points.

  • Note: Steps 6 and 7 of the activity use graph paper; while any graph paper can work, you may wish to print and use the graph sheet that we have posted here.

Student’s final distance sketches should look like the sketch to the right. Individual sketches and distances will vary based on the objects the students choose to observe and what angles they measure. However, the overall result should look similar to this.

Students mark the angles measured for A and B by centering the protractor on the ends of the baseline (blue line) as shown. They should then use a ruler to draw a line that connects the ‘A’ end of the baseline, through the mark for angle A, that continues up a good portion of the page (green lines). Do the same for angle B on the ‘B’ end of the baseline.

The dashed blue line represents the distance to the object that the students were observing. In this example, the distance is 13 feet.

Your students are free to establish a longer baseline (more than 12 feet) as the method will work the same, so long as they also make sure to mark their baseline distance accurately on the graph paper. If they choose a 14 foot baseline, they should mark a 14 square baseline on the graph paper. Likewise, if you should choose to do this experiment outside, you can have, for example, a 40 foot baseline. By choosing the correct scale of (for example) 2 feet per square of graph paper, you can use this method to measure farther distances.

Unless they are all observing the same object from the same baseline, student’s answers will vary quite a bit. It may be interesting to compare results between students to see how this method works accurately for different distances and angle measurements.

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