26.5 The Expanding Universe

Have you ever wanted to use a time machine to travel back in time? Telescopes are like time machines because they show what happened in other parts of the universe in the distant past. When you observe a star that is ten light-years away, you are seeing the star as it was ten years ago. This is because light took ten years to travel from the star to Earth. Images of galaxies that are billions of light-years away show how these galaxies looked billions of years ago.

Figure 24 Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when a galaxy moves away from Earth. Inferring How would the spectrum of a galaxy that is slowly moving away from Earth compare to one that is moving away much more quickly?

Diagram depicting spectrum of a galaxy moving away from the Earth slowly versus moving away quickly.

Hubble's Law

Recall from physics that as a sound or light source moves toward or away from an observer, its frequency and wavelength appear to change. This apparent change in frequency and wavelength is known as the Doppler effect. The Doppler effect can be used to determine how fast stars or galaxies are approaching or moving away from Earth. When a star or galaxy is approaching Earth, the lines in its spectrum are shifted toward the shorter (bluer) wavelengths, as shown in Figure 24. When the star or galaxy is moving away, the lines in its spectrum shift toward the longer (redder) wavelengths. The larger the observed shift, the greater is the speed of this movement.

In the mid-1920s, the American astronomer Edwin Hubble studied many galaxies at different distances from Earth. In 1929, Hubble announced his discovery: the light from most galaxies undergoes a red shift—that is, their light is shifted toward the red wavelengths. This red shift showed that, remarkably, nearly all galaxies are getting farther away from Earth.


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Table of Contents

Physical Science CHAPTER 1 Science Skills CHAPTER 2 Properties of Matter CHAPTER 3 States of Matter CHAPTER 4 Atomic Structure CHAPTER 5 The Periodic Table CHAPTER 6 Chemical Bonds CHAPTER 7 Chemical Reactions CHAPTER 8 Solutions, Acids, and Bases CHAPTER 9 Carbon Chemistry CHAPTER 10 Nuclear Chemistry CHAPTER 11 Motion CHAPTER 12 Forces and Motion CHAPTER 13 Forces in Fluids CHAPTER 14 Work, Power, and Machines CHAPTER 15 Energy CHAPTER 16 Thermal Energy and Heat CHAPTER 17 Mechanical Waves and Sound CHAPTER 18 The Electromagnetic Spectrum and Light CHAPTER 19 Optics CHAPTER 20 Electricity CHAPTER 21 Magnetism CHAPTER 22 Earth's Interior CHAPTER 23 Earth's Surface CHAPTER 24 Weather and Climate CHAPTER 25 The Solar System CHAPTER 26 Exploring the Universe Skills and Reference Handbook