Astronomers have measured the parallax of many nearby stars and determined their distances from Earth. However, if a star is too far away, its parallax is too small to be measured. With present technology, the parallax method gives reasonably accurate distance measurements for stars within a few hundred light-years. Astronomers have developed other ways to estimate distances to more-distant stars.

Properties of Stars

There are many different types of stars. Astronomers classify stars by their color, size, and brightness. Other important properties of stars include their chemical composition and mass.

Figure 10 The “Winter Triangle” can be seen in the late fall and winter in the eastern sky. It is made up of three of the brightest stars in the sky: Betelgeuse, Procyon, and Sirius A. Betelgeuse and the star Rigel belong to the constellation Orion.?

Applying Concepts Which star has a higher surface temperature, Betelgeuse or Sirius A?

Stars with dotted lines drawn to the three brightest stars that identify the "Winter Triangle" which is near the Orion constellation.
Color and Temperature

Have you ever looked closely at a candle flame? The hottest part of the flame near the wick is blue or white, while the cooler flame tip is orange. A propane torch flame is blue. Dying campfire embers are red. You can estimate the temperature of a flame from its color. In the same way, a star's color indicates the temperature of its surface. The hottest stars, with surface temperatures above 30,000 K, appear blue. The surfaces (photospheres) of relatively cool red stars are still a toasty 3000 K or so. Stars with surface temperatures between 5000 and 6000 K appear yellow, like the sun. As shown in Figure 10, the color differences between hot blue stars and cool red stars can be seen with the unaided eye. More precise measurements of stars' temperatures can be made by studying stars' spectra.

Brightness

When you are outside at night in a city, look for a row of street lights like the one in Figure 11. The closer lights look bright and the more distant lights look dim. However, the more distant lights are not really dimmer. They appear dim to you because, at a greater distance, their light is spread out over a greater area, so a smaller portion enters your eyes. The same is true for the light emitted by stars.

You might think that closer stars will always appear brighter than more-distant stars. Astronomers have discovered, however, that the brightness of stars can vary by a factor of more than a billion. So, stars that look bright may actually be farther away than stars that appear dim.

Although the sun appears to be the brightest star in our sky, it is really a star of only average brightness. The sun appears very bright to us because it is much closer than other stars. The brightness of a star as it appears from Earth is called its apparent brightness. The apparent brightness of a star decreases as its distance from you increases.


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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