26.1The Sun
 Key Concepts
How does the sun produce energy?
Why does the sun remain stable over time?
What is the structure of the sun?
What are some features of the sun's atmosphere?
 Vocabulary
core
radiation zone
convection zone
photosphere
chromosphere
corona
solar wind
sunspots
prominences
solar flare
 Reading Strategy
 Building Vocabulary   Copy the table below. Then, as you read, write a definition of each vocabulary term in your own words. Add seven more rows to complete the vocabulary list.
 

You know that flowers like the ones in Figure 1 need sunlight. In fact, almost all life on Earth depends on sunlight. Without the sun's radiation, Earth would be a cold, dark, and lifeless planet. But what exactly is the sun? Scientists have learned that the sun is a glowing ball of gas. The sun is extremely hot, about 15 million K at its center and 5800 K at its surface. At such temperatures, most of the atoms in the sun have lost most of their electrons, forming a plasma of ionized gas. About 70 percent of the sun's mass is hydrogen and 28 percent is helium.

Figure 1  The sun gives off tremendous amounts of energy. Plants on Earth use sunlight directly in photosynthesis.

 
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