恆星是大質量、明亮的等离子体球。太陽是離地球最近的恆星,也是地球能量的來源。白天由於有太陽照耀,無法看到其他的恆星;只有在夜晚的時間,才能在天空中看見其他的恆星。恆星一生的大部分時間,都因為核心的核融合而發光。核融合所釋放出的能量,從內部傳輸到表面,然後輻射至外太空。幾乎所有比氫和氦更重的元素都是在恆星的核融合過程中產生的。
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