| 恒星光谱的信息 |
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| 引用本文： | 潘文玲.恒星光谱的信息[J].西安科技大学学报,1996(1). |
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| 作者姓名： | 潘文玲 |
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| 作者单位： | 西安矿业学院基础部 |
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| 摘 要： | 通过光谱分析确定恒星的化学成分，测算恒星表面温度，并由多普勒红移验证星系的退行速度，为宇宙膨胀论奠定了基础；由引力红移确定光子的引力质量，使广义相对论的等效原理得到验证。
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| 关 键 词： | 夫琅和费线，多普勒红移，引力红移 |
INFORMATION OF THE STAR' S SPECTRUM |
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| Pan wenling.INFORMATION OF THE STAR' S SPECTRUM[J].JOurnal of XI’an University of Science and Technology,1996(1). |
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| Authors: | Pan wenling |
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| Abstract: | According to the spectrum analysis,the chemical composition of the star is determined,and the temperature of the star surface is calculated.The speed of the star system is verified with the aid of Doppler red moving establishing the foundating for the universe expanding theory.From the gravitational red moving the gravitational mass of photon is determinde,so the equvivalent principle of the generol theory of relativity is verified. |
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| Keywords: | Fraunhofer line Doppler red moving gravitational red moving |
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