ポインティング・ロバートソン効果
1. Poynting–Robertson effectThe Poynting–Robertson effect, also known as Poynting–Robertson drag, named after John Henry Poynting and Howard Percy Robertson, is a process by which solar radiation causes a dust grain in the Solar System to slowly spiral into the sun. The drag is essentially a component of radiation pressure tangential to the grain's motion. Poynting gave a description of the effect in 1903 based on the "luminiferous aether" theory, which was superseded by the theories of relativity in 1905–1915.
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Read “Poynting–Robertson effect” on English Wikipedia
Read “ポインティング・ロバートソン効果” on Japanese Wikipedia
Read “Poynting–Robertson effect” on DBpedia
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