Description: 黑體輻射是來自理想化物體（黑體）的電磁輻射，該物體吸收落在其上的所有輻射，並以維持熱平衡狀態的速率重新發射輻射。根據已知的定律，黑體輻射的光譜完全由物體的溫度決定。大多數恆星在幾千開爾文的溫度下會發出類似黑體的光。與同步輻射和其他形式的 "非熱 "輻射形成對比。

Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

This is an automated transliteration of the simplified Chinese translation of this term

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