Last Updated:2025/12/06
Sentence

黒体の単位面積あたりの、全波長にわたる単位時間当たりの放射エネルギーが熱力学的温度の4乗に比例するという法則は、天文学者が放射から恒星の表面温度を推定することを可能にします。

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The Stefan-Boltzmann law allows astronomers to estimate a star's surface temperature from its emitted radiation.

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The Stefan-Boltzmann law allows astronomers to estimate a star's surface temperature from its emitted radiation.

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Stefan-Boltzmann law

Proper noun
Japanese Meaning
黒体の表面から全波長にわたって放射される単位面積あたりのエネルギーが、黒体の熱力学的温度の4乗に比例するという物理法則。
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黒体の単位面積あたりの、全波長にわたる単位時間当たりの放射エネルギーが熱力学的温度の4乗に比例するという法則は、天文学者が放射から恒星の表面温度を推定することを可能にします。

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