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Updated: Feb 18, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
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冥王星 の 大気 を 暖める 霧 が その 寒い 温度 を 説明 し て いる
Xi Zhang1, Darrell F Strobel2, Hiroshi Imanaka3,4
1Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, California 95064, USA.
Nature
|November 17, 2017
まとめ
冥王星の冷たい温度を説明するのは ガスではなく 霧状の大気です ハーゼ粒子は放射線のバランスを支配し,将来の望遠鏡検出のために中赤外線の波長で冥王星を明るくします.
科学分野:
- 惑星科学
- 大気物理学
- 天体物理学
背景:
- 冥王星の大気は予想外に冷たいので 理論的な予測に逆らっています
- 低温の原因は不明な冷却メカニズムだと疑われた.
- 水蒸気は以前,冷却液として提案されていたが,必要な超飽和レベルは熱力学的に不可能であった.
研究 の 目的:
- 冥王星の気温を調節する 大気中の霧の役割を調査する
- 観測された熱プロフィールについて,ハズ粒子が説明できるかどうかを判断する.
- 冥王星の放射能バランスを再評価する
主な方法:
- 冥王星の大気温に関する観測データの分析
- 霧粒子とガス分子の 太陽熱加熱と熱冷却率のモデル化
- ハーゼの影響と無影響を伴う放射伝導均衡モデルの比較.
主要な成果:
- ハーゼ粒子はガスの分子よりも太陽熱と熱冷却の速度がかなり高い.
- 冥王星の大気放射のバランスを 700kmの高さまで支配しています
- 700km以上では 熱伝導により同熱大気が形成されます
結論:
- 冥王星の大気温は 主にガス分子ではなく 霧粒子によって調節されます
- 太陽系の惑星の大気の中で 独特なエネルギーバランスです
- 冥王星は 将来の望遠鏡で検出可能な 中赤外線波長で 顕著に明るく見えます
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