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Updated: Jul 12, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
冥王星とハロンのIRASサーデンピットーサーベイ観測
まとめ
赤外線天文衛星観測により,冥王星が発見されました.
科学分野:
- 天文学と天体物理学について
- 惑星科学は惑星科学である.
背景:
- 冥王星とハロン星系観測
- 赤外線天文衛星 (IRAS) のミッションデータ
研究 の 目的:
- 冥王星とハロンの赤外線放射を分析する.
- 冥王星の表面と大気の特性を説明する.
主な方法:
- IRASによる冥王星-ハロン星系の2つの鋭い観測.
- 60マイクロメートルと100マイクロメートルで検出できます.
- 流量密度とスペクトルデータの分析
主要な成果:
- 冥王星-ハロン星系は,Serendipitous Surveyのソースとして検出されました.
- カラー調整した流量密度:581 +/- 58 mJy (60 μm) と721 +/- 123 mJy (100 μm)
- 冥王星は, +/-45度の緯度まで,暗い赤道帯と,明瞭なメタン氷の極帯を呈している.
結論:
- 冥王星上のメタン大気柱の豊富さの上限は~9m-amagatsである.
- メタンの大気の豊富さは,地上でのスペクトル学的な限界に匹敵する.
- IRASのデータは,冥王星の大気組成と表面の特徴に関する貴重な制約を提供します.
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