関連する実験動画
Updated: Jun 21, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
ボイジャー1号とボイジャー2号との間の木星の雲の分布: 5マイクロメートルの画像から得られた結果
まとめ
木星の赤外線観測は,地球規模の雲のパターンを明らかにし,ボイジャー2のターゲティングを助けました. これらの発見は,最適なミッション画像と赤外線実験のための木星の雲の分布を予測するのに役立ちました.
科学分野:
- 惑星科学は惑星科学である.
- 赤外線天文学の天文学
- ジョビアン・システム (Jovian System) とは
背景:
- 地上からの観測は,ボイジャーのような宇宙ミッションを支援する上で極めて重要です.
- 赤外線画像は,惑星の大気動態の洞察を提供します.
研究 の 目的:
- ボイジャー2号のフライトバイの前に木星の5マイクロメートルの赤外線画像を取得するために.
- ボイジャー2号が木星の雲の覆いをマッピングすることで標的の選択を支援する.
主な方法:
- パロマー5メートル望遠鏡とNASA赤外線望遠鏡施設を利用した.
- 1979年5月に5マイクロメートルの波長領域で赤外線画像を取得しました.
主要な成果:
- 木星全体で5マイクロメートルの流動分布の変動を観測した.
- 木星のベルトの曇りと晴れのグローバルパターンを特定しました.
結論:
- データは,ボイジャー2の遭遇のために木星の雲の分布を予測した.
- 標的型画像と赤外線実験を,遮りやすい雲が少ない地域に可能にした.
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