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Updated: Jul 11, 2026

11:20
Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
"パイオニア・サターン"のイメージング・フォトポリメーター
まとめ
パイオニア11号は,土星のF環と新しい衛星を発見した. 観測によりリングの構造,粒子の大きさの推定,土星の次元が精製され,惑星科学に影響を与えました.
科学分野:
- 惑星科学は惑星科学である.
- 天文学 天文学
- 天体物理学 天体物理学
背景:
- パイオニア11号のイメージングフォトポリメーターは,土星の詳細な観測を提供した.
- 土星の環と大気に関する以前の知識は限られていた.
研究 の 目的:
- 土星,その環,タイタンについてイメージング,光度測定,極度測定を行う.
- 土星のシステムに関する新しい特徴を発見し,既存のデータを精査する.
主な方法:
- パイオニア11号の2.5センチの望遠鏡を搭載したイメージング光ポリメーターを使用した.
- 1979年8月と9月に2週間連続観察を行った.
主要な成果:
- 新しい環 (F環) と衛星 (1979 S 1) を発見した.
- リングの区切りとギャップの名称が再定義され,Enckeギャップの幅が測定されました.
- 推定平均粒子の大きさはリング (~15メートル) と土星の大きさです.
- 極度測定データを用いて土星の大気構造を分析した.
結論:
- Fリングの存在と位置が確認されました.
- 土星の環系は,これまで知られていたよりも多くの詳細を披露しています.
- パイオニア11号のデータは,土星の大気と環粒子の性質に関する重要な洞察を提供した.
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