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Updated: Jul 9, 2026

09:31
Surface Properties of Synthesized Nanoporous Carbon and Silica Matrices
Published on: March 27, 2019
火星上の固体二酸化炭素の表面貯蔵庫が活発であることの観測証拠
M C Malin1, M A Caplinger, S D Davis
1Malin Space Science Systems, Post Office Box 910148, SanDiego, CA 92191-0148, USA.
まとめ
火星 火星 火星 火星
科学分野:
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
- 気候科学 気候科学
背景:
- 火星の南極の残留キャップは,ダイナミックな表面特性を示す.
- 以前のモデルは,観測された侵食率を完全に考慮していなかった.
研究 の 目的:
- 高解像度の画像を用いて,火星の南極の残層の変化を分析する.
- 観測された表面侵食を誘発する主要なメカニズムを決定する.
主な方法:
- 1999年と2001年の高解像度火星表面画像の取得と比較.
- 斜面の後退と特徴の構成の変化の定量分析.
主要な成果:
- 穴,山頂,丘の有意な変化が観察されました.
- 斜面は火星の1年に1〜3メートル後退した.
- 侵食率は,水氷ではなく,二酸化炭素の氷の亜鉛化と一致しています.
結論:
- 観測は,火星に固体二酸化炭素の大きな表面貯蔵庫が存在することを支持しています.
- 火星の気候は均衡状態ではないので,現在進行中の地球規模の気候変動を示しています.
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