火星の「リゾート風」ビーチの痕跡を発見(Gulf of Mars: Rover finds evidence of ‘vacation-style’ beaches on Mars)

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2025-02-24 ペンシルベニア州立大学(PennState)

ペンシルベニア州立大学(Penn State University)を含む国際研究チームは、中国の火星探査車「祝融号(Zhurong)」のデータを用いて、火星の北部に古代の海が存在した可能性を示す地下の岩層を特定しました。この研究は、火星がかつて大規模な水域を持ち、生命が存在し得る環境であったことを示唆しています。祝融号は2021年にユートピア平原(Utopia Planitia)に着陸し、地中レーダーを使用して地下の岩石構造を調査しました。その結果、地球の海岸線に見られる「前浜堆積物(foreshore deposits)」と呼ばれる、海洋に向かって傾斜する層状構造が確認されました。これらの発見は、火星がかつて湿潤で温暖な気候を持ち、数千万年にわたり生命に適した環境であった可能性を示しています。

<関連情報>

火星で古代の海洋沿岸堆積物が画像化される Ancient ocean coastal deposits imaged on Mars

Jianhui Li, Hai Liu, Xu Meng, +8, and Guangyou Fang
Proceedings of the National Academy of Sciences  Published:February 24, 2025
DOI:https://doi.org/10.1073/pnas.2422213122

火星の「リゾート風」ビーチの痕跡を発見(Gulf of Mars: Rover finds evidence of ‘vacation-style’ beaches on Mars)

Significance

Various observations suggest that large amounts of liquid water once existed on the Martian surface, however, the nature and fate of this water are uncertain. Through radar data gathered by the Zhurong Rover, we identify extensive dipping deposits in the subsurface of southern Utopia Planitia. These deposits have structures similar to those of Earth’s coastal sediments. This finding implies the past existence of a large water body, supporting the hypothesis of a past ocean in the northern plains of Mars.

Abstract

The northern lowlands of early Mars could have contained a significant quantity of liquid water. However, the ocean hypothesis remains controversial due to the lack of conclusive evidence from the Martian subsurface. We use data from the Zhurong Rover Penetrating Radar on the southern Utopia Planitia to identify subsurface dipping reflectors indicative of an ancient prograding shoreline. The reflectors dip unidirectionally with inclinations in the range 6° to 20° and are imaged to a thickness of 10 to 35 m along an uninterrupted 1.3 km northward shoreline-perpendicular traverse. The consistent dip inclinations, absence of dissection by fluvial channels along the extended traverse, and low permittivity of the sediments are consistent with terrestrial coastal deposits—and discount fluvial, aeolian, or magmatic origins favored elsewhere on Mars. The structure, thickness, and length of the section support voluminous supply of onshore sediments into a large body of water, rather than a merely localized and short-lived melt event. Our findings not only provide support for the existence of an ancient Martian ocean in the northern plains but also offer crucial insights into the evolution of the ancient Martian environment.

1701物理及び化学
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