日本地球惑星科学連合2023年大会

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[J] オンラインポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS06] 月の科学と探査

2023年5月26日(金) 15:30 〜 17:00 オンラインポスターZoom会場 (3) (オンラインポスター)

コンビーナ:西野 真木(宇宙航空研究開発機構宇宙科学研究所)、鹿山 雅裕(東京大学大学院総合文化研究科広域科学専攻広域システム科学系)、仲内 悠祐(宇宙航空研究開発機構)、小野寺 圭祐(東京大学地震研究所)

現地ポスター発表開催日時 (2023/5/26 17:15-18:45)

15:30 〜 17:00

[PPS06-P21] The Lava Tube Candidate in Lunar North Oceanus Procellarum Region: The Structure and the Origin Process

*chong zheng1 (1.Wuhan University)

キーワード:Moon, Lava tube, Gravity

Lunar lava tubes are sinuous rilles without collapse portions, and as natural caves, are priority candidates for lunar exploration. Gravity data obtained by Gravity Recovery and Interior Laboratory (GRAIL) mission could allow us to study these sub-surface structures. A complex system of sinuous rilles potentially containing lava tubes is found in northern Oceanus Procellarum (NOP). Thus, we applied a gravity inversion algorithm and a forward constraint in this region to rebuild the density structure of a potential lava tube, Rima Mairan lava tube. The results indicate that this lava tube candidate is at a depth of 7.5 km beneath the lunar surface, and has a bowl-shape cross-section with a width of 3.5 km ~ 4 km and a height of 1.13 km ~ 1.33 km, as constrained by the gravity anomaly amplitude (~-20 mGal) on the surface. Furthermore, a positive quasi-circular gravity anomaly at the western end of the Rima Mairan lava tube may shed a light on the origins of this geological structure and may indicate additional mechanisms of lava transportation.