日本地球惑星科学連合2016年大会

講演情報

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-PS13] 月の科学と探査

2016年5月22日(日) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*長岡 央(早稲田大学先進理工学部)、諸田 智克(名古屋大学大学院環境学研究科)、本田 親寿(会津大学)、西野 真木(名古屋大学宇宙地球環境研究所)

17:15 〜 18:30

[PPS13-P14] 嵐の大洋の3つの火山性地形群を貫く線形質量異常構造についての考察

*山本 圭香1春山 純一1大竹 真紀子1岩田 隆浩1石原 吉明1 (1.宇宙航空研究開発機構 宇宙科学研究所)

キーワード:月重力場、GRAIL、火成活動

In western part of the Oceanus Procellarum of the lunar nearside, there are several large-scale volcanic complexes, in which volcanic geographycal features are highly concentrated. In this study, Gravity Recovery and Interior Laboratory (GRAIL)-derived lunar gravity field data is used to investigate the geophysical relevance of the major volcanic complexes in the region. One of our concerns is whether the volcanisms of these complexes are caused by common factors or not. We estimated Bouguer gravity anomaly in the region and investigated the directions of the linear structure of the anomalies. The result shows that there are linear mass anomalies, which connect the mass anomalies at the volocano complexes of Aristarchus Plateau, Marius Hills and Flamstead Basin. The observed linear structures lie inward of the large quasi-rectangular pattern revealed by Andrews-Hanna et al., and much shallower than the pattern. Considering that, the observed linear structures should have been created later than the quasi-rectangular outer structure. After the quasi-rectangular pattern was created, magma rose to the surface through the cracks. The observed linear structure is supposed to be created through cooling of the overflowed magma. The geological units, which the linear structures go through, are younger than that of the outer quasi-rectangular pattern. The linear cracks created by cooling are weaker than other locations. Therefore, magma probably rose easier than in other area. That may be why the three currently observed volcano complexes lie on the same linear structure.