月球风暴洋地区火山穹窿建造的特征和成因

月球火山穹窿建造的特征和成因的研究一直是国际月球科学领域的研究热点和难点，是月球热演化历史的研究一个瓶颈。本项目以月球风暴洋地区三个大型火山穹窿群（Marius Hills, Mons Rümker和Aristarchus）为研究对象，以近年来新获得的高分辨月球影像（CE-2CCD,LROC/WAC/NAC）、激光测高（CE-1 LAM,LRO/LOLA）和多光谱与高光谱数据(CE-1 IIM, Chandrayaan-1 M3)，）等为研究数据，对火山穹窿区进行详细的形貌学、组成成分和年代学研究，填制大比例尺火山穹窿区地质图。在此基础上，运用比较行星火山学的方法，探讨形成这些火山穹窿群的岩浆性质和热演化过程，火山穹窿区岩浆活动对月海玄武岩充填的贡献，为深化认识月海区岩浆活动特征和热演化历史、开展比较行星火山学研究开辟新途径和提供直接证据。

The characteristics and origin of volcanic dome complex on the Moon are essentially important for understanding lunar volcanism and thermal history, but have not well studied and has been a bottleneck for constraint lunar thermal history. This study will study the morphology, rock/lava's properties, mineral composition and ages of three major volcanic dome complexes in the Oceanus Procellarum e.g. Mons Rümker, Marius Hills, Aristarchus Plateau, by using newly obtained high resolution imagery (CE-1CCD,CE-2CCD,SELENE TC, LROC/WAC/NAC), laser altimetry data（CE-1 LAM,LRO LOLA）and multispectral, and high-spectral data (CE-1 IIM, Chandrayaan-1 M3, Clementine UVVIS).Based on integrated morphological and compositional studies, we would produce new and large scale geological maps of these dome complexes, provide quantitative and semi-quantitative constraints on magma properties of these volcanoes, establish thermal evolution model and provide new solid evidences for comparative planetary volcanology study, and provide essential data and service for the ongoing Chinese Lunar Chang-E missions.