CAJ | 학술논문

水星是离太阳最近的类地行星,它有着类似月球的外表和类似地球的内部,其重要的构造特征主要表现在以下方面:广泛分布的撞击坑;全球线性构造(格子构造)体系;叶片状悬崖;与Caloris盆地相关的构造;局部的拉张构造,其中叶片状悬崖是仅存在于水星的独特构造.类地行星(除地球以外)的构造形迹主要形成于星球历史的早、中期,同时小行星体的构造演化通常被认为是行星热演化以及外部作用(如强烈撞击或者潮汐)共同作用的结果.
수성시리태양최근적류지행성,타유착유사월구적외표화유사지구적내부,기중요적구조특정주요표현재이하방면:엄범분포적당격갱;전구선성구조(격자구조)체계;협편상현애;여Caloris분지상관적구조;국부적랍장구조,기중협편상현애시부존재우수성적독특구조.류지행성(제지구이외)적구조형적주요형성우성구역사적조、중기,동시소행성체적구조연화통상피인위시행성열연화이급외부작용(여강렬당격혹자조석)공동작용적결과.
Mercury, the innermost terrestrial planet of the solar system, has the similar surface to the Moon and the similar interior to the Earth. It exhibits five important tectonic features: (1)pervasive impact craters, (2)a global grid system, (3)lobate scarps, only found on Mercury, (4)structures associated with the Caloris Basin and (5)local extensional feature. Most of the structural features of terrestrial planet except the Earth is formed in the early-middle history of the planets. The tectonic evolution of small planetary bodies is usually interpreted as the result of their thermal evolution with external perturbations such as large impacts or tidal effects. On this basis this paper discusses the tectonic history of Mercury by summaring and analysing its tectonic features.