比如,NAC像显示出一种被称为瓣状陡坡(lobate scarps)的小型山脊的全月分布网络,这种陡坡由垂直地质构造运动形成,表明月球自其诞生以来就一直在缓慢地沉降和收缩。
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The shrinkage has wrinkled parts of the moon's surface like a raisin, creating pinched formations called lobate scarps…
月球的收缩使月球部分表面像葡萄干那样起皱,从而形成为“瓣状陡坡”…
The intriguing features, called lobate scarps, are faults created when the Moon's once-molten interior began to cool, causing the lunar surface to contract and then crinkle, they said.
这些被称为“叶状陡坡”的有趣的地貌特点是在月球一度融化的内核开端冷却的进程中形成的断层,这一进程使得月球表面产生压缩,并呈现褶皱。
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