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水星构造特征及演化

闫丹 曾佐勋 胡才志 徐大良 胡烨

地质科技情报2009,Vol.28Issue(4):21-27,7.
地质科技情报2009,Vol.28Issue(4):21-27,7.

水星构造特征及演化

Tectonic Features and Evolution of Mercury

闫丹 1曾佐勋 2胡才志 3徐大良 4胡烨1

作者信息

  • 1. 中国地质大学,研究生院,武汉,430074
  • 2. 中国地质大学,地球科学学院,武汉,430074
  • 3. 中国地质大学,空间科学技术研究中心,武汉,430074
  • 4. 中国地质大学,华中构造力学研究中心,武汉,430074
  • 折叠

摘要

Abstract

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.

关键词

水星/构造特征/叶片状悬崖/Caloris盆地/构造演化史

Key words

Mercury/tectonic feature/lobate scarp/Caloris Basin/tectonic history

分类

天文与地球科学

引用本文复制引用

闫丹,曾佐勋,胡才志,徐大良,胡烨..水星构造特征及演化[J].地质科技情报,2009,28(4):21-27,7.

基金项目

国家自然科学基金项目(40874092) (40874092)

地质科技情报

OA北大核心CSCDCSTPCD

2096-8523

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