月球撞击史

Barbara A. Cohen, Carolyn H. van der Bogert, William F. Bottke, Natalie M. Curran, Caleb I. Fassett, Harald Hiesinger, Katherine H. Joy, Sara Mazrouei, Alexander Nemchin, Gregory A. Neumann, Marc V. Norman, Nicolle E. B. Zellner
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引用次数: 6

摘要

建立绝对的月球撞击年表对于了解太阳系的早期结构、理解天体动力学和组成的演变都有重要影响。我们对太阳系内部年代学的现有理解是基于陨石坑密度和月球撞击通量率的类比。关于月球撞击史的话题已经有许多评论(例如,Hartmann 等人,2000 年;Ryder 等人,2000 年;Stöffler 等人,2006 年;Chapman 等人,2007 年;Fassett 和 Minton,2013 年;Bottke 和 Norman,2017 年;Zellner,2017 年...
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Impact History of the Moon
Establishing an absolute lunar impact chronology has important ramifications for understanding the early structure of the Solar System, to understand the evolution of both the dynamics and composition of the bodies. Our existing understanding of inner Solar System chronology is anchored to the crater density and analogy with impact flux rates on the Moon. The topic of lunar impact history has been the subject of numerous reviews (e.g., Hartmann et al. 2000; Ryder et al. 2000; Stöffler et al. 2006; Chapman et al. 2007; Fassett and Minton 2013; Bottke and Norman 2017; Zellner 2017...
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