岩浆演化 I:月球的最初分化

Amy M. Gaffney, Juliane Gross, Lars E. Borg, Kerri L. Donaldson Hanna, David S. Draper, Nick Dygert, Lindy T. Elkins-Tanton, Kelsey B. Prissel, Tabb C. Prissel, Edgar S. Steenstra, Wim van Westrenen
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引用次数: 6

摘要

在本章中,我们将详细介绍和讨论目前在了解月球原始分化过程方面取得的新进展。本章重点介绍四种研究途径:1)遥感任务产生的数据和观测结果;2)岩浆海洋结晶过程的实验研究;3)岩浆海洋过程的物理化学建模;4)月球分异的年代学约束。过去十五年来完成的研究成果为继续检验月球岩浆海洋(LMO)假说提供了依据。尽管最近的许多研究工作为月球岩浆海洋的形成过程提供了限制,但这些研究工作也为月球岩浆海洋假说提供了新的证据。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magmatic Evolution I: Initial Differentiation of the Moon
In this chapter, we present and discuss in detail current and novel advances in our understanding of the processes that drove primordial differentiation of the Moon. This chapter focuses on four avenues of study: 1) data and observations generated from remote sensing missions, 2) experimental investigations of magma ocean crystallization processes, 3) physiochemical modeling of magma ocean processes, and 4) chronological constraints on lunar differentiation. Investigations completed over the past decade and a half provide results that allow for continued testing of the lunar magma ocean (LMO) hypothesis. Although much of the recent work provides constraints on the processes that...
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