Nearly forty years after the return of the first lunar samples to Earth, improvements in laboratory detection limits made possible the first definitive discovery of magmatic water in lunar volcanic samples. The intervening decade has seen an exponential increase in the amount of data on the abundance of magmatic water, and its hydrogen isotope composition, in various rock types recovered from the Moon. Here we review these data and describe how the abundance of water in the lunar interior places important constraints on models for the high-temperature origin and evolution of the Moon.

中文翻译：

---

月球内部水的起源和演化

在第一批月球样本返回地球近四十年后，实验室检测限的改进使得在月球火山样本中首次明确发现岩浆水成为可能。在这十年间，从月球回收的各种岩石类型中，关于岩浆水丰度及其氢同位素组成的数据量呈指数级增长。在这里，我们回顾了这些数据，并描述了月球内部丰富的水如何对月球的高温起源和演化模型施加重要限制。