Water in the Solar System

被引：4

作者：

Litvak, M. L. ^{[1
]}

Sanin, A. B. ^{[1
]}

机构：

[1] Russian Acad Sci, Space Res Inst, Ul Profsoyuznaya 84-32, Moscow 117997, Russia

来源：

PHYSICS-USPEKHI | 2018年 / 61卷 / 08期

关键词：

water; water ice; oceans; Solar System; terrestrial planets; giant planets and their moons; SCIENCE LABORATORY MISSION; NEUTRONS DAN EXPERIMENT; GIANT PLANET FORMATION; INTERIOR STRUCTURE; CLOUD STRUCTURE; POLAR-REGIONS; GALE CRATER; EARLY MARS; GLOBAL DISTRIBUTION; DYNAMIC ALBEDO;

D O I：

10.3367/UFNe.2017.04.038277

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Over the past half century, numerous research space missions have been launched to explore various objects in the Solar System, primarily to find surface or subsurface water or water ice (in particular, to discover extraterrestrial oceans or their traces and to study their evolution in light of Earth's hydrospheric history). This paper briefly reviews the subject with an emphasis on the terrestrial planets to find out why it is that, while liquid water oceans once formed and still exist on Earth, the surfaces of other planets turned into arid deserts. Also reviewed are issues related to the origin and observation of water ice in the outer part of the Solar System. A list of important problems related to the water origin and spreading in the Solar System is presented.

引用

页码：779 / 792

页数：14

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