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海王星探测:稀有气体和挥发分分析

SMITH Thomas 贺怀宇 刘冉冉

深空探测学报(中英文)2020,Vol.7Issue(6):584-604,21.
深空探测学报(中英文)2020,Vol.7Issue(6):584-604,21.DOI:10.15982/j.issn.2096-9287.2020.20200057

海王星探测:稀有气体和挥发分分析

The Exploration of Neptune:A Noble Gas and Volatile Perspective

SMITH Thomas 1贺怀宇 2刘冉冉1

作者信息

  • 1. 中国科学院地质与地球物理研究所岩石圈演化国家重点实验室,北京 100029
  • 2. 中国科学院大学地球与行星科学学院,北京 100049
  • 折叠

摘要

Abstract

Most of the probes visiting other bodies in our Solar system only focused,due to technical shortcomings,on the exploration of the closer planets and planetary bodies and/or their natural satellites,i.e. Mercury,Venus,the Moon,Mars,and Jupiter,the comet 67P/Churyumov-Gerasimenko,or the 25143 Itokawa near-Earth asteroid. At present time,no specific missions to one of the two ice giants of our Solar System,Uranus and Neptune,has been planned. Our knowledge of Uranus and Neptune is,therefore,so far restricted to the data which have been collected during the flyby of the Voyager 2 mission,in January 1986 and August 1989,respectively,and to observations with the Hubble Space Telescope and the Keck Telescope. Ice giants are,in our galaxy,thought to be much more abundant than gas giant planets such as Jupiter or Saturn,therefore a better knowledge of ice giants is essential for our understanding of exoplanet candidates. Among other scientific goals,the atmospheric composition of ice giants,with a particular emphasis on their noble gas and volatile distribution,is of great significance,and can constrain models about their formation and evolution. In this review,we report,in a first part,the volatile inventories and the measurements in the planetary bodies of our Solar System;in a second part,we will discuss the scientific background about the concentration, distribution,and evolution of noble gases and volatiles in Uranus and Neptune,and finally describe a possible scenario of a future interstellar probe visiting one of the two ice giants as well as the feasibility of such a space mission,in term of payloads selection and mission profile. We will as well briefly evoke the possibility of using an ion trap mass spectrometer,a potential payload for the ice giant atmospheric exploration,onboard a Chinese interstellar mission to the outer Solar system.

关键词

冰巨行星/海王星/挥发分/稀有气体/同位素比值/质谱仪/进入探测器

Key words

ice giants/Neptune/volatiles/noble gases/isotopic ratios/mass spectrometry/entry probe

分类

天文与地球科学

引用本文复制引用

SMITH Thomas,贺怀宇,刘冉冉..海王星探测:稀有气体和挥发分分析[J].深空探测学报(中英文),2020,7(6):584-604,21.

基金项目

中国科学院国家重点实验室岩石圈演化资助项目(SKL-K201802) (SKL-K201802)

民用航天预研资助项目(D020302)The work of Thomas Smith is supported through the Chinese Academy of Sciences "President's International Fellowship Initiative"(PIFI). (D020302)

深空探测学报(中英文)

OA北大核心CSCDCSTPCD

2096-9287

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