Noble Gases and Stable Isotopes Track the Origin and Early Evolution of the Venus Atmosphere

被引:13
|
作者
Avice, Guillaume [1 ]
Parai, Rita [2 ,3 ]
Jacobson, Seth [4 ]
Labidi, Jabrane [1 ]
Trainer, Melissa G. [5 ]
Petkov, Mihail P. [6 ]
机构
[1] Univ Paris Cite, Inst Phys Globe Paris, CNRS, F-75005 Paris, France
[2] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[3] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
[4] Michigan State Univ, Dept Earth & Environm Sci, E Lansing, MI 48824 USA
[5] NASA Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[6] CALTECH, Jet Prop Lab, NASA, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
关键词
Noble gases; Stable isotopes; Venus; Atmosphere; MASS-SPECTROMETER; TERRESTRIAL PLANETS; SAMPLE RETURN; MARS; FRACTIONATION; NITROGEN; XENON; WATER; COMPONENTS; HYDROGEN;
D O I
10.1007/s11214-022-00929-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The composition the atmosphere of Venus results from the integration of many processes entering into play over the entire geological history of the planet. Determining the elemental abundances and isotopic ratios of noble gases (He, Ne, Ar, Kr, Xe) and stable isotopes (H, C, N, O, S) in the Venus atmosphere is a high priority scientific target since it could open a window on the origin and early evolution of the entire planet. This chapter provides an overview of the existing dataset on noble gases and stable isotopes in the Venus atmosphere. The current state of knowledge on the origin and early and long-term evolution of the Venus atmosphere deduced from this dataset is summarized. A list of persistent and new unsolved scientific questions stemming from recent studies of planetary atmospheres (Venus, Earth and Mars) are described. Important mission requirements pertaining to the measurement of volatile elements in the atmosphere of Venus as well as potential technical difficulties are outlined.
引用
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页数:30
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