Mars and the ESA Science Programme-the case for Mars polar science

被引:1
|
作者
Thomas, Nicolas [1 ]
Becerra, P. [1 ]
Smith, I. B. [2 ]
机构
[1] Univ Bern, Physikal Inst, Sidlerstr 5, CH-3012 Bern, Switzerland
[2] York Univ, Lassonde Sch Engn, Earth & Space Sci & Engn, Toronto, ON, Canada
基金
加拿大自然科学与工程研究理事会; 瑞士国家科学基金会;
关键词
Mars; Mission; Polar caps; Dynamic processes; LAYERED DEPOSITS; ICE; CAP; STRATIGRAPHY; CLIMATE; EVOLUTION; MODEL;
D O I
10.1007/s10686-021-09760-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Current plans within the European Space Agency (ESA) for the future investigation of Mars (after the ExoMars programme) are centred around participation in the Mars Sample Return (MSR) programme led by NASA. This programme is housed within the Human and Robotic Exploration (HRE) Directorate of ESA. This White Paper, in response to the Voyage 2050 call, focuses on the important scientific objectives for the investigation of Mars outside the present HRE planning. The achievement of these objectives by Science Directorate missions is entirely consistent with ESA's Science Programme. We illustrate this with a theme centred around the study of the Martian polar caps and the investigation of recent (Amazonian) climate change produced by known oscillations in Mars' orbital parameters. Deciphering the record of climate contained within the polar caps would allow us to learn about the climatic evolution of another planet over the past few to hundreds of millions of years, and also addresses the more general goal of investigating volatile-related dynamic processes in the Solar System.
引用
收藏
页码:677 / 693
页数:17
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