Analysis on Mars Exploration for the Prospect of Future Mars Migration Plan and Society Development

DOI

10.2991/assehr.k.220105.181How to use a DOI?

Keywords

exploration of Mars; Mars migration program; Martian surface

Abstract

Mars is the planet which is the closest to the earth in the solar system, humans have never stopped exploring its topography, soil characteristics and resource composition. Different from the earth-moon exploration, there are still some difficulties in the exploration of Mars. The planet’s orbital period of the earth and Mars is different, so the mission available period is limited, the distance of the ground fire is between 56 trillion and 400 million, so there is weaker solar radiation and thinner atmosphere. The long-distance journey will not only increase the delay of radio transmission and lengthen the exploration period, but also make the human mission to Mars need to consider the consumption of resources and other issues. This paper will introduce the differences and difficulties between Mars exploration and Earth-moon exploration from the motion law, distance of Earth to Mars, solar radiation and atmospheric environment. It focuses on the study of geological structure, soil and water ice, material composition and environment. It also list the lack and difficulty in data, long-distance travel and continually supply for Mars exploration. Finally, this paper analyzes and integrates Mars-related materials to provide theoretical guidance and solutions for future Mars exploration and immigration.

Copyright

© 2022 The Authors. Published by Atlantis Press SARL.

Open Access

This is an open access article under the CC BY-NC license.

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TY  - CONF
AU  - Yueyang Zhang
PY  - 2022
DA  - 2022/01/17
TI  - Analysis on Mars Exploration for the Prospect of Future Mars Migration Plan and Society Development
BT  - Proceedings of the 2021 International Conference on Social Development and Media Communication (SDMC 2021)
PB  - Atlantis Press
SP  - 981
EP  - 985
SN  - 2352-5398
UR  - https://doi.org/10.2991/assehr.k.220105.181
DO  - 10.2991/assehr.k.220105.181
ID  - Zhang2022
ER  -