Lithological study of mars surface by planet orbital stations and rovers

NASA rovers such as Viking 1.2; Pathfinder; Spirit; Opportunity; Phoenix; Curiosity collected and transmitted photo documents and data of the mineralogical and material composition of Martian sedimentary rocks. Analysis of the accumulated factual basis gives grounds for concluding that sedimentary rock formation on Mars, as on Earth, proceeded under the influence of gravitational, cryogenic, aeolian and fluvial factors, the interrelation between which was determined by the activity of physical and chemical weathering processes. Also meteorite and volcanic material participated in the formation of sedimentary rocks. It is possible to discover deposits of Fe, Mn, U, rare earth elements, noble metals, Cu, Pb, Zn, B, Ba, Sr, P, various salts and water on Mars. © 2020, Univelt Inc. All rights reserved.

Издательство
Univelt Inc.
Язык
Английский
Страницы
785-802
Статус
Опубликовано
Том
170
Год
2020
Организации
  • 1 Academy of Engineering, Peoples’ Friendship University of Russia (RUDN University), 6 Miklukho-Maklaya str, Moscow, 117198, Russian Federation
Ключевые слова
Chemical analysis; Lithology; Manganese removal (water treatment); Manned space flight; NASA; Orbits; Rare earths; Sedimentology; Space applications; Space platforms; Volcanic rocks; Weathering; Chemical weathering process; Mars surfaces; Material compositions; Orbital station; Volcanic materials; Water on Mars; Sedimentary rocks
Дата создания
02.11.2020
Дата изменения
02.11.2020
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/65127/
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