4.7 Article

Preparation and characterization of Martian soil simulant NEU Mars-1

Journal

Publisher

ELSEVIER
DOI: 10.1016/S1003-6326(19)65193-9

Keywords

Martian soil; stimulant; volcanic rock; basalt; in-situ resource utilization

Funding

  1. National Key R&D Program of China [2017YFC0805100]
  2. Guangxi Innovation-driven Development Program, China [GUIKE AA18118030]
  3. Fundamental Research Funds for the Central Universities, China [N172502003]

Ask authors/readers for more resources

To develop Martian soil simulant, basalts of the Chahar volcanic group in Wulanchabu, Inner Mongolia, China were selected as the simulant initial materials, which were ground and sorted to a predetermined particle size ratio, and small amounts of magnetite and hematite were added. The main phases of NEU Mars-1 simulant were plagioclase, augite and olivine. The glass transition and crystallization temperatures of NEU Mars-1 were 547.8 and 795.7 degrees C, respectively. The complex dielectric constant, magnetic conductivity (0.99-1.045), and dielectric loss tangent angles (0.0025-0.030) of NEU Mars-1 were all stable in the frequency range of 2-18 GHz. Mossbauer spectroscopy results showed that the mass ratio of Fe2+ to Fe3+ in the simulant was 77.6:22.4. The NEU Mars-1 Martian soil simulant demonstrated particle size ratio, chemical composition, phase composition, thermal stability, and dielectric property similar to Martian soil, and can be used as the substitute material to extract oxygen and metals with in-situ resource utilization technologies.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available