Simulating Martian regolith in the laboratory

作者：Seiferlin Karsten^*; Ehrenfreund Pascale; Garry James; Gunderson Kurt; Huetter E; Kargl Guenter; Maturilli Alessandro; Merrison Jonathan Peter

来源：Planetary and Space Science, 2008, 56(15): 2009-2025.

DOI：10.1016/j.pss.2008.09.017

• Martian soil
• Lunar soil
• Soil simulants
• JSC-1
• Salten Skov
• Thermal conductivity

Regolith and dust cover the surfaces of the Solar Systems solid bodies, and thus constitute the visible Surface of these objects. The topmost layers also interact with space or the atmosphere in the case of Mars. Venus and Titan. Surface probes have been proposed, studied and flown to some of these worlds. Landers and some of the mechanisms they carry, e.g. sampling devices, drills and subsurface probes ("moles") will interact with the porous surface layer. The absence of true extraterrestrial test materials in ample quantities restricts experiments to the use of soil or regolith analogue materials. Several standardized soil simulants have been developed and produced and are commonly Used for a variety of laboratory experiments. In this paper we intend to give in overview of some of the most important soil simulants, and describe experiments (penetrometry, thermal conductivity, acolian transport, goniometry, spectroscopy and exobiology) made in various European laboratory facilities.

• 出版日期2008-12