Planetary Simulant Database: CUG-1A China University of Geosciences

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Mineral Abundance %
Olivine 48
Glass 23
Pyroxene 20
Plagioclase 9

Bulk Chemistry

Oxide Wt.%
SiO2 48.32
TiO2 2.38
Al2O3 16.01
FeO 12.5
MnO 0.15
MgO 6.95
CaO 7.39
Na2O 0.19
K2O 2.12
P2O5 0.54
LOI 0.19
Total 99.8

Physical Properties

Property Value
Mean grain size 92 μm
Median grain size 80 μm
Specific gravity 2.88
Internal friction angle 20°
Cohesion 5-21 kPa
Simulant Name: CUG-1A Chinese University of Geosciences
Current Status: Unknown
Developed By: Chinese University of Geosciences, Wuhan
Available From: N/A
Publications: He, X. X. et al. (2010), Lunar Regolith Simulant CUG-1A. 41st Lunar and Planetary Science Conference, Abstract #1183.

CUG-1A is a geotechnical lunar mare simulant developed at the Chinese University of Geosciences at Wuhan. It is described in a single conference abstract by He et al. The simulant was made from basaltic volcanic scoria from Huinan County in northeast China and is chemically similar to Apollo 14 soils.

The scoria was ground and sieved into different size fractions that were then re-combined to achieve the desired particle size distribution. He et al. (2010) claim that several hundred kilograms were produced, but it is unclear what the current status of the simulant is.

Other Lunar Mare Simulants
ALS | ALRS-1 | BP-1 | CAS-1 | CLRS-1 | CSM-CL | CUG-1A | DNA-1 | FJS-1/2/3 | GSC-1 | JSC-1/1A/1AF/1AC/2A | KLS-1 | KOHLS-1/KAUMLS | Maryland-Sanders | MLS-1/1P | MKS-1 | NEU-1 | Oshima | TJ-1/2