Fig. 7: Comparison of the isotopic composition of Ne in the lunar soil. | Communications Earth & Environment

Fig. 7: Comparison of the isotopic composition of Ne in the lunar soil.

From: Weak influence of the secondary surface processes on the regolith of Chang’E-5 landing site

Fig. 7

The (20Ne/22Ne)tr ratios of the CE-5 bulk soil seem less fractionated than those of the Apollo soils, particularly for the (20Ne/22Ne)tr ratio in ilmenite, which is very close to that of the modern solar wind, indicating that the secondary process endured by the CE-5 soils was not strong. The relatively higher 21Ne/22Ne ratios of the CE-5 soil than those of other lunar soils indicate that the sample contains a certain proportion of cosmogenic 21Ne, which may result from the longer cosmic-ray irradiation time than those of the Apollo samples. The uncertainties of (20Ne/22Ne)tr ratios in CE-5 samples are at 1σ. The data of Apollo soils are from previous reports16,17,19,22,28,31,53,54,57.

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