Related Experiment Video
Updated: May 8, 2026

Experimental Methods of Dust Charging and Mobilization on Surfaces with Exposure to Ultraviolet Radiation or Plasmas
Published on: April 3, 2018
Differences in space weathering between the near and far side of the Moon: evidence from Chang'e-6 samples
Jiarui Lin1,2,3,4, Haiyang Xian1,2,3, Yiping Yang1,2,3
1State Key Laboratory of Deep Earth Processes and Resources, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China.
Abstract:
The differences in terrain and chemical composition between the far side of the Moon (lunar farside) and the near side have been identified through remote sensing spectroscopy. The lunar farside samples returned by the Chang'e-6 mission show differences in terms of space weathering features compared to nearside samples. The studied farside samples lack vapor deposition layers found on the nearside and exhibit thinner amorphized layers, lower solar flare track densities, reduced number densities of nano phase metallic iron (npFe0) and larger npFe0 grain sizes. These findings suggest that the solar wind plays a dominant role in space weathering on the Chang'e-6 sampling site, surpassing micrometeorite impacts. This could provide critical sample-based evidence of the lunar space environment's dichotomy, enhancing our understanding of how solar wind and micrometeoroid impacts shape the lunar surface, even over short exposure periods.
Related Concept Videos
Conditions on Early Earth
Gravity between Spherical Bodies
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
Tidal Forces
Simple Harmonic Motion and Uniform Circular Motion
There is an easy way to produce simple harmonic motion by using uniform circular motion. For instance, consider a ball attached to a uniformly rotating...

