It was also able to provide insights into how the planet evolved.
The far side of the moon is of great importance due to its interesting geological formations, but this hidden side also blocks all the electromagnetic noise from human activity, making it an ideal place to build radio telescopes.
Ground penetrating radar
Orbiter radars have been used for planetary sciences since the early 2000s, but the recent Chinese and US rover missions were the first to use ground-penetrating radar on site. This ground-breaking radar is now set to become part of the scientific payload of future planetary missions, where it will be used to map the subsurface of landing sites and shed light on what is happening below the ground.
GPR has also the ability to retrieve significant information regarding the type of planetary soils and their subsurface layers. This information can be used to get an insight into the geological evolution of an area and even assess its structural stability for future planetary bases and research stations.
Perseverance and Tianwen-1 are currently active, and the first GPR images from Mars are expected to be published in 2022. But the first available planetary on-site GPR data was from the Chang'E-3, E-4 and E-5 lunar missions, where it was used to investigate the structure of surface layers of the far side of the moon, and provide valuable information about the geological evolution of the area.
Despite the benefits of GPR, one major drawback is its inability to detect layers with smooth boundaries between them. This means gradual variations from one layer to another go undetected, giving the false impression that the subsurface consists of a homogenous block, while in fact it may be a much more complex structure representing a completely different geological history.
Our team developed a new method capable of detecting these layers by using the radar signatures of hidden rocks and boulders. The newly developed tool has been used to process the GPR data captured by Chang'E-4's Yutu-2 rover which landed in the Von Kármán crater, part of the Aitken Basin at the moon's south pole.
The Aitken basin is the biggest and oldest known crater, believed to have been created by a meteoroid impact that penetrated the crust of the moon and uplifted materials from the top mantle (the interior layer just below it). Our detection tool revealed a previously unseen layered structure in the first 10m of the lunar surface, which had been understood to be one homogenous block.
Using our method, we can make more accurate estimations regarding the depth of the top surface of lunar soil, which is an important way to determine the stability and strength of the soil foundation for developing lunar bases and research stations.
This newly discovered complex layered structure also suggests that small craters are more important and may have contributed much more than previously believed to the materials deposited by meteorite strikes—and the overall evolution of lunar craters.
This means we will have a more coherent understanding of the complex geological history of our satellite, and enable us to predict more accurately what lies beneath the surface of the moon.