Our knowledge about the way the highlands located on the far side of the lunar surface were formed and the possibility that they could be able to sustain a near-future human expedition is restricted due to the fact that there have been just a limited number of journeys to the moon and scientific investigations carried out there. If sufficient evidence of practically accessible water ice can be found in close proximity to certain land areas, the chance of future human settlement may increase. As a consequence of this, the objective of this research is to design a concept for a sweeping lunar penetrating radar. This radar will have six degrees of freedom, and its primary function should be to lay the groundwork for future human missions and lunar outposts. With the help of this design, it will be able to get a better knowledge of the topography of the roving region in addition to the regolith structure, layer composition, mineral, and volatile compositions, as well as the likely existence of water can be accomplished without affecting the maximum height of either the rover or the lander.