We consider the system consisting of the plasma environment in the Low Earth Orbital (LEO) region in presence of charged space debris objects. This system is modelled for the first time as a weakly coupled dusty plasma; where the charged space debris objects are treated as weakly coupled dust particles with two dimensional space and time dependences. The dynamics of dust ion acoustic waves in the system is found to be governed by a forced Kadomtsev-Petviashvili (KP) type model equation, where the forcing term depends on the distribution of debris objects. Accelerated planar solitary wave solutions are obtained from the forced KP equation upon transferring the frame of reference, and applying a specific non holonomic constraint condition. For a different constraint condition, the forced KP equation also admits lump wave solutions. The dynamics of accelerated lump wave solutions, which are happened to be pinned, is also explored. Approximate dust ion acoustic wave solutions for different types of localized space debris or forcing functions are analysed using different perturbation methods. Our work provides a much clearer insight of the debris dynamics in the plasma medium in the LEO region, revealing some novel results that are immensely helpful for various space missions by space agencies in the world. Different perspectives for practical applications of our theoretical results are discussed in detail.