(Abstract) We present a two-body validation test for the candidate solutionsidentified in Paper III of this series. Simulations including bothSolution A (2. 5 M⊕, a=100 au) and Solution B (6 M⊕, a=75 au) confirm that Solution B is the dominant perturber responsible forthe Kuiper Cliff morphology, with a two-body combined score of 0. 586 (−2. 3% relative to the single-body reference). The three-bodyscenario (Erebo + Solution A + Solution B) is ruled out. The control-run anomaly (Rₘaxcontrol=0. 6446) is resolved byadopting the depletion proxy as the primary discriminant metric. SHA-256 of simulation output: 027f47017a1f32cacca31ecf8517396bda8eade3dce685d0d510c03554b5bf13. This is Paper IV of the ATMAN v5. 0 series. Author: Ariel Fernando Martini, Buenos Aires, Argentina (2026). Contact: arielₘartini₃@hotmail. com
Ariel Fernando Martini (Thu,) studied this question.