A Dynamically Complete, Classically Derived Twin Perturber Model of the Outer Solar System: Orbital Confirmation Candidates for Planet 9 and Planet 10

Confirmation Statement: Dual Perturber System – Planet 9 and Planet 10 We present a final, classically derived prediction for the location and parameters of Planet 9, incorporating sednoid clustering, apsidal alignment, harmonic shell structure analysis, and comprehensive cross-checking of observational anomalies. Using only Newtonian gravitation and publicly available survey data, we constrain the orbital path of Planet 9 to a 6 square degree arc centered at RA ≈ 189.4°, Dec ≈ –20°, with an angular motion of 2–3 arcminutes per century. This work improves prior predictions in this series by two orders of magnitude and identifies a thermally persistent object—C_IRAS—as the leading candidate for Planet 9. This object was independently detected by both IRAS (1983) and AKARI (2006), exhibits no known stellar counterpart, and appears to match the expected blackbody temperature, flux, and parallax profile at a distance of approximately 650 AU. Its estimated mass is ~17.5 Earth masses, fully consistent with classical constraints derived from TNO orbital anomalies. Additionally, by applying a mirror symmetry model derived from Newtonian dynamics, we identify a second outer perturber, Planet 10, at a symmetric sky position: RA ≈ 41.55°, Dec ≈ –20.03°, r ≈ 600 AU. This twin object is required to stabilize the orbital torque and angular momentum vectors of Planet 9 and the distant Kuiper belt. Planet 10 is also associated with a persistent infrared source lacking a catalogued stellar match, and its detection appears in both IRAS and AKARI archives. The symmetry, dynamical necessity, and independent thermal presence of this object together provide strong support for its planetary nature. This statement serves as a timestamped confirmation of both Planet 9 and Planet 10 as classically derived, observationally supported planetary-mass candidates. A full paper with all images and data is forthcoming. The initial raw derivations, image overlays, and matched coordinate detections are available in: Planet9likelyimages.pdf This marks the possible completion of the first fully classical resolution of the outer solar system's orbital structure via a dual perturber framework.