Interstellar Object 3I/ATLAS's Jets Linked to Non-Gravitational Acceleration

This paper builds upon previous work analyzing the jet morphology and periodic wobble of interstellar object 3I/ATLAS. The authors link observed jet position angles to the non-gravitational acceleration components in the 3D RTN frame. They compute RTN directions from heliocentric state vectors and project them onto the sky, comparing them to three persistent jets. The study estimates thrust and accelerations from HST/WFC3-UVIS F350LP net counts, accounting for uncertainties in background handling, phase-function systematics, and geometric degeneracies. The results show alignment between Jet2 and the projected transverse direction on a specific date, while Jet3 is close to the projected normal direction. Jet2 also exhibits a monotonic PA drift over time. This research provides valuable insights into the behavior of interstellar objects and the forces acting upon them. Further investigation is needed to fully understand the complex dynamics of 3I/ATLAS's jets and their relationship to its non-gravitational acceleration.

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