Published February 22, 2026 | Version v2
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Kinematic and Thermodynamic Constraints on the Anomalous Acceleration of Interstellar Object 3I/ATLAS (C/2025 N1)

Description

ABSTRACT: We present a kinematic and thermodynamic analysis of Interstellar Object 3I/ATLAS (C/2025 N1), identifying significant deviations from standard cometary behavior. The object exhibits a non-gravitational acceleration of $3 \times 10^{-10} \text{ AU/d}^2$ aligned with a persistent, 400,000 km collimated sunward jet.

Unlike typical cometary outgassing, which is driven by isotropic surface sublimation in thermal equilibrium, the ejecta from 3I/ATLAS displays a profound thermal deficit ($T_{obs} \approx 140 \text{ K}$ vs. $T_{eq} \approx 180 \text{ K}$), implying rapid adiabatic expansion through a constricted geometry. We demonstrate that the observed collimation requires an exhaust velocity $v_{ex} > 0.5 \text{ km/s}$ to overcome solar wind dynamic pressure.

Based on recent spectroscopic data indicating a 20-fold surge in post-perihelion mass loss (January 2026), we propose a "Contained Volatile" model (an ablative propulsion mechanism utilizing a monolithic pressure vessel) that challenges the standard "rubble pile" surface sublimation hypothesis.

To rigorously test this model against natural outgassing, we derive two critical, falsifiable constraints:

  • Thermodynamic Discontinuity: Unlike natural comets which fade gradually (inverse-square law), we predict a "Step-Function" cessation of outgassing (a "Hard Stop") in April 2026.

  • Kinematic Deviation: We predict a non-gravitational inclination change ($\Delta i$) at the Jupiter periapsis (May 2026) exceeding ballistic scattering predictions.

These predictions serve as a rigorous test to distinguish between natural cometary outgassing and active, directed propulsion mechanisms.

PUBLICATION STATUS:

  • Status: Independent Pre-print (2026).

CRITICAL DISCLAIMER: This manuscript is currently an independent pre-print hosted on Zenodo and has NOT been peer-reviewed. The findings, kinematic analyses, and thermodynamic models presented herein are preliminary and subject to revision based on expert feedback. The hypothesis of an ablative propulsion mechanism remains speculative until confirmed by independent observation.

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Additional details

Related works

Is described by
Preprint: 10.5281/zenodo.18147198 (DOI)

Dates

Created
2026-02-01

References

  • Whipple, F. L. (1950). A Comet Model. I. The Acceleration of Comet Encke. The Astrophysical Journal, 111, 375.
  • Jewitt, D. (2015). Color and Activity of the Interstellar Object 1I/'Oumuamua. The Astronomical Journal, 150(6), 201.
  • Anderson, J. D. (1990). Modern Compressible Flow: With Historical Perspective. McGraw-Hill.
  • Micheli, M., et al. (2018). Non-gravitational acceleration in the trajectory of 1I/2017 U1 ('Oumuamua). Nature, 559, 223–226.