Rotation Period of 3I/ATLAS After Perihelion from Jet Position Angle Wobble and Photometric Variability
Toni Scarmato, Abraham Loeb

TL;DR
This study determines the post-perihelion rotation period of comet 3I/ATLAS using jet morphology and photometric variability, revealing a rotation period of approximately 7.1 hours and jet precession.
Contribution
It introduces a dual-method approach combining jet PA wobble analysis and photometry to measure comet rotation periods post-perihelion, providing new insights into comet dynamics.
Findings
Rotation period of 7.1 hours identified
Jet precession of 20 degrees observed
Rotation axis aligned with sunward direction
Abstract
We determine the post-perihelion rotation period of 3I/ATLAS using two independent diagnostics: the temporal modulation of the position angle (PA) of a persistent jet-like feature, and a time-series photometric light curve in the Gr (R) band. For the jet morphology, we measure the PA at multiple epochs by applying the Larson-Sekanina Rotational Gradient filter to Hubble Space Telescope images between November 20, 2025 and December 27, 2025, and model the phase-folded PA curve with weighted least-squares Fourier series up to two harmonics while scanning trial periods P to identify minima in \c{hi}2(P). For the photometry, we adopt the best-fit period from an independent 30-minute binned analysis (from a 0.25 meter telescope MPC L92) based on a refined \c{hi}2(P) profile for a sinusoidal model with nightly offsets. We find that the jet-PA modulation gives a period Pjet = 7.20 +/-0.05 h…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Astrophysics and Cosmic Phenomena · Cosmology and Gravitation Theories
