Comets and Asteroids

Dust Properties of the Interstellar Object 3I/ATLAS Revealed by Optical and Near-Infrared Polarimetry

By Keith Cowing
Status Report
astro-ph.EP
January 15, 2026
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Dust Properties of the Interstellar Object 3I/ATLAS Revealed by Optical and Near-Infrared Polarimetry
Polarization degree (Pr) and polarization position angle (θr) of 3I/ATLAS as a function of phase angle, measured in five bands (RC, IC, J, H, and Ks). Colored symbols denote our visible and near-infrared imaging polarimetric data obtained with different instruments, while orange symbols show previously published measurements of 3I/ATLAS (Z. Gray et al. 2025; M. Zheltobryukhov et al. 2025). Gray symbols represent polarimetric measurements of Solar System comets compiled in the Database of Comet Polarimetry (DBCP; N. Kiselev et al. 2017), and the pink triangles indicate the PPC of the interstellar comet 2I/Borisov (S. Bagnulo et al. 2021). The dashed curves show the best-fit linear–exponential models (Equation 1) to our data. — astro-ph.EP

We present independent polarimetric observations of the interstellar object 3I/ATLAS, including the first near-infrared polarimetric measurements. Using imaging polarimeters, we measured the degree of linear polarization from the visible RC band (0.64 µm) to the near-infrared Ks band (2.25 µm), and investigated its dependence on solar phase angle (polarization phase curve; PPC) and wavelength (polarization color curve; PCC).

We confirm that the PPC of 3I/ATLAS differs significantly from those of typical Solar System comets, showing an unusually large polarization amplitude. This PPC shows no significant change in the RC band across perihelion passage, despite the perihelion lying within the water snow line.

This indicates that the unusual polarimetric behavior of 3I/ATLAS is unlikely to be driven by transient volatile activity, but instead reflects intrinsic optical properties of refractory dust particles. The PCC increases with wavelength over 0.6–1.2 µm and peaks at 1.5–2.0 µm, suggesting that the dominant scattering units are dust aggregates composed of submicron-sized monomers, broadly consistent with interstellar dust and solar-system cometary aggregates.

Taken together, our results indicate that 3I/ATLAS preserves polarimetric properties characteristic of a primitive cometary planetesimal formed in another planetary system, with a refractory dust composition that differs from that typically observed among Solar System comets, despite sharing a similar size scale of the aggregate building blocks.

Seungwon Choi, Masateru Ishiguro, Jun Takahashi, Tomoki Saito, Yoonsoo P. Bach, Bumhoo Lim, Hiroyuki Naito, Jooyeon Geem, Sunho Jin, Jinguk Seo, Hyeonwoo Ju, Hiroshi Akitakya, Koji S. Kawabata, Mahito Sasada, Kazuya Doi, Hisayuki Kubota, Seiko Takagi, Makoto Watanabe, Tomohiko Sekiguchi, Myungshin Im

Comments: 11 pages, 4 Figures, 3 Tables
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2601.08591 [astro-ph.EP] (or arXiv:2601.08591v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2601.08591
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Submission history
From: Masateru Ishiguro
[v1] Tue, 13 Jan 2026 14:20:18 UTC (215 KB)
https://arxiv.org/abs/2601.08591

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