[astro-ph.EP] We present new post-perihelion polarimetric observations of the third discovered interstellar object, 3I/ATLAS (C/2025 N1; hereafter 3I), obtained using FORS2 at the Very Large Telescope, ALFOSC at the Nordic Optical Telescope, and FoReRo2 at the 2 m Ritchey-Chrétien-Coudé telescope.
The observations span phase angles 1-30∘, providing the most extensive polarimetric phase angle coverage obtained for an interstellar object to date. The post-perihelion measurements reveal that the unusual polarimetric properties of 3I persist across perihelion and match recent independent post-perihelion observations, indicating no significant evolution in the polarimetric properties.
The increased phase angle coverage allowed us to further constrain the minimum polarisation to −2.9% at phase angle 5.5∘. Multi-band BVRI observations reveal a wavelength dependence of polarisation, with the negative polarisation branch becoming deeper and shifted toward smaller phase angles at longer wavelengths. The polarimetric colour is predominantly red and increases with phase angle, consistent with behaviour observed in other comets.
Imaging and polarimetric maps show a substantially more extended coma after perihelion, while the polarisation distribution itself remains smooth and spatially homogeneous.
Numerical modelling suggests that the unusually deep polarisation phase curve originates from moderately porous dust aggregates consisting of weakly absorbing sub-micron monomers, resulting in much brighter dust than that in typical solar system comets.
Zuri Gray, Galin Borisov, Ludmilla Kolokolova, Johannes Markkanen, Yuna G. Kwon, Stefano Bagnulo, Alberto Cellino, Rosemary C. Dorsey, Grigori Fedorets, Mikael Granvik, Eric MacLennan, Antti Penttilä, Karri Muinonen, Olga Muñoz, Philippe Bendjoya, Maxime Devogèle, Simone Ieva, Francisco J. García-Izquierdo
Comments: 19 pages, 8 figures
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Astrophysics of Galaxies (astro-ph.GA)
Cite as: arXiv:2609.04932 [astro-ph.EP] (or arXiv:2609.04932v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2609.04932
Focus to learn more
Submission history
From: Zuri Gray
[v1] Fri, 4 Sep 2026 09:33:08 UTC (1,938 KB)
https://arxiv.org/abs/2609.04932
Astrobiology
