Extreme Negative Polarization of New Interstellar Comet 3I/ATLAS

dc.contributor.authorGray, Zuri
dc.contributor.authorBagnulo, Stefano
dc.contributor.authorBorisov, Galin
dc.contributor.authorKwon, Yuna G.
dc.contributor.authorCellino, Alberto
dc.contributor.authorKolokolova, Ludmilla
dc.contributor.authorDorsey, Rosemary C.
dc.contributor.authorFedorets, Grigori
dc.contributor.authorGranvik, Mikael
dc.contributor.authorMaclennan, Eric
dc.contributor.authorMuñoz, Olga
dc.contributor.authorBendjoya, Philippe
dc.contributor.authorDevogèle, Maxime
dc.contributor.authorIeva, Simone
dc.contributor.authorPenttilä, Antti
dc.contributor.authorMuinonen, Karri
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.converis.publication-id504950666
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/504950666
dc.date.accessioned2026-01-21T15:00:03Z
dc.date.available2026-01-21T15:00:03Z
dc.description.abstract<p>We present the first polarimetric observations of the third discovered interstellar object (ISO), 3I/ATLAS (C/2025 N1, or 3I), obtained preperihelion with FORS2 at the Very Large Telescope, ALFOSC at the Nordic Optical Telescope, and FoReRo2 at the 2 m Ritchey-Chrétien-Coudé telescope, over a phase angle range of 77–224. This marks the second-ever polarimetric study of an ISO, the first distinguishing 2I/Borisov from most solar system comets by its higher positive polarization. Our polarimetric measurements as a function of phase angle reveal that 3I is characterized by a deep and narrow negative polarization branch, reaching a minimum value of −2.7% at phase angle 7<sup>∘</sup>, and an inversion angle of 17<sup>∘</sup>—a combination unprecedented among asteroids and comets, including 2I/Borisov. At very small phase angles, the extrapolated slope of the polarization phase curve is consistent with that of certain small trans-Neptunian objects and Centaur Pholus, consistent with independent spectroscopic evidence for a red, possibly water-ice-bearing object. Imaging confirms a diffuse coma present from our earliest observations, though no strong polarimetric features are spatially resolved. These findings may demonstrate that 3I represents a distinct type of comet, expanding the diversity of known interstellar bodies.</p>
dc.identifier.eissn2041-8213
dc.identifier.jour-issn2041-8205
dc.identifier.olddbid213978
dc.identifier.oldhandle10024/196996
dc.identifier.urihttps://www.utupub.fi/handle/11111/56198
dc.identifier.urlhttps://doi.org/10.3847/2041-8213/ae0c08
dc.identifier.urnURN:NBN:fi-fe202601216363
dc.language.isoen
dc.okm.affiliatedauthorFedorets, Grigori
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherInstitute of Physics Publishing
dc.publisher.countryUnited Kingdomen_GB
dc.publisher.countryBritanniafi_FI
dc.publisher.country-codeGB
dc.relation.articlenumberL29
dc.relation.doi10.3847/2041-8213/ae0c08
dc.relation.ispartofjournalAstrophysical Journal Letters
dc.relation.issue2
dc.relation.volume992
dc.source.identifierhttps://www.utupub.fi/handle/10024/196996
dc.titleExtreme Negative Polarization of New Interstellar Comet 3I/ATLAS
dc.year.issued2025

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