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dc.contributorArmagh Observatory & Planetarium, College Hill, Armagh, UK
dc.contributorINAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
dc.contributorDepartment of Astronomy, University of Maryland, College Park, MD, US
dc.contributorArmagh Observatory & Planetarium, College Hill, Armagh, UK; Mullard Space Science Laboratory, Department of Space & Climate Physics, University College London, Dorking, Surrey, UK; Centre for Planetary Sciences, University College London/Birkbeck, London, UK
dc.contributorDepartamento de Fisica, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, Alicante, Spain; Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB), Barcelona, Spain
dc.contributorArmagh Observatory & Planetarium, College Hill, Armagh, UK; Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences, Sofia, Bulgaria
dc.contributorUniversité Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France
dc.contributorArecibo Observatory, University of Central Florida, Arecibo, PR, USA
dc.contributor.authorBagnulo, S.
dc.contributor.authorCellino, A.
dc.contributor.authorKolokolova, L.
dc.contributor.authorNežič, R.
dc.contributor.authorSantana-Ros, T.
dc.contributor.authorBorisov, G.
dc.contributor.authorChristou, A. A.
dc.contributor.authorBendjoya, Ph.
dc.contributor.authorDevogèle, M.
dc.date.accessioned2024-02-21T11:02:04Z
dc.date.available2024-02-21T11:02:04Z
dc.date.issued2021-01-01T00:00:00Z
dc.identifier.doi10.1038/s41467-021-22000-x
dc.identifier.other10.1038/s41467-021-22000-x
dc.identifier.other2021NatCo..12.1797B
dc.identifier.other0000-0002-7156-8029
dc.identifier.other0000-0002-6645-334X
dc.identifier.other-
dc.identifier.other0000-0001-5992-5612
dc.identifier.other0000-0002-0143-9440
dc.identifier.other0000-0002-4516-459X
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1629
dc.description.abstractSo far, only two interstellar objects have been observed within our Solar System. While the first one, 1I/`Oumuamua, had asteroidal characteristics, the second one, 2I/Borisov, showed clear evidence of cometary activity. We performed polarimetric observations of comet 2I/Borisov using the European Southern Observatory Very Large Telescope to derive the physical characteristics of its coma dust particles. Here we show that the polarization of 2I/Borisov is higher than what is typically measured for Solar System comets. This feature distinguishes 2I/Borisov from dynamically evolved objects such as Jupiter-family and all short- and long-period comets in our Solar System. The only object with similar polarimetric properties as 2I/Borisov is comet C/1995 O1 (Hale-Bopp), an object that is believed to have approached the Sun only once before its apparition in 1997. Unlike Hale-Bopp and many other comets, though, comet 2I/Borisov shows a polarimetrically homogeneous coma, suggesting that it is an even more pristine object.
dc.publisherNature Communications
dc.titleUnusual polarimetric properties for interstellar comet 2I/Borisov
dc.typearticle
dc.source.journalNatCo
dc.source.journalNatCo..12
dc.source.volume12
refterms.dateFOA2024-02-21T11:02:05Z
dc.identifier.bibcode2021NatCo..12.1797B


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