Author
Listed:
- S. Bagnulo
(Armagh Observatory & Planetarium)
- A. Cellino
(INAF – Osservatorio Astrofisico di Torino)
- L. Kolokolova
(University of Maryland)
- R. Nežič
(Armagh Observatory & Planetarium
University College London
University College London/Birkbeck)
- T. Santana-Ros
(Universidad de Alicante
Universitat de Barcelona (IEEC-UB))
- G. Borisov
(Armagh Observatory & Planetarium
Bulgarian Academy of Sciences)
- A. A. Christou
(Armagh Observatory & Planetarium)
- Ph. Bendjoya
(Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange)
- M. Devogèle
(University of Central Florida)
Abstract
So 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.
Suggested Citation
S. Bagnulo & A. Cellino & L. Kolokolova & R. Nežič & T. Santana-Ros & G. Borisov & A. A. Christou & Ph. Bendjoya & M. Devogèle, 2021.
"Unusual polarimetric properties for interstellar comet 2I/Borisov,"
Nature Communications, Nature, vol. 12(1), pages 1-11, December.
Handle:
RePEc:nat:natcom:v:12:y:2021:i:1:d:10.1038_s41467-021-22000-x
DOI: 10.1038/s41467-021-22000-x
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