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dc.contributorINAF, Osservatorio Astrofisico di Torino, Pino Torinese (TO), Italy
dc.contributorArmagh Observatory and Planetarium, Armagh, UK
dc.contributorV.N. Karazin Kharkiv National University, Kharkiv, Ukraine
dc.contributor.authorCellino, Alberto
dc.contributor.authorBagnulo, Stefano
dc.contributor.authorChristou, Apostolos
dc.contributor.authorBelskaya, Irina
dc.date.accessioned2024-02-21T11:03:25Z
dc.date.available2024-02-21T11:03:25Z
dc.date.issued2019-09-01T00:00:00Z
dc.identifier.other2019EPSC...13...89C
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/1835
dc.description.abstractWe discovered well in advance that (101955) Bennu, the target of the OSIRIS-REx space mission, had polarimetric properties that could make this object a candidate to be a comet, or a borderline object between asteroids and comets. The first results of the in situ exploration by OSIRIS-Rex fully confirm our expectations. This is a great achievement, and demonstrates that linear polarisation measurements of small bodies are a powerful tool to infer the physical properties of these bodies and to identify possible cometary characteristics.
dc.publisherEPSC-DPS Joint Meeting 2019
dc.titleThe unusual properties of (101955) Bennu, as found by OSIRIS-REx, were not unexpected
dc.typeabstract
dc.source.journalEPSC
dc.source.journalEPSC...13
dc.source.volume2019
refterms.dateFOA2024-02-21T11:03:26Z
dc.identifier.bibcode2019EPSC...13...89C


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